NormalizeHEADmain

96 files changed, 17 insertions, 8598 deletions

diff --git a/.gitattributes b/.gitattributes
new file mode 100644
index 0000000..d7b82bc
--- /dev/null
+++ b/.gitattributes
@@ -0,0 +1,4 @@
+*.txt text eol=lf
+*.htm text eol=lf
+*.html text eol=lf
+*.md text eol=lf
diff --git a/LICENSE.txt b/LICENSE.txt
new file mode 100644
index 0000000..6312041
--- /dev/null
+++ b/LICENSE.txt
@@ -0,0 +1,11 @@
+This eBook, including all associated images, markup, improvements,
+metadata, and any other content or labor, has been confirmed to be
+in the PUBLIC DOMAIN IN THE UNITED STATES.
+
+Procedures for determining public domain status are described in
+the "Copyright How-To" at https://www.gutenberg.org.
+
+No investigation has been made concerning possible copyrights in
+jurisdictions other than the United States. Anyone seeking to utilize
+this eBook outside of the United States should confirm copyright
+status under the laws that apply to them.
diff --git a/README.md b/README.md
new file mode 100644
index 0000000..04bd515
--- /dev/null
+++ b/README.md
@@ -0,0 +1,2 @@
+Project Gutenberg (https://www.gutenberg.org) public repository for
+eBook #52838 (https://www.gutenberg.org/ebooks/52838)
diff --git a/old/52838-0.txt b/old/52838-0.txt
deleted file mode 100644
index 17dca7e..0000000
--- a/old/52838-0.txt
+++ /dev/null
@@ -1,4175 +0,0 @@
-The Project Gutenberg EBook of Creation of the Teton Landscape, by 
-J. D. Love and John C. Reed
-
-This eBook is for the use of anyone anywhere in the United States and most
-other parts of the world at no cost and with almost no restrictions
-whatsoever.  You may copy it, give it away or re-use it under the terms of
-the Project Gutenberg License included with this eBook or online at
-www.gutenberg.org.  If you are not located in the United States, you'll have
-to check the laws of the country where you are located before using this ebook.
-
-Title: Creation of the Teton Landscape
-       The Geologic Story of Grand Teton National Park
-
-Author: J. D. Love
-        John C. Reed
-
-Release Date: August 18, 2016 [EBook #52838]
-
-Language: English
-
-Character set encoding: UTF-8
-
-*** START OF THIS PROJECT GUTENBERG EBOOK CREATION OF THE TETON LANDSCAPE ***
-
-
-
-
-Produced by Stephen Hutcheson, Dave Morgan and the Online
-Distributed Proofreading Team at http://www.pgdp.net
-
-
-
-
-
-
-    View west toward Grand Teton on skyline. Hedrick’s Pond surrounded
-    by “knob and kettle” topography is in foreground, tree-covered
-    Burned Ridge moraine is in middle distance, and extending from it to
-    foot of mountains is gray flat treeless glacial outwash plain.
-    _National Park Service photo by W. E. Dilley._
-
-    [Illustration: View west up Cascade Canyon, with north face of Mt.
-    Owen in center. _National Park Service photo by H. D. Pownall._]
-
-              _To Fritiof M. Fryxell, geologist, teacher,
-          writer, mountaineer, and the first ranger-naturalist
-                     in Grand Teton National Park._
-
-                 _All who love and strive to understand
-             the Teton landscape follow in his footsteps._
-
-
-
-
-                            _CREATION OF THE
-                            TETON LANDSCAPE_
-                         The Geologic Story of
-                       Grand Teton National Park
-
-
-                                  _By
-                    J. D. LOVE AND JOHN C. REED, JR.
-                        U.S. Geological Survey_
-
-           _Library of Congress Catalogue Card No._: 68-20628
-                          _ISBN_ O-931895-08-1
-
-                              1st Edition
-                                  1968
-
-                          1st Revised Edition
-                                  1971
-
-                             Reprinted 1979
-                             Reprinted 1984
-                             Reprinted 1989
-
-                Grand Teton Natural History Association
-                          Moose, Wyoming 83012
-
-
-
-
-                                CONTENTS
-
-
-  Foreword                                                         6
-  THE STORY BEGINS                                                 8
-      First questions, brief answers                               9
-      An extraordinary story                                      10
-      An astronaut’s view                                         12
-      A pilot’s view                                              14
-      A motorist’s view                                           15
-          View north                                              15
-          View west                                               18
-          View south                                              19
-      A mountaineer’s view                                        20
-  CARVING THE RUGGED PEAKS                                        24
-      Steep mountain slopes—the perpetual battleground            24
-      Rock disintegration and gravitational movement              24
-      Running water cuts and carries                              26
-      Glaciers scour and transport                                28
-      Effects on Jackson Hole                                     30
-  MOUNTAIN UPLIFT                                                 36
-      Kinds of mountains                                          36
-      Anatomy of faults                                           38
-      Time and rate of uplift                                     40
-      Why are mountains here?                                     41
-      The restless land                                           43
-  ENORMOUS TIME AND DYNAMIC EARTH                                 45
-      Framework of time                                           45
-      Rocks and relative age                                      45
-      Fossils and geologic time                                   46
-      Radioactive clocks                                          47
-      The yardstick of geologic time                              48
-  PRECAMBRIAN ROCKS—THE CORE OF THE TETONS                        51
-      Ancient gneisses and schists                                51
-      Granite and pegmatite                                       55
-      Black dikes                                                 58
-      Quartzite                                                   63
-      A backward glance                                           64
-      The close of the Precambrian—end of the beginning           64
-  THE PALEOZOIC ERA—TIME OF LONG-VANISHED SEAS AND THE DEVELOPMENT
-          OF LIFE                                                 66
-      The Paleozoic sequence                                      66
-      Alaska Basin—site of an outstanding rock and fossil record  66
-      Advance and retreat of Cambrian seas; an example            69
-      Younger Paleozoic formations                                74
-  THE MESOZOIC—ERA OF TRANSITION                                  79
-      Colorful first Mesozoic strata                              79
-      Drab Cretaceous strata                                      81
-      Birth of the Rocky Mountains                                82
-  TERTIARY—TIME OF MAMMALS, MOUNTAINS, LAKES, AND VOLCANOES       86
-      Rise and burial of mountains                                88
-      The first big lake                                          92
-      Development of mammals                                      95
-      Volcanoes                                                   98
-  QUATERNARY—TIME OF ICE, MORE LAKES, AND CONTINUED CRUSTAL
-          DISTURBANCE                                            102
-      Hoback normal fault                                        103
-      Volcanic activity                                          103
-      Preglacial lakes                                           104
-      The Ice Age                                                105
-      Modern glaciers                                            112
-  THE PRESENT AND THE FUTURE                                     113
-  APPENDIX                                                       115
-      Acknowledgements                                           115
-      Selected references—if you wish to read further            116
-      About the authors                                          117
-      Index of selected terms and features                       118
-
-
-
-
-                                   _FOREWORD_
-
-
-Geology is the science of the Earth—the study of the forces, processes,
-and past life that not only shape our land but influence our daily lives
-and our Nation’s welfare. This booklet, prepared by two members of the
-U.S. Geological Survey, discusses how geologic phenomena are responsible
-for the magnificent scenery of the Teton region.
-
-Recognition of the complex geologic history of our Earth is vital to the
-enjoyment and appreciation of beautiful landscapes and other natural
-wonders, to the planning of our cities and highway systems, to the wise
-use of our water supplies, to the study of earthquake and landslide
-areas, to the never-ending search for new mineral deposits, and to the
-conservation and development of our known natural resources. Who can
-say, in the long run, which of the many uses of this knowledge is the
-most compelling reason to seek an understanding of the Earth?
-
-    [Illustration: Signature]
-
-                                                W. T. Pecora, _Director_
-                                                  U.S. Geological Survey
-
-        _This booklet is based on geologic investigations by the
- U. S. Geological Survey in cooperation with the National Park Service,
-                     U. S. Department of Interior._
-
-  “_Something hidden. Go and find it.
-  Go and look behind the Ranges—
-  Something lost behind the Ranges.
-  Lost and waiting for you. Go._”
-                                                  KIPLING—_THE EXPLORER_
-
-
-
-
-                            THE STORY BEGINS
-
-
-The Teton Range is one of the most magnificent mountain ranges on the
-North American Continent. Others are longer, wider, and higher, but few
-can rival the breath-taking alpine grandeur of the eastern front of the
-Tetons. Ridge after jagged ridge of naked rock soar upward into the
-western sky, culminating in the towering cluster of peaks to which the
-early French voyageurs gave the name “_les Trois Tetons_” (the three
-breasts). The range hangs like a great stone wave poised to break across
-the valley at its base. To the south and east are lesser mountains,
-interesting and scenic but lacking the magic appeal of the Tetons.
-
-This is a range of many moods and colors: stark and austere in morning
-sun, but gold and purple and black in the softly lengthening shadows of
-afternoon; somber and foreboding when the peaks wrap themselves in the
-tattered clouds of an approaching storm, but tranquil and ethereal blue
-and silver beneath a full moon.
-
-These great peaks and much of the floor of the valley to the east,
-_Jackson Hole_ (a _hole_ was the term used by pioneer explorers and
-mountain men to describe any open valley encircled by mountains), lie
-within Grand Teton National Park, protected and preserved for the
-enjoyment of present and future generations. Each year more than 3
-million visitors come to the park. Many pause briefly and pass on.
-Others stay to explore its trails, fish its streams, study the plants
-and wildlife that abound within its borders, or to savor the colorful
-human history of this area.
-
-Most visitors, whatever their interests and activities, are probably
-first attracted to the park by its unsurpassed mountain scenery. The
-jagged panorama of the Tetons is the backdrop to which they may turn
-again and again, asking questions, seeking answers. How did the
-mountains form? How long have they towered into the clouds, washed by
-rain, riven by frost, swept by wind and snow? What enormous forces
-brought them forth and raised them skyward? What stories are chronicled
-in their rocks, what epics chiseled in the craggy visage of this
-mountain landscape? Why are the Tetons different from other mountains?
-
-
-                     First questions, brief answers
-
-_How did the Tetons and Jackson Hole form?_ They are both tilted blocks
-of the earth’s crust that behaved like two adjoining giant trapdoors
-hinged so that they would swing in opposite directions. The block on the
-west, which forms the Teton Range, was hinged along the Idaho-Wyoming
-State line; the eastern edge was uplifted along a fault (a fracture
-along which displacement has occurred). This is why the highest peaks
-and steepest faces are near the east margin of the range. The hinge line
-of the eastern block, which forms Jackson Hole, was in the highlands to
-the east. The western edge of the block is downdropped along the fault
-at the base of the Teton Range. As a consequence, the floor of Jackson
-Hole tilts westward toward the Tetons (see cross section inside back
-cover).
-
-_When did the Tetons and Jackson Hole develop the spectacular scenery we
-see today?_ The Tetons are the youngest of all the mountain ranges in
-the Rocky Mountain chain. Most other mountains in the region are at
-least 50 million years old but the Tetons are less than 10 million and
-are still rising. Jackson Hole is of the same age and is still sinking.
-The Teton landscape is the product of many earth processes, the most
-recent of which is cutting by water and ice. Within the last 15,000
-years, ice sculpturing of peaks and canyons and impounding of glacial
-lakes have added finishing touches to the scenic beauty.
-
-_Why did the Tetons rise and Jackson Hole sink?_ For thousands of years
-men have wondered about the origin of mountains and their speculations
-have filled many books. Two of the more popular theories are: (1)
-continental drift (such as South America moving away from Africa), with
-the upper lighter layer of the earth’s crust moving over the lower
-denser layer and wrinkling along belts of weakness; and (2) convection
-currents within the earth, caused by heat transfer, resulting in linear
-zones of wrinkling, uplift, and collapse.
-
-These concepts were developed to explain the origin of mountainous areas
-hundreds or thousands of miles long but they do not answer directly the
-question of why the Tetons rose and Jackson Hole sank. As is discussed
-in the chapter on mountains, it is probable that semifluid rock far
-below the surface of Jackson Hole flowed north into the Yellowstone
-Volcanic Plateau-Absaroka Range volcanic area, perhaps taking the place
-of the enormous amount of ash and lava blown out of volcanoes during the
-last 50 million years. The origin of the line of weakness that marks the
-Teton fault along the east face of the Teton Range may go back to some
-unknown inequality in the earth’s composition several billion years ago.
-Why it suddenly became active late in the earth’s history is an
-unanswered question.
-
-The ultimate source of heat and energy that caused the mountains and
-basins to form probably is disintegration of radioactive materials deep
-within the earth. The Tetons are a spectacular demonstration that the
-enormous energy necessary to create mountains is not declining, even
-though our planet is several billion years old.
-
-
-                         An extraordinary story
-
-Visitors whose curiosity is whetted by this unusual and varied panorama
-are not satisfied with only a few questions and answers. They sense that
-here for the asking is an extraordinary _geologic_ (_geo_—earth;
-_logic_—science) story. With a little direction, many subtle features
-become evident—features that otherwise might escape notice. Here, for
-example, is a valley with an odd U-shape. There is a sheer face
-crisscrossed with light- and dark-colored rocks. On the valley floor is
-a tuft of pine trees that seem to be confined to one particular kind of
-rock. On the rolling hills is a layer of peculiar white soil—the only
-soil in which coyote dens are common. All these are geologically
-controlled phenomena. In short, with a bit of initial guidance, the
-viewer gains an ability to observe and to understand so much that the
-panorama takes on new depth, vividness, and excitement. It changes from
-a flat, two-dimensional picture to a colorful multi-dimensional exhibit
-of the earth’s history.
-
-    [Illustration: Figure 1. _The Tetons from afar—an astronaut’s view
-    of the range and adjacent mountains, basins, and plateaus. Width of
-    area shown in photo is about 100 miles. Stippled pattern marks
-    boundary of Grand Teton National Park._]
-
-    [Illustration: Figure 2. _Sketch of the Teton Range and Jackson
-    Hole, southwest view. Drawing by J. R. Stacy._
-
-    BLOCK DIAGRAM VIEW SOUTHWEST SHOWING THE TETON RANGE AND JACKSON
-    HOLE]
-
-
-                          An astronaut’s view
-
-The Tetons are a short, narrow, and high mountain range, distinctive in
-the midst of the great chain of the Rocky Mountains, the backbone of
-western North America. Figure 1 shows how the Tetons and their
-surroundings might appear if you viewed them from a satellite at an
-altitude of perhaps a hundred miles. The U. S. Geological Survey
-topographic map of Grand Teton National Park shows the names of many
-features not indicated on figure 1 or on the geologic map inside the
-back cover. The Teton Range is a rectangular mountain block about 40
-miles long and 10-15 miles wide. It is flanked on the east and west by
-flat-floored valleys. Jackson Hole is the eastern one and Teton Basin
-(called Pierre’s Hole by the early trappers) is the western.
-
-The Teton Range is not symmetrical. The highest peaks lie near the
-eastern edge of the mountain block, rather than along its center, as is
-true in conventional mountains, and the western slopes are broad and
-gentle in contrast to the precipitous eastern slopes. The northern end
-of the range disappears under enormous lava flows that form the
-Yellowstone Volcanic Plateau. Even from this altitude the outlines of
-some of these flows can be seen.
-
-On the south the Teton Range abuts almost at right angles against a
-northwest-trending area of lower and less rugged mountains (the Snake
-River, Wyoming, and Hoback Ranges). These mountains appear altogether
-different from the Tetons. They consist of a series of long parallel
-ridges cut or separated by valleys and canyons. This pattern is
-characteristic of mountains composed of crumpled, steeply tilted rock
-layers—erosion wears away the softer layers, leaving the harder ones
-standing as ridges.
-
-On the east and northeast, Jackson Hole is bounded by the Gros Ventre
-and Washakie Ranges, which are composed chiefly of folded hard and soft
-sedimentary rocks. In contrast, between these mountains and the deepest
-part of Jackson Hole to the west, thick layers of soft nearly flat-lying
-sedimentary rocks have been sculptured by streams and ice into randomly
-oriented knife-edge ridges and rolling hills separated by broad valleys.
-The hills east of the park are called the Mount Leidy Highlands and
-those northeast are the Pinyon Peak Highlands.
-
-
-                             A pilot’s view
-
-If you descend from 100 miles to about 5 miles above the Teton region,
-the asymmetry of the range, the extraordinary variety of landscapes, and
-the vivid colors of rocks become more pronounced.
-
-Figure 2 shows a panorama of the Teton Range and Jackson Hole from a
-vantage point over the Pinyon Peak Highlands. The rough steep slopes and
-jagged ridges along the east front of the range contrast with smoother
-slopes and more rounded ridges on the western side. Nestled at the foot
-of the mountains and extending out onto the floor of Jackson Hole are
-tree-rimmed sparkling lakes of many sizes and shapes. Still others lie
-in steep-sided rocky amphitheaters near the mountain crests.
-
-One of the most colorful flight routes into Jackson Hole is from the
-east, along the north flank of the Gros Ventre Mountains. For 40 miles
-this mountain range is bounded by broad parallel stripes of bright-red,
-pink, purple, gray, and brown rocks. Some crop out as cliffs or ridges,
-and others are _badlands_ (bare unvegetated hills and valleys with steep
-slopes and abundant dry stream channels). In places the soft beds have
-broken loose and flowed down slopes like giant varicolored masses of
-taffy. These are mudflows and landslides. The colorful rocks are bounded
-on the south by gray and yellow tilted layers forming snowcapped peaks
-of the Gros Ventre Mountains.
-
-These landscapes are the product of many natural forces acting on a
-variety of rock types during long or short intervals of geologic time.
-Each group of rocks records a chapter in the geologic story of the
-region. Other chapters can be read from the tilting, folding, and
-breaking of the rocks. The latest episodes are written on the face of
-the land itself.
-
-
-                           A motorist’s view
-
-Most park visitors first see the Teton peaks from the highway. Whether
-they drive in from the south, east, or north, there is one point on the
-route at which a spectacular panorama of the Tetons and Jackson Hole
-suddenly appears. Part of the thrill of these three views is that they
-are so unexpected and so different. The geologic history is responsible
-for these differences.
-
-
-  _View north._—
-
-Throughout the first 4 miles north of the town of Jackson, the view of
-the Tetons from U. S. 26-89 is blocked by East Gros Ventre Butte. At the
-north end of the butte, the highway climbs onto a flat upland at the
-south boundary of Grand Teton National Park. Without any advance
-warning, the motorist sees the whole east front of the Teton Range
-rising steeply from the amazingly flat floor of Jackson Hole.
-
-From the park boundary turnout no lakes or rivers are visible to the
-north but the nearest line of trees in the direction of the highest
-Teton peaks marks the approximate position of the Gros Ventre River. The
-elevation of this river is surprising, for the route has just come up a
-150-foot hill, out of the flat valley of a much smaller stream, yet here
-at eye-level is a major river perched on an upland plain. The reason for
-these strange relations is that the hill is a fault scarp (see fig. 16A
-for a diagram) and the valley in which the town of Jackson is located
-was dropped 150 feet or more in the last 15,000 years.
-
-On the skyline directly west of the turnout are horizontal and inclined
-layers of rocks. These once extended over the tops of the highest peaks
-but were worn away from some parts as the mountains rose. All along the
-range, trees grow only up to _treeline_ (also called _timberline_—a
-general elevation above which trees do not grow) which here is about
-10,500 feet above the sea. To the southeast and east, beyond the
-sage-covered floor of Jackson Hole, are rolling partly forested slopes
-marking the west end of the Gros Ventre Mountains. They do not look at
-all like the Tetons because they were formed in a very different manner.
-The Gros Ventres are folded mountains that have foothills; the Tetons
-are faulted mountains that do not.
-
-    Figure 3. _The Teton landscape as seen from Signal Mountain._
-
-    [Illustration: A. _View west across Jackson Lake. Major peaks,
-    canyons, and outcrops of sedimentary rocks are indicated by “s.”_]
-
-    [Illustration: B. _View northeast; a study in contrast with the
-    panorama above._]
-
-Three steepsided hills called _buttes_ rise out of the flat floor of
-Jackson Hole. They are tilted and faulted masses of hard, layered rock
-that have been shaped by southward-moving glaciers. Six miles north of
-the boundary turnout is Blacktail Butte, on the flanks of which are
-west-dipping white beds. Southwest of the turnout is East Gros Ventre
-Butte, composed largely of layered rocks that are exposed along the road
-from Jackson almost to the turnout. These are capped by very young lava
-that forms the brown cliff overlooking the highway at the north end of
-the butte. To the southwest is West Gros Ventre Butte, composed of
-similar rocks.
-
-
-  _View west._—
-
-The motorist traveling west along U. S. 26-287 is treated to two
-magnificent views of the Teton Range. The first is 8 miles and the
-second 13 miles west of Togwotee Pass. At these vantage points, between
-20 and 30 miles from the mountains, the great peaks seem half suspended
-between earth and sky—too close, almost, to believe, but too distant to
-comprehend.
-
-Only from closer range can the motorist begin to appreciate the size and
-steepness of the mountains and to discern the details of their
-architecture. The many roads on the floor of Jackson Hole furnish
-ever-changing vistas, and signs provided by the National Park Service at
-numerous turnouts and scenic overlooks help the visitor to identify
-quickly the major peaks and canyons and the principal features of the
-valley floor. Of all these roadside vantage points, the top of Signal
-Mountain, an isolated hill rising nearly 1,000 feet out of the east
-margin of Jackson Lake, probably offers the best overall perspective
-(fig. 3). To the west, across the shimmering blue waters of Jackson
-Lake, the whole long parade of rugged peaks stretches from the north
-horizon to the south, many of the higher ones wearing the tattered
-remnants of winter snow. From here, only 8 miles away, the towering
-pinnacles, saw-toothed ridges, and deep U-shaped canyons are clearly
-visible.
-
-Unlike most other great mountain ranges, the Tetons rise steeply from
-the flat valley floor in a straight unbroken line. The high central
-peaks tower more than a mile above the valley, but northward and
-southward the peaks diminish in height and lose their jagged character,
-gradually giving way to lower ridges and rounded hills. Some of the
-details of the mountain rock can be seen—gnarled gray rocks of the high
-peaks threaded by a fine white lacework of dikes, the dark band that
-cleaves through Mount Moran from base to summit, and the light brown and
-gray layers on the northern and southern parts of the range.
-
-At first glance the floor of Jackson Hole south of Signal Mountain seems
-flat, smooth, and featureless, except for the Snake River that cuts
-diagonally across it. Nevertheless, even the flats show a variety of
-land forms. The broad sage-covered areas, low isolated hills, and
-hummocky tree-studded ridges that form the foreground are all parts of
-the Teton landscape, and give us clues to the natural processes that
-shaped it. A critical look to the south discloses more strange things.
-We take for granted the fact that the sides of normal valleys slope
-inward toward a central major stream. South of Signal Mountain, however,
-the visitor can see that the Snake River Valley does not fit this
-description. The broad flat west of the river should slope east but it
-does not. Instead, it has been tilted westward by downward movement
-along the Teton fault at the base of the mountains.
-
-
-  _View south._—
-
-About a million motorists drive south from Yellowstone to Grand Teton
-National Park each year. As they wind along the crooked highway on the
-west brink of Lewis River Canyon (fig. 1), the view south is everywhere
-blocked by dense forest. Then, abruptly the road leaves the canyon,
-straightens out, and one can look south down a 3-mile sloping avenue cut
-through the trees. There, 20 to 30 miles away, framed by the roadway,
-are the snow-capped Tetons, with Jackson Lake, luminous in reflected
-light, nestled against the east face. This is one of the loveliest and
-most unusual views of the mountains that is available to the motorist,
-partly because he is 800 feet above the level of Jackson Lake and partly
-because this is the only place on a main highway where he can see
-clearly the third dimension (width) of the Tetons. The high peaks are on
-the east edge; they rise 7,000 feet above the lake but other peaks and
-precipitous ridges, progressively diminishing in height, extend on to
-the west for a dozen miles (fig. 14). Giant, relatively young lava
-flows, into which the Lewis River Canyon was cut, poured southward all
-the way to the shore of Jackson Lake and buried the north end of the
-Teton Range (figs. 13 and 53). South of Yellowstone Park these flows
-were later tilted and broken by the dropping of Jackson Hole and the
-rise of the mountains.
-
-
-                          A mountaineer’s view
-
-As in many pursuits in life, the greatest rewards of a visit to the
-Tetons come to those who expend a real effort to earn them. Only by
-leaving the teeming valley and going up into the mountains to hike the
-trails and climb the peaks can the visitor come to know the Tetons in
-all their moods and changes and view close at hand the details of this
-magnificent mountain edifice.
-
-Even a short hike to Hidden Falls and Inspiration Point affords an
-opportunity for a more intimate view of the mountains. Along the trail
-the hiker can examine outcrops of sugary white granite, glittering
-mica-studded dikes, and dark intricately layered rocks. Nearby are great
-piles of broken fragments that have fallen from the cliffs above, and
-the visitor can begin to appreciate how vulnerable are the towering
-crags to the relentless onslaught of frost and snow. The roar of the
-foaming stream and the thunder of the falls are constant reminders of
-the patient work of running water in wearing away the “everlasting
-hills.” Running his hand across one of the smoothly polished rock faces
-below Inspiration Point, the hiker gains an unforgettable concept of the
-power of glacial ice and its importance in shaping this majestic
-landscape. Looking back across Jenny Lake at the encircling ridge of
-glacial debris, he can easily comprehend the size of the ancient glacier
-that once flowed down Cascade Canyon and emerged onto the floor of
-Jackson Hole.
-
-The more ambitious hiker or mountaineer can seek out the inner recesses
-of the range and explore other facets of its geology. He can visit the
-jewel-like mountain lakes—Solitude, Holly, and Amphitheater are just a
-few—cradled in high remote basins left by the Ice Age glaciers. He can
-get a closeup view of the Teton Glacier above Amphitheater Lake, or
-explore the Schoolroom Glacier, the tiny ice body below Hurricane Pass.
-He may follow the trail into Garnet Canyon to see the crystals from
-which the canyon takes its name and to examine the soaring ribbonlike
-black dike near the end of the trail. In Alaska Basin he can study the
-gently tilted layers of sandstone, limestone, and shale that once
-blanketed the entire Teton Range and can search for the fossils that
-help determine their age and decipher their history. From Hurricane Pass
-he can see how these even layers of sedimentary rock have been broken
-and displaced and how the older harder rocks that form the highest Teton
-peaks have been raised far above them along the Buck Mountain fault.
-
-Of all those who explore the high country, it is the mountaineer who has
-perhaps the greatest opportunity to appreciate its geologic story.
-Indeed, the success of his climb and his very life may depend on an
-intuitive grasp of the mountain geology and the processes that shaped
-the peaks. He observes the most intimate details—the inclination of the
-joints and fractures, which gullies are swept by falling rocks, which
-projecting knobs are firm, and which cracks will safely take a piton. To
-many climbers the ascent of a peak is a challenge to technical
-competence, endurance, and courage, but to those endowed with curiosity
-and a sharp eye it can be much more. As he stands shoulder to shoulder
-with the clouds on some windswept peak, such as the Grand Teton, with
-the awesome panorama dropping away on all sides, he can hardly avoid
-asking how this came to be. What does the mountaineer see that inspires
-this curiosity? From the very first glance, it is apparent that the
-scenes to the north, south, east, and west are startlingly different.
-
-Looking west from the rough, narrow, weather-ravaged granite summit of
-the Grand Teton, one sees far below him the layered gray cliffs of
-_marine sedimentary rocks_ (solidified sediment originally deposited in
-a shallow arm of the ocean) overlapping the granite and dipping gently
-west, finally disappearing under the checkerboard farmland of Teton
-Basin. Still farther west are the rolling timbered slopes of the Big
-Hole Range in Idaho. A glance at the foreground, 3,000 feet below, shows
-some unusual relations of the streams to the mountains. The watershed
-divide of the Teton Range is not marked by the highest peaks as one
-would expect. Streams in Cascade Canyon and in other canyons to the
-north and south begin west of the peaks, bend around them, then flow
-eastward in deep narrow gorges cut through the highest part of the
-range, and emerge onto the flat floor of Jackson Hole.
-
-In the view north along the crest of the Teton Range, the asymmetry of
-the mountains is most apparent. The steep east face culminating in the
-highest peaks contrasts with the lower more gentle west flank of the
-uplift. From the Grand Teton it is not possible to see the actual place
-where the mountains disappear under the lavas of Yellowstone Park, but
-the heavily timbered broad gentle surface of the lava plain is visible
-beyond the peaks and extends across the entire north panorama. Still
-farther north, 75 to 100 miles away, rise the snowcapped peaks (from
-northwest to northeast) of the Madison, Gallatin, and Beartooth
-Mountains.
-
-The view east presents the greatest contrasts in the shortest
-distances—the flat floor of Jackson Hole is 3 miles away and 7,000 feet
-below the top of the Grand Teton. Along the junction of the mountains
-and valley floor are blue glacial lakes strung out like irregular beads
-in a necklace. They are conspicuously rimmed by black-appearing margins
-of pine trees that grow only on the surrounding glacial moraines. Beyond
-these are the broad treeless boulder-strewn plains of Jackson Hole.
-Fifty miles to the east and northeast, on the horizon beyond the rolling
-hills of the Pinyon Peak Highlands, are the horizontally layered
-volcanic rocks of the Absaroka Range. Southeast is the colorful red,
-purple, green, and gray Gros Ventre River Valley, with the fresh giant
-scar of the Lower Gros Ventre Slide near its mouth. Bounding the south
-side of this valley are the peaks of the Gros Ventre Mountains, whose
-tilted slabby gray cliff-forming layers resemble (and are the same as)
-those on the west flank of the Teton Range. Seventy miles away, in the
-southeast distance, beyond the Gros Ventre Mountains are the shining
-snowcapped peaks of the Wind River Range, the highest peak of which
-(Gannett Peak) is about 20 feet higher than the Grand Teton.
-
-Conspicuous on the eastern and southeastern skyline are high-level
-(11,000-12,000 feet) flat-topped surfaces on both the Wind River and
-Absaroka Ranges. These are remnants that mark the upper limit of
-sedimentary fill of the basins adjacent to the mountains. A plain once
-connected these surfaces and extended westward at least as far as the
-conspicuous flat on the mountain south of Lower Gros Ventre Slide. It is
-difficult to imagine the amount of rock that has been washed away from
-between these remnants in comparatively recent geologic time, during and
-after the rise of the Teton Range.
-
-From this vantage point the mountaineer also gets a concept of the
-magnitude of the first and largest glaciers that scoured the landscape.
-Ice flowed southwestward in an essentially unbroken stream from the
-Beartooth Mountains, 100 miles away, westward from the Absaroka Range,
-and northwestward from the Wind River Range (fig. 57). Ice lapped up to
-treeline on the Teton Range and extended across Jackson Hole nearly to
-the top of the Lower Gros Ventre Slide. The Pinyon Peak and Mount Leidy
-Highlands were almost buried. All these glaciers came together in
-Jackson Hole and flowed south within the ever-narrowing Snake River
-Valley.
-
-The view south presents a great variety of contrasts. Conspicuous, as in
-the view north, is the asymmetry of the range. South of the high peaks
-of crystalline rocks, gray layered cliffs of limestone extend in places
-all the way to the steep east face of the Teton Range where they are
-abruptly cut off by the great Teton fault.
-
-The flat treeless floor of Jackson Hole narrows southward. Rising out of
-the middle are the previously described steepsided ice-scoured rocky
-buttes. Beginning near the town of Jackson, part of which is visible,
-and extending as far south as the eye can see are row upon row of sharp
-ridges and snowcapped peaks that converge at various angles. These are
-the Hoback, Wyoming, Salt River, and Snake River Ranges.
-
-
-
-
-                        CARVING THE RUGGED PEAKS
-
-
-The rugged grandeur of the Tetons is a product of four geologic factors:
-the tough hard rocks in the core, the amount of vertical uplift, the
-recency of the mountain-making movement, and the dynamic forces of
-destruction. Many other mountains in Wyoming have just as hard rocks in
-their cores and an equally great amount of vertical uplift, but they
-rose 50 to 60 million years ago and have been worn down by erosion from
-that time on. The Tetons, on the other hand, are the youngest range in
-Wyoming, less than 10 million years old, and have not had time to be so
-deeply eroded.
-
-
-            Steep mountain slopes—the perpetual battleground
-
-Any steep slope or cliff is especially vulnerable to nature’s methods of
-destruction. In the Tetons we see the never-ending struggle between two
-conflicting factors. The first is the extreme toughness of the rocks and
-their consequent resistance to erosion. The second is the presence of
-efficient transporting agencies that move out and away from the
-mountains all rock debris that might otherwise bury the lower slopes.
-
-The rocks making up most of the Teton Range are among the hardest,
-toughest, and least porous known. Therefore, they resist mechanical
-disintegration by temperature changes, ice, and water. They consist
-predominantly of minerals that are subject to very little chemical decay
-in the cold climate of the Tetons.
-
-Absence of weak layers prevents breaking of the tough rock masses under
-their own weight. All these conditions, then, are favorable for
-preservation of steep walls and high rock pinnacles. Nevertheless, they
-do break down. Great piles of broken rock _(talus)_ that festoon the
-slopes of all the higher peaks bear witness to the unrelenting assault
-by the process of erosion upon the mountain citadels (figs. 4 and 31).
-
-
-             Rock disintegration and gravitational movement
-
-A great variation in both daily and annual temperatures results in
-minute amounts of contraction and expansion of rock particles. Repeated
-changes in volume produce stress and strain. Although the rocks in the
-Tetons are very dense, they eventually yield; a crack forms. Water which
-seeps in along this surface of weakness freezes, either overnight or
-during long cold spells, and expands, thereby prying a slab of rock away
-from the mountain wall. Repeated _frost wedging_, as the process is
-called, results eventually in tipping the slab so that it falls.
-
-    [Illustration: Figure 4. _Talus at the foot of the jagged
-    frost-riven peaks around Ice Floe Lake in the south fork of Cascade
-    Canyon. Photo by Philip Hyde._]
-
-What happens to the rock slab? It may fall and roll several hundred or
-thousand feet, depending on the steepness of the mountain surface.
-Pieces are broken off as it encounters obstacles. All the fragments find
-their way to a valley floor or slope, where they momentarily come to
-rest. Thus, rock debris is moved significant and easily observed
-distances by gravity.
-
-None of this debris is stationary. If it is mixed with snow or saturated
-with water, the whole mass may slowly flow in the same manner as a
-glacier. These are called _rock glaciers_; some can be seen on the south
-side of Granite Canyon and one, nearly a mile long, is in the valley
-north of Eagles Rest Peak.
-
-The countless snow avalanches that thunder down the mountain flanks
-after heavy winter snowfalls play their part, too, in gravitational
-transport. Loose rocks and debris are incorporated with the moving snow
-and borne down the mountainsides to the talus piles below. Trees,
-bushes, and soil are swept from the sites of the slides, leaving
-conspicuous scars down the slopes and exposing new rock surfaces to the
-attack of water and frost. Battered, broken, and uprooted trees along
-many of the canyon trails bear silent witness to the awesome power of
-snowslides.
-
-These are some of the methods used by Nature in making debris and then,
-by means of gravity, clearing it from the mountain slopes. There are
-other ways, too. A weak layer of rock (usually one with a lot of clay in
-it), parallel to and underlying a mountain slope, may occur between two
-hard layers. An extended rainy spell may result in saturation of the
-weak zone so that it is well lubricated; then an earthquake or perhaps
-merely the weight of the overlying rock sends the now unstable mass
-cascading down the slope to the valley below. The famous Lower Gros
-Ventre Slide (fig. 5) was formed in this way on June 23, 1925.
-
-
-                     Running water cuts and carries
-
-Running water is another effective agent that transports rock debris and
-has helped dissect the Teton Range. The damage a broken water main can
-wreak on a roadbed is well known, as is the havoc of destructive floods.
-The spring floods of streams in the Tetons, swollen by melting snow and
-ice (annual precipitation, mostly snow, in the high parts would average
-a layer of water 5 feet thick), move some rock debris onto the adjoining
-floor of Jackson Hole.
-
-    [Illustration: Figure 5. _The Lower Gros Ventre slide, air oblique
-    view south. The top of the scar is 2,000 feet above the river; the
-    slide is more than a mile long and one-half mile wide. It dammed the
-    Gros Ventre River in the foreground, impounding a lake about 200
-    feet deep and 5 miles long. Gros Ventre Mountains are in the
-    distance. Photo by P. E. Millward._]
-
-Now and then the range is deluged by summer cloudbursts. Water funnels
-down the maze of gullies on the mountainsides, quickly gathering volume
-and power, and plunges on to the talus slopes below, as if from gigantic
-hoses. The sudden onslaught of these torrents of water on the saturated
-unstable talus may trigger enormous rock and mudflows that carry vast
-quantities of material down into the canyons. During the summer of 1941
-more than 100 of these flows occurred in the park.
-
-Wherever water moves, it carries rock fragments varying in size from
-boulders to sand grains and on down to minute clay particles. _Erosion_
-(wearing away) by streams is conspicuous wherever the water is muddy, as
-it always is each spring in the Snake, Buffalo Fork, and Gros Ventre
-Rivers. Clear mountain streams likewise can erode. Although the volume
-of material moved and the amount of downcutting of the stream bottom may
-not seem great in a single stream, the cumulative effect of many streams
-in an area, year after year and century after century, is enormous.
-Streams not only transport rocks brought to them by gravitational
-movement but also continually widen and deepen their valleys, thereby
-increasing the volume of transported debris.
-
-The effectiveness of streams as transporting agents in the Tetons is
-enhanced by steep _gradients_ (slopes); these increase water velocity
-which in turn expands the capability of the streams to carry larger and
-larger rock fragments.
-
-
-                      Glaciers scour and transport
-
-Mountain landscapes shaped by frost action, gravitational transport, and
-stream erosion alone generally have rounded summits, smooth slopes, and
-V-shaped valleys. The jagged ridges, sharply pointed peaks, and deep
-U-shaped valleys of the Tetons show that glaciers have played an
-important role in their sculpture. The small present-day glaciers still
-cradled in shaded recesses among the higher peaks (fig. 6) are but
-miniature replicas of great ice streams that occupied the region during
-the Ice Age. Evidence both here and in other parts of the world confirms
-that glaciers were once far more extensive than they are today.
-
-Glaciers form wherever more snow accumulates during the winter than is
-melted during the summer. Gradually the piles of snow solidify to form
-ice, which begins to flow under its own weight. Rocks that have fallen
-from the surrounding ridges or have been picked up from the underlying
-bedrock are incorporated in the moving ice mass and carried along. The
-ability of ice to transport huge volumes of rock is easily observed even
-in the small present-day glaciers in the Tetons, all of which carry
-abundant rock fragments both on and within the ice.
-
-    [Illustration: Figure 6. _The Teton Glacier on the north side of
-    Grand Teton, air oblique view west. Photo by A. S. Post, August 19,
-    1963._]
-
-Recent measurements show that the ice in the present Teton Glacier (fig.
-6) moves nearly 30 feet per year. The ancient glaciers, which were much
-wider and deeper, may have moved as much as several hundred feet a year,
-like some of the large glaciers in Alaska.
-
-As the glacier moves down a valley, it scours the valley bottom and
-walls. The efficiency of ice in this process is greatly increased by the
-presence of rock fragments which act as abrasives. The valley bottom is
-plowed, quarried, and swept clean of soil and loose rocks. Fragments of
-many sizes and shapes are dragged along the bottom of the moving ice and
-the hard ones scratch long parallel grooves in the underlying tough
-bedrock (fig. 7). Such grooves (_glacial striae_) record the direction
-of ice movement.
-
-The effectiveness of glaciers in cutting a U-shaped valley is
-particularly striking in Glacier Gulch and Cascade Canyon (figs. 2 and
-8).
-
-The rock-walled amphitheater at the head of a glaciated valley is called
-a _cirque_ (a good example is at the upper edge of the Teton Glacier,
-fig. 6). The steep cirque walls develop by frost action and by quarrying
-and abrasive action of the glacier ice where it is near its maximum
-thickness. Commonly the glacier scoops out a shallow basin in the floor
-of the cirque. Amphitheater Lake, Lake Solitude, Holly Lake, and many of
-the other small lakes high in the Teton Range are located in such
-basins.
-
-The sharp peaks and the jagged knife-edge ridges so characteristic of
-the Tetons are divides left between cirques and valleys carved by the
-ancient glaciers.
-
-
-                        Effects on Jackson Hole
-
-Rock debris is carried toward the end of the glacier or along the
-margins where it is released as the ice melts. The semicircular ridge of
-rock fragments that marks the downhill margin of the glacier is called a
-_terminal moraine_; that along the sides is a _lateral moraine_ (figs. 9
-and 10). These are formed by the slow accumulation of material in the
-same manner as that at the end of a conveyor belt. They are not built by
-material pushed up ahead of the ice as if by a bulldozer. Large boulders
-carried by ice are called _erratics_; many of these are scattered on the
-floor of Jackson Hole and on the flanks of the surrounding mountains
-(fig. 11).
-
-    [Illustration: Figure 7. _Rock surface polished and grooved by ice
-    on the floor of Glacier Gulch._]
-
-Great volumes of water pour from melting ice near the lower end of a
-glacier. These streams, heavily laden with rock flour produced by the
-grinding action of the glacier and with debris liberated from the
-melting ice, cut channels through the terminal moraine and spread a
-broad apron of gravel, sand, and silt down-valley from the glacier
-terminus (end). Material deposited by streams issuing from a glacier is
-called _outwash_; the sheet of outwash in front of the glacier is called
-an _outwash plain_. If the terminus is retreating, masses of old
-stagnant ice commonly are buried beneath the outwash; when these melt,
-the space they once occupied becomes a deep circular or irregular
-depression called a _kettle_ (fig. 12); many of these now contain small
-lakes or swamps.
-
-As a glacier retreats, it may build a series of terminal moraines,
-marking pauses in the recession of the ice front. Streams issuing from
-the ice behind each new terminal moraine are incised more and more
-deeply into the older moraines and their outwash plains. Thus, new and
-younger layers of bouldery debris are spread at successively lower and
-lower levels. These surfaces are called _outwash terraces_.
-
-    [Illustration: Figure 8. _East face of the Teton Range showing some
-    of the glacial features, air oblique view. Cascade Canyon, the
-    U-shaped valley, was cut by ice. The glacier flowed toward the
-    flats, occupied the area of Jenny Lake (foreground), and left an
-    encircling ring of morainal debris, now covered with trees. The flat
-    bare outwash plain in foreground was deposited by meltwater from the
-    glacier. The lake occupies a depression that was left when the ice
-    melted away. National Park Service photo by Bryan Harry._]
-
-    [Illustration: Figure 9. _Cutaway view of a typical valley
-    glacier._]
-
-    [Illustration: Figure 10. _Recently-built terminal moraine of the
-    Schoolroom Glacier, a small ice mass near the head of the south fork
-    of Cascade Canyon. The present glacier lies to the right just out of
-    the field of view. The moraine marks a former position of the ice
-    terminus; the lake (frozen over in this picture) occupies the
-    depression left when the glacier wasted back from the moraine to its
-    present position. Crest of the moraine stands about 50 feet above
-    the lake level. Many of the lakes along the foot of the Teton Range
-    occupy similar depressions behind older moraines. Photo by Philip
-    Hyde._]
-
-    [Illustration: Figure 11. _Large ice-transported boulder of
-    coarse-grained pegmatite and granite resting on Cretaceous shale
-    near Mosquito Creek, on the southwest margin of Jackson Hole. Many
-    boulders at this locality are composed of pegmatite rock
-    characteristic of the middle part of the Teton Range. This
-    occurrence demonstrates that boulders 40 feet in diameter were
-    carried southward 25 miles and left along the west edge of the ice
-    stream, 1,500 feet above the base of the glacier on the floor of
-    Jackson Hole._]
-
-Just as the jagged ridges, U-shaped valleys, and ice-polished rocks of
-the Teton Range attest the importance of glaciers in carving the
-mountain landscape, the flat gravel outwash plains and hummocky moraines
-on the floor of Jackson Hole demonstrate their efficiency in
-transporting debris from the mountains and shaping the scenery of the
-valley.
-
-Glaciers sculptured all sides of Jackson Hole and filled it with ice to
-an elevation between 1,000 and 2,000 feet above the present valley
-floor. The visitor who looks eastward from the south entrance to the
-park can see clearly glacial scour lines that superficially resemble a
-series of terraces on the bare lower slopes of the Gros Ventre
-Mountains. Southward-moving ice cut these features in hard rocks.
-Elsewhere around the margins of Jackson Hole, especially where the rocks
-are soft, evidence that the landscape was shaped by ice has been partly
-or completely obliterated by later events. Rising 1,000 feet above the
-floor of Jackson Hole are several steepsided buttes (figs. 13 and 55)
-described previously, that represent “islands” of hard rock overridden
-and abraded by the ice. After the ice melted, these buttes were
-surrounded and partly buried by outwash debris.
-
-    [Illustration: Figure 12. _“The Potholes,” knob and kettle
-    topography caused by melting of stagnant ice partly buried by
-    outwash gravel. Air oblique view north from over Burned Ridge
-    moraine (see fig. 61 for orientation). Photo by W. B. Hall and J. M.
-    Hill._]
-
-The story of the glaciers and their place in the geologic history of the
-Teton region is discussed in more detail later in this booklet.
-
-    [Illustration: Figure 13. _Radar image of part of Tetons and Jackson
-    Hole. Distance shown between left and right margins is 35 miles.
-    Lakes from left to right: Phelps, Taggart, Bradley, Jenny, Leigh,
-    Jackson. Blacktail Butte is at lower left. Channel of Snake River
-    and outwash terraces are at lower left. Burned Ridge and Jackson
-    Lake moraines are in center. Lava flows at upper right engulf north
-    end of Tetons. Striated surfaces at lower right are glacial scour
-    lines made by ice moving south from Yellowstone National Park. Image
-    courtesy of National Aeronautics and Space Administration._]
-
-
-
-
-                            MOUNTAIN UPLIFT
-
-
-Mountains appear ageless, but as with people, they pass through the
-stages of birth, youth, maturity, and old age, and eventually disappear.
-The Tetons are youthful and steep and are, therefore, extremely
-vulnerable to destructive processes that are constantly sculpturing the
-rugged features and carrying away the debris. The mountains are being
-destroyed. Although the processes of destruction may seem slow to us, we
-know they have been operating for millions of years—so why have the
-mountains not been leveled? How did they form in the first place?
-
-
-                           Kinds of mountains
-
-There are many kinds of mountains. Some are piles of lava and debris
-erupted from a volcano. Others are formed by the bowing up of the
-earth’s crust in the shape of a giant dome or elongated arch. Still
-others are remnants of accumulated sedimentary rocks that once filled a
-basin between preexisting mountains and which are now partially worn
-away. An example of this type is the Absaroka Range 40 miles northeast
-of the Tetons (figs. 1 and 52).
-
-The Tetons are a still different kind—a _fault block mountain range_
-carved from a segment of the earth’s crust that has been uplifted along
-a fault. The _Teton fault_ is approximately at the break in slope where
-the eastern foot of the range joins the flats at the west edge of
-Jackson Hole (see map inside back cover), but in most places is
-concealed beneath glacial deposits and debris shed from the adjacent
-steep slopes. The shape of the range and its relation to Jackson Hole
-have already been described. Clues as to the presence of the fault are:
-(1) the straight and deep east face of the Teton Range, (2) absence of
-foothills, (3) asymmetry of the range (fig. 14), and (4) small _fault
-scarps_ (cliffs or steep slopes formed by faulting) along the mountain
-front (fig. 15).
-
-    [Illustration: Figure 14. _Air oblique view south showing the width
-    and asymmetry of Teton Range. Grand Teton is left of center and Mt.
-    Moran is the broad humpy peak still farther left. Photo taken
-    October 1, 1965_.]
-
-Recent geophysical surveys of Jackson Hole combined with data from deep
-wells drilled in search of oil and gas east of the park also yield
-valuable clues. By measuring variations in the earth’s magnetic field
-and in the pull of gravity and by studying the speed of shock waves
-generated by small dynamite explosions, Dr. John C. Behrendt of the U.
-S. Geological Survey has determined the depth and tilt of rock layers
-buried beneath the veneer of glacial debris and stream-laid sand and
-gravel on the valley floor. This information was used in constructing
-the geologic cross section in the back of the booklet. The same rock
-layers that cap the summit of Mount Moran (fig. 27) are buried at depths
-of nearly 24,000 feet beneath the nearby floor of Jackson Hole but are
-cut off by the Teton fault at the west edge of the valley. Thus the
-approximate amount of movement along the fault here would be about
-30,000 feet.
-
-
-                           Anatomy of faults
-
-The preceding discussion shows that the Tetons are an upfaulted mountain
-block. Why is this significant? The extreme youth of the Teton fault,
-its large amount of displacement, and the fact that the newly upfaulted
-angular mountain block was subjected to intense glaciation are among the
-prime factors responsible for the development of the magnificent alpine
-scenery of the Teton Range. An understanding of the anatomy of faults
-is, therefore, pertinent.
-
-    [Illustration: Figure 15. _Recent fault scarp (arrows indicate base)
-    offsetting alluvial fan at foot of Rockchuck Peak. View west from
-    Cathedral Group scenic turnout. National Park Service photo by W. E.
-    Dilley and R. A. Mebane._]
-
-A fault is a plane or zone in the earth’s crust along which the rocks on
-one side have moved in relation to the rocks on the other. There are
-various kinds of faults just as there are various types of mountains.
-Three principal types of faults are present in the Teton region: normal
-faults, reverse faults, and thrust faults. A _normal fault_ (fig. 16A)
-is a steeply _dipping_ (steeply inclined) fault along which rocks above
-the fault have moved _down_ relative to those beneath it. A _reverse
-fault_ (fig. 16B) is a steeply inclined fault along which the rocks
-above the fault have moved _up_ relative to those below it. A _thrust
-fault_ (fig. 16C) is a gently inclined fault along which the principal
-movement has been more nearly horizontal than vertical.
-
-Normal faults may be the result of tension or pulling apart of the
-earth’s crust or they may be caused by adjustment of the rigid crust to
-the flow of semi-fluid material below. The crust sags or collapses in
-areas from which the subcrustal material has flowed and is bowed up and
-stretched in areas where excess subcrustal material has accumulated. In
-both areas the adjustments may result in normal faults.
-
-Reverse faults are generally caused by compression of a rigid block of
-the crust, but some may also be due to lateral flow of subcrustal
-material.
-
-Thrust faults are commonly associated with tightly bent or folded rocks.
-Many of them are apparently caused by severe compression of part of the
-crust, but some are thought to have formed at the base of slides of
-large rock masses that moved from high areas into adjacent low areas
-under the influence of gravity.
-
-The Teton fault (see cross section inside back cover) is a normal fault;
-the Buck Mountain fault, which lies west of the main peaks of the Teton
-Range, is a reverse fault. No thrust faults have been recognized in the
-Teton Range, but the mountains south and southwest of the Tetons (fig.
-1) display several enormous thrust faults along which masses of rocks
-many miles in extent have moved tens of miles eastward and
-northeastward.
-
-
-                        Time and rate of uplift
-
-When did the Tetons rise?
-
-A study of the youngest sedimentary rocks on the floor of Jackson Hole
-shows that the Teton Range began to rise rapidly and take its present
-shape less than 9 million years ago. The towering peaks themselves are
-direct evidence that the rate of uplift far exceeded the rate at which
-the rising block was worn away by erosion. The mountains are still
-rising, and comparatively rapidly, as is indicated by small faults
-cutting the youngest deposits (fig. 15).
-
-How rapidly? Can the rate be measured?
-
-We know that in less than 9 million years (and probably in less than 7
-million years) there has been 25,000 to 30,000 feet of displacement on
-the Teton fault. This is an average of about 1 foot in 300-400 years.
-The movement probably was not continuous but came as a series of jerks
-accompanied by violent earthquakes. One fault on the floor of Jackson
-Hole near the southern boundary of the park moved 150 feet in the last
-15,000 years, an average of 1 foot per 100 years.
-
-In view of this evidence of recent crustal unrest, it is not surprising
-that small earthquakes are frequent in the Teton region. More violent
-ones can probably be expected from time to time.
-
-    Figure 16. _Types of faults._
-
-    [Illustration: A.—Normal fault (tensional)]
-
-    [Illustration: B.—Reverse fault (compressional)]
-
-    [Illustration: C.—Thrust fault (compressional)]
-
-
-                        Why are mountains here?
-
-Why did the Tetons form where they are?
-
-At the beginning of this booklet we discussed briefly the two most
-common theories of origin of mountains: continental drift and convection
-currents. The question of why mountains are where they are and more
-specifically why the Tetons are here remains a continuing scientific
-challenge regardless of the wealth of data already accumulated in our
-storehouse of knowledge.
-
-The mobility of the earth’s crust is an established fact. Despite its
-apparent rigidity, laboratory experiments demonstrate that rocks flow
-when subjected to extremely high pressures and temperatures. If the
-stress exceeds the strength at a given pressure and temperature, the
-rock breaks. Flowing and fracturing are two of the ways by which rocks
-adjust to the changing environments at various levels in the earth’s
-crust. These acquired characteristics, some of which can be duplicated
-in the laboratory, are guides by which we interpret the geologic history
-of rocks that once were deep within the earth.
-
-The site of the Teton block no doubt reflects hidden inequalities at
-depth. We cannot see these, nor in this area can we drill below the
-outer layer of the earth; nevertheless, measurements of gravity and of
-the earth’s magnetic field clearly show that they exist.
-
-We know that the Tetons rose at the time Jackson Hole collapsed but the
-volume of the uplifted block is considerably less than that of the
-downdropped block. This, then, was not just a simple case in which all
-the subcrustal material displaced by the sinking block was squeezed
-under the rising block (the way a hydraulic jack works). What happened
-to the rest of the material that once was under Jackson Hole? It could
-not be compressed so it had to go somewhere.
-
-As you look northward from the top of the Grand Teton or Mount Moran, or
-from the main highway at the north edge of Grand Teton National Park,
-you see the great smooth sweep of the volcanic plateau in Yellowstone
-National Park. Farther off to the northeast are the strikingly layered
-volcanic rocks of the Absaroka Range (fig. 52). For these two areas, an
-estimate of the volume of volcanic rock that reached the surface and
-flowed out, or was blown out and spread far and wide by wind and water,
-is considerably in excess of 10,000 cubic miles. On the other hand, this
-volume is many times more than that displaced by the sagging and
-downfaulting of Jackson Hole.
-
-Where did the rest of the volcanic material come from? Is it pertinent
-to our story? Teton Basin, on the west side of the Teton Range, and the
-broad Snake River downwarp farther to the northwest (fig. 1) are
-sufficiently large to have furnished the remainder of the volcanic
-debris. As it was blown out of vents in the Yellowstone-Absaroka area,
-its place could have been taken deep underground by material that moved
-laterally from below all three downdropped areas. The movement may have
-been caused by slow convection currents within the earth, or perhaps by
-some other, as yet unknown, force. The sagging of the earth’s crust on
-both sides of the Teton Range as well as the long-continued volcanism
-are certainly directly related to the geologic history of the park.
-
-In summary, we theorize as to how the Tetons rose and Jackson Hole sank
-but are not sure why the range is located at this particular place, why
-it trends north, why it rose so high, or why this one, of all the
-mountain ranges surrounding the Yellowstone-Absaroka volcanic area, had
-such a unique history of uplift. These are problems to challenge the
-minds of generations of earth scientists yet to come.
-
-
-                           The restless land
-
-Among the greatest of the park’s many attractions is the solitude one
-can savor in the midst of magnificent scenery. Only a short walk
-separates us from the highway, torrents of cars, noise, and tension.
-Away from these, everything seems restful.
-
-Quiescent it may seem, yet the landscape is not static but dynamic. This
-is one of the many exciting ideas that geology has contributed to
-society. The concept of the “everlasting hills” is a myth. All the
-features around us are actually rather short-lived in terms of geologic
-time. The discerning eye detects again and again the restlessness of the
-land. We have discussed many bits of evidence that show how the
-landscape and the earth’s crust beneath it are constantly being carved,
-pushed up, dropped down, folded, tilted, and faulted.
-
-The Teton landscape is a battleground, the scene of a continuing
-unresolved struggle between the forces that deform the earth’s crust and
-raise the mountains and the slow processes of erosion that strive to
-level the uplands, fill the hollows, and reduce the landscape to an
-ultimate featureless plain. The remainder of this booklet is devoted to
-tracing the seesaw conflict between these inexorable antagonists through
-more than 2.5 billion years as they shaped the present landscape—and the
-battle still goes on.
-
-Evidence of the struggle is all around us. Even though to some observers
-it may detract from the restfulness of the scene, perhaps it conveys to
-all of us a new appreciation of the tremendous dynamic forces
-responsible for the magnificence of the Teton Range.
-
-The battle is indicated by the small faults that displace both the land
-surface and young deposits at the east base of Mount Teewinot, Rockchuck
-Peak (fig. 15), and other places along the foot of the Tetons.
-
-Jackson Hole continues to drop and tilt. The gravel-covered surfaces
-that originally sloped southward are now tilted westward toward the
-mountains. The Snake River, although the major stream, is not in the
-lowest part of Jackson Hole; Fish Creek, a lesser tributary near the
-town of Wilson, is 15 feet lower. For 10 miles this creek flows
-southward parallel to the Snake River but with a gentler gradient, thus
-permitting the two streams to join near the south end of Jackson Hole.
-As tilting continues, the Snake River west of Jackson tries to move
-westward but is prevented from doing so by long flood-control levees
-built south of the park.
-
-Recent faults also break the valley floor between the Gros Ventre River
-and the town of Jackson.
-
-The ever-changing piles of rock debris that mantle the slopes adjacent
-to the higher peaks, the creeping advance of rock glaciers, the
-devastating snow avalanches, and the thundering rockfalls are specific
-reminders that the land surface is restless. Jackson Hole contains more
-landslides and rock mudflows than almost any other part of the Rocky
-Mountain region. They constantly plague road builders (fig. 17) and add
-to the cost of other types of construction.
-
-All of these examples of the relentless battle between constructive and
-destructive processes modifying the Teton landscape are but minor
-skirmishes. The bending and breaking of rocks at the surface are small
-reflections of enormous stresses and strains deep within the earth where
-the major conflict is being waged. It is revealed every now and then by
-a convulsion such as the 1959 earthquake in and west of Yellowstone
-Park. Events of this type release much more energy than all the nuclear
-devices thus far exploded by man.
-
-    [Illustration: Figure 17. _Slide blocking main highway in northern
-    part of Grand Teton National Park. National Park Service photo by
-    Eliot Davis, May 1952._]
-
-
-
-
-                    ENORMOUS TIME AND DYNAMIC EARTH
-
-
-                           Framework of time
-
-One of geology’s greatest philosophical contributions has been the
-demonstration of the enormity of geologic time. Astronomers deal with
-distances so great that they are almost beyond understanding; nuclear
-physicists study objects so small that we can hardly imagine them.
-Similarly, the geologist is concerned with spans of time so immense that
-they are scarcely comprehensible. Geology is a science of time as well
-as rocks, and in our geologic story of the Teton region we must refer
-frequently to the geologic time scale, the yardstick by which we measure
-the vast reaches of time in earth history.
-
-
-                         Rocks and relative age
-
-Very early in the science of geology it was recognized that in many
-places one can tell the comparative ages of rocks by their relations to
-one another. For example, most _sedimentary rocks_ are consolidated
-accumulations of large or small rock fragments and were deposited as
-nearly horizontal layers of gravel, sand, or mud. In an undisturbed
-sequence of sedimentary rocks, the layer on the bottom was deposited
-first and the layer on top was deposited last. All of these must, of
-course, be younger than any previously formed rock fragments
-incorporated in them.
-
-_Igneous rocks_ are those formed by solidification of molten material,
-either as lava flows on the earth’s surface (_extrusive igneous rocks_)
-or at depth within the earth (_intrusive igneous rocks_). The relative
-ages of extrusive igneous rocks can often be determined in much the same
-way as those of sedimentary strata. A lava flow is younger than the
-rocks on which it rests, but older than those that rest on top of it.
-
-An intrusive igneous rock must be younger than the rocks that enclosed
-it at the time it solidified. It may contain pieces of the enclosing
-rocks that broke off the walls and fell into the liquid. Pebbles of the
-igneous rock that are incorporated in nearby sedimentary layers indicate
-that the sediments must be somewhat younger.
-
-All of these criteria tell us only that one rock is older or younger
-than another. They tell us little about the absolute age of the rocks or
-about how much older one is than the other.
-
-
-                       Fossils and geologic time
-
-Fossils provide important clues to the ages of the rocks in which they
-are found. The slow evolution of living things through geologic time can
-be traced by a systematic study of fossils. The fossils are then used to
-determine the relative ages of the rocks that contain them and to
-establish a geologic time scale that can be applied to fossil-bearing
-rocks throughout the world. Figure 18 shows the major subdivisions of
-the last 600 million years of geologic time and some forms of life that
-dominated the scene during each of these intervals. Strata containing
-closely related fossils are grouped into _systems_; the time interval
-during which the strata comprising a particular system were deposited is
-termed a _period_. The periods are subdivisions of larger time units
-called _eras_ and some are split into smaller time units called
-_epochs_. Strata deposited during an epoch comprise a _series_. Series
-are in turn subdivided into rock units called _groups_ and formations.
-Expressed in tabular form these divisions are:
-
-  Subdivisions of       Time-rock units       Rock units
-  geologic time
-
-  Era
-     Period             System
-        Epoch              Series
-                                              Group
-                                                 Formation
-
-The time scale based on the study of fossil-bearing sedimentary rocks is
-called the stratigraphic time scale; it is given in table 1. The
-subdivisions are arranged in the same order in which they were
-deposited, with the oldest at the bottom and the youngest at the top.
-All rocks older than Cambrian (the first period in the Paleozoic Era)
-are classed as Precambrian. These rocks are so old that fossils are rare
-and therefore cannot be conveniently used as a basis for subdivision.
-
-The stratigraphic time scale is extremely useful, but it has serious
-drawbacks. It can be applied only to fossil-bearing strata or to rocks
-whose ages are determined by their relation to those containing fossils.
-It cannot be used directly for rocks that lack fossils, such as igneous
-rocks, or metamorphic rocks in which fossils have been destroyed by heat
-or pressure. It is used to establish the relative ages of sedimentary
-strata throughout the world, but it gives no information as to how long
-ago a particular layer was deposited or how many years a given period or
-era lasted.
-
-
-                           Radioactive clocks
-
-The measurement of geologic time in terms of years was not possible
-until the discovery of natural radioactivity. It was found that certain
-atoms of a few elements spontaneously throw off particles from their
-nuclei and break down to form atoms of other elements. These decay
-processes take place at constant rates, unaffected by heat, pressure, or
-chemical conditions. If we know the rate at which a particular
-radioactive element decays, the length of time that has passed since a
-mineral crystal containing the elements formed can be calculated by
-comparing the amount of the radioactive element remaining in the crystal
-with the amount of disintegration products present.
-
-    [Illustration: Figure 18. _Major subdivisions of the last 600
-    million years of geologic time and some of the dominant forms of
-    life._]
-
-   MILLIONS OF
-     YEARS AGO
-
-             0                                              Man
-          0-60  CENOZOIC         QUATERNARY and TERTIARY    Mammals
-        60-130  MESOZOIC         CRETACEOUS
-       130-180                   JURASSIC                   Dinosaurs
-       180-220                   TRIASSIC
-       220-260  PALEOZOIC        PERMIAN                    Reptiles
-       260-350                   PENNSYLVANIAN,             Amphibians
-                                 MISSISSIPPIAN
-       350-400                   DEVONIAN                   Fishes
-       400-440                   SILURIAN                   Sea scorpions
-       440-500                   ORDOVICIAN                 Nautiloids
-       500-530                   CAMBRIAN                   Trilobites
-          530-  PRECAMBRIAN                                 Soft-bodied
-                                                            creatures
-
-Three principal radioactive clocks now in use are based on the decay of
-uranium to lead, rubidium to strontium, and potassium to argon. They are
-effective in dating minerals millions or billions of years old. Another
-clock, based on the decay of one type of carbon (_Carbon-14_) to
-nitrogen, dates organic material, but only if it is less than about
-40,000 years old.
-
-The uranium, rubidium, and potassium clocks are especially useful in
-dating igneous rocks. By determining the absolute ages of igneous rocks
-whose stratigraphic relations to fossil-bearing strata are known, it is
-possible to estimate the number of years represented by the various
-subdivisions of the stratigraphic time scale.
-
-
-                     The yardstick of geologic time
-
-Recent estimates suggest that the earth was formed at least 4.5 billion
-years ago. To visualize the length of geologic time and the relations
-between the stratigraphic and absolute time scales, let us imagine a
-yardstick as representing the length of time from the origin of the
-earth to the present (fig. 19). On one side of the yardstick we plot
-time in years; on the other, we plot the divisions of the stratigraphic
-time scale according to the most reliable absolute age determinations.
-
-    [Illustration: Table 1. The stratigraphic time scale.]
-
-  Era                   System or period      Series or epoch
-
-  Cenozoic              Quaternary            Recent
-                                              Pleistocene
-                        Tertiary              Pliocene
-                                              Miocene
-                                              Oligocene
-                                              Eocene
-                                              Paleocene
-  Mesozoic              Cretaceous
-                        Jurassic
-                        Triassic
-  Paleozoic             Permian
-                        Pennsylvanian
-                        Mississippian
-                        Devonian
-                        Silurian[1]
-                        Ordovician
-                        Cambrian
-  —                     Precambrian
-
-
-[1]_The Silurian is the only major subdivision of the stratigraphic time
-    scale not represented in Grand Teton National Park._
-
-
-We are immediately struck by the fact that all of the subdivisions of
-the stratigraphic time scale since the beginning of the Paleozoic are
-compressed into the last 5 inches of our yardstick! All of the other 31
-inches represent Precambrian time. We also see that subdivisions of the
-stratigraphic time scale do not represent equal numbers of years. We use
-smaller and smaller subdivisions as we approach the present. (Notice the
-subdivisions of the Tertiary and Quaternary in table 1 that are too
-small to show even in the enlarged part of figure 19). This is because
-the record of earth history is more vague and incomplete the farther
-back in time we go. In effect, we are very nearsighted in our view of
-time. This “geological myopia” becomes increasingly evident throughout
-the remainder of this booklet.
-
-    [Illustration: Figure 19. _The geologic time scale—our yardstick in
-    time._]
-
-     ABSOLUTE TIME (Years ago)  INCHES  STRATIGRAPHIC TIME SCALE
-
-                   First man →       0  CENOZOIC
-                                     1  MESOZOIC
-             First dinosaurs →       2  PALEOZOIC
-                                     3
-                   500 million       4
-      First abundant fossils →       5  PRECAMBRIAN
-                                     6
-                                     7
-                     1 billion       8
-                                     9
-                                    10
-                                    11
-                                    12
-                                    13
-                                    14
-        Oldest known fossils →      15
-                     2 billion      16
-                                    17
-                                    18
-                                    19
-                                    20
-                                    21
-                                    22
-                                    23
-                     3 billion      24
-                                    25
-                                    26
-                                    27
-          Oldest dated rocks →      28
-                                    29
-                                    30
-                                    31
-                     4 billion      32
-                                    33
-                                    34
-                                    35
-    Minimum age of the earth →      36
-
-                         ENLARGEMENT OF THE LAST SIX INCHES
-    ABSOLUTE TIME   INCHES   STRATIGRAPHIC TIME SCALE
-      (Years Ago)
-
-                0     0      CENOZOIC          QUATERNARY
-                                               TERTIARY
-                             MESOZOIC          CRETACEOUS
-                      1                        JURASSIC
-                                               TRIASSIC
-                      2      PALEOZOIC         PERMIAN
-                                               PENNSYLVANIAN
-                                               MISSISSIPPIAN
-                      3                        DEVONIAN
-                                               SILURIAN
-                                               ORDOVICIAN
-      500 million     4      CAMBRIAN
-                      5      PRECAMBRIAN
-                      6
-
-
-
-
-                PRECAMBRIAN ROCKS—THE CORE OF THE TETONS
-
-
-The visitor who looks at the high, rugged peaks of the Teton Range is
-seeing rocks that record about seven-eighths of all geologic time. These
-Precambrian rocks are part of the very foundation of the continent and
-are therefore commonly referred to by geologists as basement rocks. In
-attempting to decipher their origin and history we peer backward through
-the dim mists of time, piecing together scattered clues to events that
-occurred billions of years ago, perhaps during the very birth of the
-North American Continent. To cite an oft-quoted example, it is as though
-we were attempting to read the history of an ancient and long-forgotten
-civilization from the scattered unnumbered pages of a torn manuscript,
-written in a language that we only partially understand.
-
-
-                      Ancient gneisses and schists
-
-The oldest Precambrian rocks in the Teton Range are layered gneisses and
-schists exposed over wide areas in the northern and southern parts of
-the range and as scattered isolated masses in the younger granite that
-forms the high peaks in the central parts. The layered gneisses may be
-seen easily along the trails in the lower parts of Indian Paintbrush and
-Death Canyons, and near Static Peak.
-
-The _layered gneisses_ are composed principally of quartz, feldspar,
-_biotite_ (black mica), and _hornblende_ (a very dark-green or black
-mineral commonly forming rodlike crystals). Distinct layers, a few
-inches to several feet thick, contain different proportions of these
-minerals and account for the banded appearance. Layers composed almost
-entirely of quartz and feldspar are light-gray or white, whereas darker
-gray layers contain higher proportions of biotite and hornblende.
-
-Some layers are dark-green to black _amphibolite_, composed principally
-of hornblende but with a little feldspar and quartz. In many places the
-gneisses include layers of _schist_, a flaky rock, much of which is
-mica. At several places on the east slopes of Mount Moran thin layers of
-impure gray marble are found interleaved with the gneisses. West of
-Static Peak along the Alaska Basin Trail a heavy dark rock with large
-amounts of _magnetite_ (strongly magnetic black iron oxide) occurs as
-layers in the gneiss.
-
-In some places the gneiss contains dark-reddish crystals of garnet as
-much as an inch in diameter. Commonly the garnet crystals are surrounded
-by white “halos” which lack biotite or hornblende, probably because the
-constituents necessary to form these minerals were absorbed by the
-garnet crystals. In Death Canyon and on the slopes of Static Peak some
-layers of gray gneiss contain egg-shaped masses of magnetite as much as
-one-half inch in diameter (fig. 20). These masses are likewise
-surrounded by elliptical white halos and have the startling appearance
-of small eyes peering from the rock. Appropriately, this rock has been
-called the “bright-eyed” gneiss by Prof. Charles C. Bradley in his
-published study (Wyoming Geological Association, 1956) of this area.
-
-What were the ancient rocks from which the gneisses of the Teton Range
-were formed? Most of the evidence has been obliterated but a few
-remaining clues enable us to draw some general conclusions. The banded
-appearance of many of the gneisses suggests that they were formed from
-sedimentary and volcanic rocks that accumulated on the sea floor near a
-chain of volcanic islands—perhaps somewhat similar to the modern
-Aleutians or the islands of Indonesia. When these deposits were buried
-deep in the earth’s crust the chemical composition of some layers may
-have undergone radical changes. Other layers, however, still have
-compositions resembling those of younger rocks elsewhere whose origins
-are better known. For example, the layers of impure marble were probably
-once beds of sandy limestone, and the lighter colored gneiss may have
-been muddy sandstone, possibly containing volcanic ash. Some dark
-amphibolite layers could represent altered lava flows or beds of
-volcanic ash; others may have resulted from the addition of silica to
-muddy magnesium-rich limestone during metamorphism. The magnetite-rich
-gneiss probably was originally a sedimentary iron ore.
-
-    [Illustration: Figure 20. _“Bright-eyed” gneiss from Death Canyon.
-    The dark magnetite spots are about ¼ inch in diameter. The
-    surrounding gneiss is composed of quartz, feldspar, and biotite, but
-    biotite is missing in the white halos around the magnetite._]
-
-Minerals that were most easily altered at depth reacted with one another
-to form new minerals more “at home” under the high temperature and
-pressure in this environment just as the ingredients in a cake react
-when heated in an oven. Rocks formed by such processes are called
-_metamorphic rocks_; careful studies of the minerals that they contain
-suggest that the layered gneisses developed at temperatures as high as
-1000°F at depths of 5 to 10 miles. Under these conditions the rocks must
-have behaved somewhat like soft taffy as is shown by layers that have
-been folded nearly double without being broken (fig. 21). Folds such as
-these range from fractions of an inch to thousands of feet across and
-are found in gneisses throughout the Teton Range. In a few places folds
-are superimposed in such a way as to indicate that the rocks were
-involved in several episodes of deformation in response to different
-sets of stress during metamorphism.
-
-When did these gneisses form? Age determinations of minerals containing
-radioactive elements show that granite which was intruded into them
-after they were metamorphosed and folded is more than 2.5 billion years
-old. They must, therefore, be older than that. Thus, they probably are
-at least a billion years older than rocks containing the first faint
-traces of life on earth and 2 billion years older than the oldest rocks
-containing abundant fossils. How much older is not known, but the
-gneisses are certainly among the oldest rocks in North America and
-record some of the earliest events in the building of this continent.
-
-    Figure 21. _Folds in layered gneisses._
-
-    [Illustration: A. _North face of the ridge west of Eagles Rest Peak.
-    The face is about 700 feet high. Notice the extreme contortion of
-    the gneiss layers._]
-
-    [Illustration: B. _Closeup view of some of the folds near the bottom
-    of the face in figure A. The light-colored layers are composed
-    principally of quartz and feldspar. The darker layers are rich in
-    hornblende._]
-
-Irregular bodies of granite gneiss are interleaved with the layered
-gneisses in the northern part of the Teton Range. The _granite gneiss_
-is relatively coarse grained, streaky gray or pink, and composed
-principally of quartz, feldspar, biotite, and hornblende. It differs
-from enclosing layered gneisses in its coarser texture, lack of
-layering, and more uniform appearance. The dark minerals (biotite and
-hornblende) are concentrated in thin discontinuous wisps that give the
-rock its streaky appearance.
-
-The largest body of granite gneiss is exposed in a belt 1 to 2 miles
-wide and 10 miles long extending northeastward from near the head of
-Moran Canyon, across the upper part of Moose Basin, and into the lower
-reaches of Webb Canyon. This gneiss may have been formed from granite
-that invaded the ancient sedimentary and volcanic rocks before they were
-metamorphosed, or it may have been formed during metamorphism from some
-of the sediments and volcanics themselves.
-
-At several places in Snowshoe, Waterfalls, and Colter Canyons the
-layered gneisses contain discontinuous masses a few tens or hundreds of
-feet in diameter of heavy dark-green or black _serpentine_. This rock is
-frequently called “_soapstone_” because the surface feels smooth and
-soapy to the touch. Indians carved bowls (fig. 22) from similar material
-obtained from the west side of the Tetons and from the Gros Ventre
-Mountains to the southeast. Pebbles of serpentine along streams draining
-the west side of the Tetons have been cut and polished for jewelry and
-sold as “_Teton jade_”; it is much softer and less lustrous than real
-jade. The serpentine was formed by metamorphism of dark-colored igneous
-rocks lacking quartz and feldspar.
-
-
-                         Granite and pegmatite
-
-Contrary to popular belief, _granite_ (crystalline igneous rock composed
-principally of quartz and feldspar) forms only a part of the Teton
-Range. The Grand Teton (fig. 6) and most surrounding subsidiary peaks
-are sculptured from an irregular mass of granite exposed continuously
-along the backbone of the range from Buck Mountain northward toward
-upper Leigh Canyon. The rock is commonly fine grained, white or
-light-gray, and is largely composed of crystals of gray quartz and white
-feldspar about the size and texture of the grains in very coarse lump
-sugar. Flakes of black or dark-brown mica (biotite) and silvery white
-mica (_muscovite_) about the size of grains of pepper are scattered
-through the rock.
-
-From the floor of Jackson Hole the granite cliffs and buttresses of the
-high peaks appear nearly white in contrast to the more somber grays and
-browns of surrounding gneisses and schists. These dark rocks are laced
-by a network of irregular light-colored granite dikes ranging in
-thickness from fractions of an inch to tens of feet (fig. 23).
-
-    [Illustration: Figure 22. _Indian bowls carved from soapstone,
-    probably from the Teton Range. Mouth of the unbroken bowl is about 4
-    inches in diameter._]
-
-The largest masses of granite contain abundant unoriented angular blocks
-and slabs of the older gneisses. These inclusions range from a few
-inches in diameter (fig. 24) to slabs hundreds of feet thick and
-thousands of feet long.
-
-Dikes or irregular intrusions of pegmatite are found in almost every
-exposure of granite. _Pegmatite_ contains the same minerals as granite
-but the individual mineral crystals are several inches or even as much
-as a foot in diameter.
-
-Some pegmatites contain silvery plates or tabular crystals of muscovite
-mica as much as 6 inches across that can be split into transparent
-sheets with a pocket knife. Others have dark-brown biotite mica in
-crystals about the size and shape of the blade of a table knife.
-
-A few pegmatites contain scattered red-brown crystals of garnet ranging
-in size from that of a BB shot to a small marble; a few in Garnet Canyon
-and Glacier Gulch are larger than baseballs (fig. 25). The garnets are
-fractured and many are partly altered to _chlorite_ (a dull-green
-micaceous mineral) so they are of no value as gems.
-
-    Figure 23. _Dikes of granite and pegmatite._
-
-    [Illustration: A. _Network of light-colored granite dikes on the
-    northeast face of the West Horn on Mt. Moran. The dikes cut through
-    gneiss in which the layers slant steeply downward to the left. The
-    face is about 700 feet high. Snowfield in the foreground is at the
-    edge of the Falling Ice Glacier._]
-
-    [Illustration: B. _Irregular dike of granite and pegmatite cutting
-    through dark layered gneisses near Wilderness Falls in Waterfalls
-    Canyon. The cliff face is about 80 feet high. Contacts of the dike
-    are sharp and angular and cut across the layers in the enclosing
-    gneiss._]
-
-Pegmatite _dikes_ (tabular bodies of rock that, while still molten, were
-forced along fractures in older rocks) commonly cut across granite
-dikes, but in many places the reverse is true. Some dikes are composed
-of layers of pegmatite alternating with layers of granite (fig. 26),
-showing that the pegmatite and granite are nearly contemporaneous. Prof.
-Bruno Giletti and his coworkers at Brown University, using the
-rubidium-strontium radioactive clock, determined that the granite and
-pegmatite in the Teton Range are about 2.5 billion years old.
-
-    [Illustration: Figure 24. _Angular blocks of old streaky granite
-    gneiss in fine-grained granite northwest of Lake Solitude. The
-    difference in orientation of the streaks in the gneiss blocks
-    indicates that the blocks have been rotated with respect to one
-    another and that the fine-grained granite must therefore have been
-    liquid at the time of intrusion. A small light-colored dike in the
-    upper left-hand block of gneiss ends at the edge of the block; it
-    intruded the gneiss before the block was broken off and incorporated
-    in the granite. A small dike of pegmatite cuts diagonally through
-    the granite just to the left of the hammer and extends into the
-    blocks of gneiss at both ends. This dike was intruded after the
-    granite had solidified. Thus, in this one small exposure we can
-    recognize four ages of rocks: the streaky granite gneiss, the
-    light-colored dike, the fine-grained granite, and the small
-    pegmatite dike._]
-
-
-                              Black dikes
-
-Even the most casual visitor to the Teton Range notices the remarkable
-black band that extends down the east face of Mount Moran (figs. 27 and
-28) from the summit and disappears into the trees north of Leigh Lake.
-This is the outcropping edge of a steeply inclined dike composed of
-_diabase_, a nearly black igneous rock very similar to basalt. Thinner
-diabase dikes are visible on the east face of Middle Teton, on the south
-side of the Grand Teton, and in several other places in the range (see
-geologic map inside back cover).
-
-    [Illustration: Figure 25. _Garnet crystal in pegmatite. The crystal
-    is about 6 inches in diameter. Other minerals are feldspar (white)
-    and clusters of white mica flakes. The mica crystals appear dark in
-    the photograph because they are wet._]
-
-The diabase is a heavy dark-greenish-gray to black rock that turns rust
-brown on faces that have been exposed to the weather. It is studded with
-small lath-shaped crystals of feldspar that are greenish gray in the
-fresh rock and milk white on weathered surfaces.
-
-The black dikes formed from molten rock that welled up into nearly
-vertical fissures in the older Precambrian rocks. Toward the edges of
-the dikes the feldspar laths in the diabase become smaller and smaller
-(fig. 29), indicating that the wall rocks were relatively cool when the
-_magma_ or melted rock was intruded. Rapid chilling at the edges
-prevented growth of large crystals. In many places hot solutions from
-the dike permeated the wall rocks, staining them rosy red.
-
-    [Illustration: Figure 26. _A small dike of pegmatite and granite
-    cutting through folded layered gneiss in Death Canyon.
-    Coarse-grained pegmatite forms most of the dike, but fine-grained
-    granite is found near the center. Small offshoots of the dike
-    penetrate into the wall rocks. The dike cuts straight across folds
-    in the enclosing gneisses and must therefore have been intruded
-    after development of the folds. The white ruler is about 6 inches
-    long._]
-
-The black dike on Mount Moran is about 150 feet thick near the summit of
-the peak. This dike has been traced westward for more than 7 miles.
-Where it passes out of the park south of Green Lakes Mountain it is 100
-feet thick. The amount of molten material needed to form the exposed
-segment of this single dike could fill Jenny Lake three times over. The
-other dikes are thinner and not as long: the dike on Middle Teton is 20
-to 40 feet thick, and the dike on Grand Teton is 40 to 60 feet thick.
-
-    [Illustration: Figure 27. _Air oblique view of the east face of Mt.
-    Moran, showing the great black dike. Main mass of the mountain is
-    layered gneiss and streaky granite gneiss. White lines are dikes of
-    granite and pegmatite; light-gray mound on the summit is about 50
-    feet of Cambrian sedimentary rock (Flathead Sandstone). Notice that
-    the black dike cuts across the dikes of granite and pegmatite but
-    that its upper edge is covered by the much younger layer of
-    sandstone. Falling Ice Glacier is in the left center; Skillet
-    Glacier is in the lower right center. Photo by A. S. Post.
-    University of Washington, August 19, 1963._]
-
-    [Illustration: Figure 28. _The great black dike on the east face of
-    Mt. Moran. The dike is about 150 feet thick and its vertical extent
-    in the picture is about 3,000 feet. The fractures in the dike
-    perpendicular to its walls are cracks formed as the liquified rock
-    cooled and crystallized. Falling Ice Glacier is in the center.
-    National Park Service photo by H. D. Pownall._]
-
-    [Illustration: Figure 29. _Closeup view of the edge of the Middle
-    Teton black dike exposed on the north wall of Garnet Canyon near the
-    west end of the trail. Dike rock (diabase) is on the right; wall
-    rock (gneiss) is on the left. Match shows scale._]
-
-The black dikes must be the youngest of the Precambrian units because
-they cut across all other Precambrian rocks. The dikes must have been
-intruded before the beginning of Cambrian deposition inasmuch as they do
-not cut the oldest Cambrian beds. Gneiss adjacent to the dike on Mount
-Moran contains biotite that was heated and altered about 1.3 billion
-years ago according to Professor Giletti. The alteration is believed to
-have occurred when the dike was emplaced; therefore this and similar
-dikes elsewhere in the range are probably about 1.3 billion years old.
-
-
-                               Quartzite
-
-At about the same time as the dikes were being intruded in the Tetons,
-many thousands of feet of sedimentary rocks, chiefly sandstone, were
-deposited in western Montana, 200 miles northwest of Grand Teton
-National Park. The sandstone was later recrystallized and recemented and
-became a very dense hard rock called _quartzite_. Similar quartzite,
-possibly part of the same deposit, was laid down west of the north end
-of the Teton Range, within the area now called the Snake River downwarp
-(fig. 1).
-
-The visitor who hikes or camps anywhere on the floor of Jackson Hole
-becomes painfully aware of the thousands upon thousands of remarkably
-rounded hard quartzite boulders. He wonders where they came from because
-nowhere in the adjacent mountains is this rock type exposed. The answer
-is that the quartzites were derived from a long-vanished uplift (figs.
-42 and 46), carried eastward by powerful rivers past the north end of
-the Teton Range, and then were deposited in a vast sheet of gravel that
-covered much of Jackson Hole 60 to 80 million years ago. Since then,
-these virtually indestructible boulders have been re-worked many times
-by streams and ice, yet still retain the characteristics of the original
-ancient sediments.
-
-
-                           A backward glance
-
-So far we have seen that the Precambrian basement exposed in the Teton
-Range contains a complex array of rocks of diverse origins and various
-ages. Before passing on to the younger rocks, reference to our yardstick
-may help to place the Precambrian events in their proper perspective.
-
-In all of Precambrian time, which encompasses more than 85 percent of
-the history of the earth (31 of the 36 inches of our yardstick), only
-two events are dated in the Teton Range: the intrusion of granite and
-pegmatite about 2.5 billion years ago, and the emplacement of the black
-dikes about 1.3 billion years ago. These dates are indicated by heavy
-arrows on the time scale (fig. 30). The ancient gneisses and schists
-were formed sometime before 2.5 billion years ago, and probably are no
-older than 3.5 billion years, the age of the oldest rocks dated anywhere
-in the world.
-
-
-           The close of the Precambrian—end of the beginning
-
-More than 700 million years elapsed between intrusion of the black dikes
-and deposition of the first Paleozic sedimentary rocks—a longer period
-of time than has elapsed since the beginning of the Paleozic Era. During
-this enormous interval the Precambrian rocks were uplifted, exposed to
-erosion, and gradually worn to a nearly featureless plain, perhaps
-somewhat resembling the vast flat areas in which similar Precambrian
-rocks are now exposed in central and eastern Canada. At the close of
-Precambrian time, about 600 million years ago, the plain slowly
-floundered and the site of the future Teton Range disappeared beneath
-shallow seas that were to wash across it intermittently for the next 500
-million years. It is to the sediments deposited in these seas that we
-turn to read the next chapter in the geologic story of the Teton Range.
-
-    [Illustration: Figure 30. _A glance at the yardstick. The geologic
-    time scale shows positions of principal events recorded in the
-    Precambrian rocks of the Tetons._]
-
-                                ABSOLUTE TIME (Years ago)  INCHES
-
-     Beginning of the Paleozoic. First abundant fossils →    4
-                                                1 billion    8
-                             Maximum age of black dikes →    10
-                                     Oldest known fossils    15
-                                                2 billion    16
-                                Old granite and pegmatite    20
-                                                3 billion    24
-    Gneisses and schists formed sometime in this interval  20-27
-                                     Oldest dated rocks →    28
-                                              4 billion →    32
-                                 Minimum age of the earth    36
-
-
-
-
-THE PALEOZOIC ERA—TIME OF LONG-VANISHED SEAS AND THE DEVELOPMENT OF LIFE
-
-
-                         The Paleozoic sequence
-
-North, west, and south of the highest Teton peaks the soaring spires and
-knife-edge ridges of Precambrian rock give way to rounded spurs and
-lower flat-topped summits, whose slopes are palisaded by continuous gray
-cliffs that resemble the battlements of some ancient and long-abandoned
-fortress (fig. 31). As mentioned previously, the cliffs are the
-projecting edges of layers of sedimentary rocks of Paleozoic age that
-accumulated in or along the margins of shallow seas. At one time the
-layers formed a thick unbroken, nearly horizontal blanket across the
-Precambrian basement rocks, but subsequent uplift of the eastern edge of
-the Teton fault block tilted them westward. They were then stripped from
-the highest peaks.
-
-The Paleozoic and younger sedimentary rocks in the Teton region are
-subdivided into _formations_, each of which is named. A formation is
-composed of rock layers which, because of their similar physical
-characteristics, can be distinguished from overlying and underlying
-layers. They must be thick enough to be shown on a geologic map. Table 2
-lists the various Paleozoic formations present in and adjacent to Grand
-Teton National Park and gives their thicknesses and characteristics.
-These sedimentary rocks are of special interest, for they not only
-record an important chapter of geologic history but elsewhere in the
-region they contain petroleum and other mineral deposits.
-
-The Paleozoic rocks can be viewed close at hand from the top of the
-Teton Village tram (fig. 32) on the south boundary of the park. A less
-accessible but equally spectacular exposure of Paleozoic rocks is in
-Alaska Basin, along the west margin of the park, where they are stacked
-like even layers in a gigantic cake (fig. 33).
-
-
-       Alaska Basin—site of an outstanding rock and fossil record
-
-Strata in Alaska Basin record with unusual clarity the opening chapters
-in the chronicle of seas that flowed and ebbed across the future site of
-the Teton Range during most of the Paleozoic Era. In the various rock
-layers are inscribed stories of the slow advance and retreat of ancient
-shorelines, of the storm waves breaking on long-vanished beaches, and of
-the slow and intricate evolution of the myriads of sea creatures that
-inhabited these restless waters.
-
-    [Illustration: Figure 31. _Paleozoic rocks on the west flank of the
-    Teton Range, air oblique view west. Ragged peaks in the foreground
-    (Buck Mountain on the left center, Mt. Wister, with top outlined by
-    snow patch on the extreme right), are carved in Precambrian rocks.
-    Banded cliffs in the background are sedimentary rocks. Alaska Basin
-    is at upper right. Teton Basin, a broad, extensively farmed valley
-    in eastern Idaho, is at top. Photo by A. S. Post, University of
-    Washington, 1963._]
-
-Careful study of the fossils allows us to determine the age of each
-formation (table 3). Even more revealing, the fossils themselves are
-tangible evidence of the orderly parade of life that crossed the Teton
-landscape during more than 250 million years. Here is a record of
-Nature’s experiments with life, the triumphs, failures, the bizarre, the
-beautiful.
-
-    [Illustration: Table 2.—Paleozoic sedimentary rocks exposed in the
-    Teton region.]
-
- Age            Formation    Thickness   Description          Where exposed
-                             (feet)
-
- Permian        Phosphoria   150-250     Dolomite, gray,      North and west
-                 Formation                cherty, sandy,       flanks of Teton
-                                          black shale and      Range, north
-                                          phosphate beds;      flank of Gros
-                                          marine.              Ventre Mountains,
-                                                               southern Jackson
-                                                               Hole.
- Pennsylvanian  Tensleep     600-1,500   Tensleep Sandstone,  North and west
-                 and Amsden               light-gray, hard,    flanks of Teton
-                 Formations               underlain by         Range, north
-                                          Amsden Formation,    flank of Gros
-                                          a domolite and red   Ventre Mountains,
-                                          shale with a basal   southern Jackson
-                                          red sandstone;       Hole.
-                                          marine.
- Mississippian  Madison      1,000-1,200 Limestone,           North and west
-                 Limestone                blue-gray, hard,     flanks of Teton
-                                          fossiliferous;       Range, north
-                                          thin red shale in    flank of Gros
-                                          places near top;     Ventre Mountains,
-                                          marine.              southern Jackson
-                                                               Hole.
- Devonian       Darby        200-500     Dolomite, dark-gray  North and west
-                 Formation                to brown, fetid,     flanks of Teton
-                                          hard, and brown,     Range, north
-                                          black, and yellow    flank of Gros
-                                          shale; marine.       Ventre Mountains,
-                                                               southern Jackson
-                                                               Hole.
- Ordovician     Bighorn      300-500     Dolomite,            North and west
-                 Dolomite                 light-gray,          flanks of Teton
-                                          siliceous, very      Range, north and
-                                          hard; white dense    west flanks of
-                                          very fine-grained    Gros Ventre
-                                          dolomite at top;     Mountains,
-                                          marine.              southern Jackson
-                                                               Hole.
- Cambrian       Gallatin     180-300     Limestone, blue      North and west
-                 Limestone                gray, hard,          flanks of Teton
-                                          thin-bedded;         Range and Gros
-                                          marine.              Ventre Mountains.
-                Gros Ventre  600-800     Shale, green,        North and west
-                 Formation                flaky, with Death    flanks of Teton
-                                          Canyon Limestone     Range and Gros
-                                          Member composed of   Ventre Mountains.
-                                          about 300 feet of
-                                          hard cliff-forming
-                                          limestone in
-                                          middle; marine.
-                Flathead     175-200     Sandstone,           North and west
-                 Sandstone                reddish-brown,       flanks of Teton
-                                          very hard,           Range and Gros
-                                          brittle; partly      Ventre Mountains.
-                                          marine.
-
-The regularity and parallel relations of the layers in well-exposed
-sections such as the one in Alaska Basin suggest that all these rocks
-were deposited in a single uninterrupted sequence. However, the fossils
-and regional distribution of the rock units show that this is not really
-the case. The incomplete nature of this record becomes apparent if we
-plot the ages of the various formations on the absolute geologic time
-scale (fig. 34). The length of time from the beginning of the Cambrian
-Period to the end of the Mississippian Period is about 285 million
-years. The strata in Alaska Basin are a record of approximately 120
-million years. More than half of the pages in the geologic story are
-missing even though, compared with most other areas, the book as a whole
-is remarkably complete! During these unrecorded intervals of time either
-no sediments were deposited in the area of the Teton Range or, if
-deposited, they were removed by erosion.
-
-    [Illustration: Figure 32. _Paleozoic marine sedimentary rocks near
-    south boundary of Grand Teton National Park. View is south from top
-    of Teton Village tram. National Park Service photo by W. E. Dilley
-    and R. A. Mebane._]
-
-
-  Madison Limestone
-  Darby Formation
-  Bighorn Dolomite
-  Gallatin Limestone
-
-
-            Advance and retreat of Cambrian seas: an example
-
-The first invasion and retreat of the Paleozoic sea are sketched on
-figure 35. Early in Cambrian time a shallow seaway, called the
-_Cordilleran trough_, extended from southern California northeastward
-across Nevada into Utah and Idaho (fig. 35A). The vast gently rolling
-plain on Precambrian rocks to the east was drained by sluggish
-westward-flowing rivers that carried sand and mud into the sea. Slow
-subsidence of the land caused the sea to spread gradually eastward. Sand
-accumulated along the beaches just as it does today. As the sea moved
-still farther east, mud was deposited on the now-submerged beach sand.
-In the Teton area, the oldest sand deposit is called the Flathead
-Sandstone (fig. 36).
-
-The mud laid down on top of the Flathead Sandstone as the shoreline
-advanced eastward across the Teton area is now called the Wolsey Shale
-Member of the Gros Ventre Formation. Some shale shows patterns of cracks
-that formed when the accumulating mud was briefly exposed to the air
-along tidal flats. Small phosphatic-shelled animals called _brachiopods_
-inhabited these lonely tidal flats (fig. 37A and 37B) but as far as is
-known, nothing lived on land. Many shale beds are marked with faint
-trails and borings of wormlike creatures, and a few contain the remains
-of tiny very intricately developed creatures with head, eyes, segmented
-body, and tail. These are known as trilobites (fig. 37C and 37D).
-Descendants of these lived in various seas that crossed the site of the
-dormant Teton Range for the next 250 million years.
-
-    [Illustration: Figure 33. _View southwest across Alaska Basin,
-    showing tilted layers of Paleozoic sedimentary rocks on the west
-    flank of the Teton Range. National Park Service photo._]
-
-
-  Mount Meek
-  Madison Limestone
-  Bighorn Dolomite
-  Death Canyon Limestone Member
-  Flathead Sandstone
-  Precambrian Rock
-
-
-As the shoreline moved eastward, the Death Canyon Limestone Member of
-the Gros Ventre Formation (fig. 33) was deposited in clear water farther
-from shore. Following this the sea retreated to the west for a short
-time. In the shallow muddy water resulting from this retreat the Park
-Shale Member of the Gros Ventre Formation was deposited. In places
-underwater “meadows” of algae flourished on the sea bottom and built
-extensive reefs (fig. 38A). From time to time shoal areas were hit by
-violent storm waves that tore loose platy fragments of recently
-solidified limestone and swept them into nearby channels where they were
-buried and cemented into thin beds of jumbled fragments (fig. 38B)
-called _“edgewise” conglomerate_. These are widespread in the shale and
-in overlying and underlying limestones.
-
-    [Illustration: Table 3. _Formations exposed in Alaska Basin._]
-
-   AGE (Numbers    FORMATION (Thickness)     ROCKS AND FOSSILS
-    show age in
-    millions of
-      years)
-
-       (310)
-   MISSISSIPPIAN   MADISON LIMESTONE         Uniform thin beds of
-                   (Total about 1,100        blue-gray limestone and
-                   feet, but only lower      sparse very thin layers of
-                   300 feet preserved in     shale. Brachiopods, corals,
-                   this section)             and other fossils abundant.
-       (345)
-     LATE AND      DARBY FORMATION (About    Thin beds of gray and buff
-  MIDDLE DEVONIAN  350 feet)                 dolomite interbedded with
-                                             layers of gray, yellow, and
-                                             black shale. A few fossil
-                                             brachiopods, corals, and
-                                             bryozoans.
-       (390)
-       (425)
-     LATE AND      BIGHORN DOLOMITE (About   Thick to very thin beds of
-      MIDDLE       450 feet; Leigh           blue-gray or brown dolomite,
-    ORDOVICIAN     Dolomite Member about     white on weathered surfaces.
-                   40 feet thick at top)     A few broken fossil
-                                             brachiopods, bryozoans, and
-                                             horn corals. Thin beds of
-                                             white fine-grained dolomite
-                                             at top are the Leigh Member.
-       (440)
-       (500)
-   LATE CAMBRIAN   GALLATIN LIMESTONE (180   Blue-gray limestone mottled
-                   feet)                     with irregular rusty or
-                                             yellow patches. Trilobites
-                                             and brachiopods.
-       (530)
-  MIDDLE CAMBRIAN  GROS VENTRE FORMATION
-                       PARK SHALE MEMBER     Gray-green shale containing
-                       (220 feet)            beds of platy limestone
-                                             conglomerate. Trilobites,
-                                             brachiopods, and fossil algal
-                                             heads.
-                       DEATH CANYON          Two thick beds of
-                       LIMESTONE MEMBER      dark-blue-gray limestone
-                       (285 feet)            separated by 15 to 20 feet of
-                                             shale that locally contains
-                                             abundant fossil brachiopods
-                                             and trilobites.
-                       WOLSEY SHALE MEMBER   Soft greenish-gray shale
-                       (100 feet)            containing beds of purple and
-                                             green sandstone near base. A
-                                             few fossil brachiopods.
-                   FLATHEAD LIMESTONE (175   Brown, maroon, and white
-                   feet)                     sandstone, locally containing
-                                             many rounded pebbles of
-                                             quartz and feldspar. Some
-                                             beds of green shale at top.
-       (570)
-    PRECAMBRIAN                              Granite, gneiss, and
-                                             pegmatite.
-
-    [Illustration: Figure 34. _Absolute ages of the formations in Alaska
-    Basin. Shaded parts of the scale show intervals for which there is
-    no record._]
-
- STRATIGRAPHIC SCALE                     ABSOLUTE     ENLARGED PIECE OF
-                                         TIME (Years  YARDSTICK SHOWN ON
-                                         ago)         FIGURE 19
-
-                                                      2
- PALEZOIC     PENNSYLVANIAN ?
-                                         300 million
-              MISSISSIPPIAN MADISON
-              DEVONIAN      DARBY
-                                                      3
-                                         400 million
-              SILURIAN
-              ORDOVICIAN    BIGHORN
-                                         500 million  4
-              CAMBRIAN      GALLATIN
-                            GROS VENTRE
-                            FLATHEAD
-                                         600 million
- PRECAMBRIAN                                          5
-
-    Figure 35. _The first invasions of the Paleozoic sea._
-
-    [Illustration: A. _In Early Cambrian time an arm of the Pacific
-    Ocean occupied a deep trough in Idaho, Nevada, and part of Utah. The
-    land to the east was a broad gently rolling plain of Precambrian
-    rocks drained by sluggish westward-flowing streams. The site of the
-    Teton Range was part of this plain. Slow subsidence of the land
-    caused the sea to move eastward during Middle Cambrian time flooding
-    the Precambrian plain._]
-
-    [Illustration: B. _By Late Cambrian time the sea had drowned all of
-    Montana and most of Wyoming. The Flathead Sandstone and Gros Ventre
-    Formation were deposited as the sea advanced. The Gallatin Limestone
-    was being deposited when the shoreline was in about the position
-    shown in this drawing._]
-
-    [Illustration: C. _In Early Ordovician time uplift of the land
-    caused the sea to retreat back into the trough, exposing the
-    Cambrian deposits to erosion. Cambrian deposits were partly stripped
-    off of some areas. The Bighorn Dolomite was deposited during the
-    next advance of the sea in Middle and Late Ordovician time._]
-
-    [Illustration: Figure 36. _Conglomeratic basal bed of Flathead
-    Sandstone and underlying Precambrian granite gneiss; contact is
-    indicated by a dark horizontal line about 1 foot below hammer. This
-    contact is all that is left to mark a 2-billion year gap in the rock
-    record of earth history. The locality is on the crest of the Teton
-    Range 1 mile northwest of Lake Solitude._]
-
-Once again the shoreline crept eastward, the seas cleared, and the
-Gallatin Limestone was deposited. The Gallatin, like the Death Canyon
-Limestone Member, was laid down for the most part in quiet, clear water,
-probably at depths of 100 to 200 feet. However, a few beds of “edgewise”
-conglomerate indicate the occurrence of sporadic storms. At this time,
-the sea covered all of Idaho and Montana and most of Wyoming (fig. 35B)
-and extended eastward across the Dakotas to connect with shallow seas
-that covered the eastern United States. Soon after this maximum stage
-was reached slow uplift caused the sea to retreat gradually westward.
-The site of the Teton Range emerged above the waves, where, as far as is
-now known, it may have been exposed to erosion for nearly 70 million
-years (fig. 35C).
-
-The above historical summary of geologic events in Cambrian time is
-recorded in the Cambrian formations. This is an example of the
-reconstructions, based on the sedimentary rock record, that have been
-made of the Paleozoic systems in this area.
-
-    Figure 37. _Cambrian fossils in Grand Teton National Park._
-
-    A-B. _Phosphatic-shelled brachiopods, the oldest fossils found in
-    the park. Actual width of specimens is about ¼ inch._
-
-    C-D. _Trilobites. Width of C is ¼ inch, D is ½ inch. National Park
-    Service photos by W. E. Dilley and R. A. Mebane._
-
-    [Illustration: A.]
-
-    [Illustration: B.]
-
-    [Illustration: C.]
-
-    [Illustration: D.]
-
-
-                      Younger Paleozoic formations
-
-Formations of the remaining Paleozoic systems are likewise of interest
-because of the ways in which they differ from those already described.
-
-    Figure 38. _Distinctive features of Cambrian rocks._
-
-    [Illustration: A. _Algal heads in the Park Shale Member of the Gros
-    Ventre Formation. These calcareous mounds were built by algae
-    growing in a shallow sea in Cambrian time. They are now exposed on
-    the divide between North and South Leigh Creeks, nearly 2 miles
-    above sea level!_]
-
-    [Illustration: B. _Bed of “edgewise” conglomerate in the Gallatin
-    Limestone. Angular plates of solidified lime-ooze were torn from the
-    sea bottom by storm waves, swept into depressions, and then buried
-    in lime mud. These fragments, seen in cross section, make the
-    strange design on the rock. Thin limestone beds below are
-    undisturbed. National Park Service photo by W. E. Dilley._]
-
-The Bighorn Dolomite of Ordovician age forms ragged hard massive
-light-gray to white cliffs 100 to 200 feet high (figs. 32 and 33).
-_Dolomite_ is a calcium-magnesium carbonate, but the original sediment
-probably was a calcium carbonate mud that was altered by magnesium-rich
-sea water shortly after deposition. Corals and other marine animals were
-abundant in the clear warm seas at this time.
-
-Dolomite in the Darby Formation of Devonian age differs greatly from the
-Bighorn Dolomite; that in the Darby is dark-brown to almost black, has
-an oily smell, and contains layers of black, pink, and yellow mudstone
-and thin sandstone. The sea bottom during deposition of these rocks was
-foul and frequently the water was turbid. Abundant fossil fragments
-indicate fishes were common for the first time. Exposures of the Darby
-Formation are recognizable by their distinctive dull-yellow thin-layered
-slopes between the prominent gray massive cliffs of formations below and
-above.
-
-The Madison Limestone of Mississippian age is 1,000 feet thick and is
-exposed in spectacular vertical cliffs along canyons in the north, west,
-and south parts of the Tetons. It is noted for the abundant remains of
-beautifully preserved marine organisms (fig. 39). The fossils and the
-relatively pure blue-gray limestone in which they are embedded indicate
-deposition in warm tranquil seas. The beautiful Ice Cave on the west
-side of the Tetons and all other major caves in the region were
-dissolved out of this rock by underground water.
-
-The Pennsylvanian System is represented by the Amsden Formation and the
-Tensleep Sandstone. Cliffs of the Tensleep Sandstone can be seen along
-the Gros Ventre River at the east edge of the park. The Amsden, below
-the Tensleep, consists of red and green shale, sandstone, and thin
-limestone. The shale is especially weak and slippery when exposed to
-weathering and saturated with water. These are the strata that make up
-the glide plane of the Lower Gros Ventre Slide (fig. 5) east of the
-park.
-
-The Phosphoria Formation and its equivalents of Permian age are unlike
-any other Paleozoic rocks because of their extraordinary content of
-uncommon elements. The formation consists of sandy dolomite, widespread
-black phosphate beds and black shale that is unusually rich not only in
-phosphorus, but also in vanadium, uranium, chromium, zinc, selenium,
-molybdenum, cobalt, and silver. The formation is mined extensively in
-nearby parts of Idaho and in Wyoming for phosphatic fertilizer, for the
-chemical element phosphorus, and for some of the metals that can be
-derived from the rocks as byproducts. These elements and compounds are
-not everywhere concentrated enough to be of economic interest, but their
-dollar value is, in a regional sense, comparable to that of some of the
-world’s greatest mineral deposits.
-
-    Figure 39. _A glimpse of the sea floor during deposition of the
-    Madison Limestone 330 million years ago, showing the remains of
-    brachiopods, corals, and other forms of life that inhabited the
-    shallow warm water._
-
-    [Illustration: A. _Slab in which fossils are somewhat broken and
-    scattered. Scale slightly reduced. National Park Service photo by W.
-    E. Dilley and R. A. Mebane._]
-
-    [Illustration: B. _Slab in which fossils are remarkably complete.
-    Silver dollar gives scale. Specimen is in University of Wyoming
-    Geological Museum._]
-
-
-
-
-                     THE MESOZOIC—ERA OF TRANSITION
-
-
-The Mesozoic Era in the Teton region was a time of alternating marine,
-transitional, and continental environments. Moreover, the highly
-diversified forms of life, ranging from marine mollusks to tremendous,
-land-living dinosaurs, confirm and reinforce the story of the rocks.
-Living things, too, were in transition, for as environment changed, many
-forms moved from the sea to land in order to survive. It was the time
-when some of the most spectacularly colored rock strata of the region
-were deposited.
-
-
-                     Colorful first Mesozoic strata
-
-Bright-red soft Triassic rocks more than 1,000 feet thick, known as the
-Chugwater Formation, comprise most of the basal part of the Mesozoic
-sequence (table 4). They form colorful hills east and south of the park.
-The red color is caused by a minor amount of iron oxide. Mud cracks and
-the presence of fossil reptiles and amphibians indicate deposition in a
-tidal flat environment, with the sea lying several miles southwest of
-Jackson Hole. A few beds of white _gypsum_ (calcium sulfate) are
-present; they were apparently deposited during evaporation of shallow
-bodies of salt water cut off from the open sea.
-
-As the Triassic Period gave way to the Jurassic, salmon-red windblown
-sand (Nugget Sandstone) spread across the older red beds and in turn was
-buried by thin red shale and thick gypsum deposits of the Gypsum Spring
-Formation. Then down from Alaska and spreading across most of Wyoming
-came the _Sundance Sea_, a warm, muddy, shallow body of water that
-teemed with marine mollusks. In it more than 500 feet of highly
-fossiliferous soft gray shale and thin limestones and sandstones were
-deposited. The sea withdrew and the Morrison and Cloverly Formations
-(Jurassic and Lower Cretaceous) were deposited on low-lying tropical
-humid flood plains. These rocks are colorful, consisting of red, pink,
-purple, and green badland-forming claystones and mudstones, and yellow
-to buff sandstones. Vegetation was abundant and large and small
-dinosaurs roamed the countryside or inhabited the swamps.
-
-    [Illustration: Table 4.—Mesozoic sedimentary rocks exposed in the
-    Teton region.]
-
- Age Formation        Thickness    Description          Where exposed
-                      (feet)
-
- CRETACEOUS
-     Harebell         0-5,000      Sandstone, olive     Eastern and
-     Formation                     drab, silty, drab    northeastern parts
-                                   siltstone, and       of Jackson Hole.
-                                   dark-gray shale;
-                                   thick beds of
-                                   quartzite pebble
-                                   conglomerate in
-                                   upper part.
-     Meeteetse        0-700        Sandstone, gray to   Spread Creek area.
-     Formation                     chalky white,
-                                   blue-green to gray
-                                   siltstone, thin
-                                   coal, and green to
-                                   yellow bentonite.
-     Mesaverde        0-1,000      Sandstone, white,    Eastern Jackson
-     Formation                     massive, soft, thin  Hole.
-                                   gray shale, sparse
-                                   coal.
-     Unnamed          3,500±       Sandstone and        Eastern Jackson
-     sequence of                   shale, gray to       Hole and eastern
-     lenticular                    brown; abundant      margin of the park.
-     sandstone,                    coal in lower 2,000
-     shale, and                    feet.
-     coal.
-     Bacon Ridge      900-1,200    Sandstone, light     Eastern Jackson
-     Sandstone                     gray, massive,       Hole and eastern
-                                   marine, gray shale,  margin of the park.
-                                   many coal beds.
-     Cody Shale       1,300-2,200  Shale, gray, soft;   Eastern and
-                                   thin green           northern parts of
-                                   sandstone, some      Jackson Hole.
-                                   bentonite; marine.
-     Frontier         1,000        Sandstone, gray,     Eastern and
-     Formation                     and black to gray    northern parts and
-                                   shale, marine; many  south-western
-                                   persistent white     margin of Jackson
-                                   bentonite beds in    Hole.
-                                   lower part.
-     Mowry Shale      700          Shale,               Gros Ventre River
-                                   silvery-gray, hard,  Valley, northern
-                                   siliceous, with      margin of the park,
-                                   many fish scales;    and southern part
-                                   thin bentonite       of Jackson Hole.
-                                   beds; marine.
-     Thermopolis      150-200      Shale, black, soft,  Gros Ventre River
-     Shale                         fissile, with        Valley, northern
-                                   persistent           margin of the park,
-                                   sandstone at top;    and southern part
-                                   marine.              of Jackson Hole.
-     Cloverly and     650          Sandstone, light     North end of Teton
-     Morrison(?)                   gray, sparkly,       Range and Gros
-     Formations                    rusty near top,      Ventre River Valley.
-                                   underlain by
-                                   variegated soft
-                                   claystone; basal
-                                   part is silty
-                                   dully-variegated
-                                   sandstone and
-                                   claystone.
- JURASSIC
-     Sundance         500-700      Sandstone, green,    North end of Teton
-     Formation                     underlain by soft    Range, Blacktail
-                                   gray shale and thin  Butte, Gros Ventre
-                                   highly               River Valley.
-                                   fossiliferous
-                                   limestones; marine.
-     Gypsum Spring    75-100       Gypsum, white,       North end of Teton
-     Formation                     interbedded with     Range, Blacktail
-                                   red shale and gray   Butte, Gros Ventre
-                                   dolomite; partly     River Valley.
-                                   marine.
-     Nugget           0-350        Sandstone,           North flank of Gros
-     Sandstone                     salmon-red, hard.    Ventre Mountains,
-                                                        southern Jackson
-                                                        Hole.
- TRIASSIC
-     Chugwater        1,000-1,500  Siltstone and        North flank of Gros
-     Formation                     shale, red,          Ventre Mountains,
-                                   thin-bedded; one     north end of Teton
-                                   thin marine          Range, southernmost
-                                   limestone in upper   Jackson Hole.
-                                   third.
-     Dinwoody         200-400      Siltstone, brown,    North flank of Gros
-     Formation                     hard, thin-bedded;   Ventre Mountains,
-                                   marine.              north end of Teton
-                                                        Range, southernmost
-                                                        Jackson Hole.
-
-
-                         Drab Cretaceous strata
-
-The youngest division of the _Mesozoic_ Era is the Cretaceous Period.
-Near the beginning of this period, brightly colored rocks continued to
-be deposited. Then, the Teton region, as well as most of Wyoming, was
-partly, and at times completely, submerged by shallow muddy seas. As a
-result, the brightly variegated strata were covered by 10,000 feet of
-generally drab-colored sand, silt, and clay containing some coal beds,
-volcanic ash layers, and minor amounts of gravel.
-
-The Cretaceous sea finally retreated eastward from the Teton region
-about 85 million years ago, following the deposition of the Bacon Ridge
-Sandstone (fig. 40). As it withdrew, extensive coal swamps developed
-along the sea coast. The record of these swamps is preserved in coal
-beds 5 to 10 feet thick in the Upper Cretaceous deposits. The coal beds
-are now visible in abandoned mines along the east margin of the park.
-Coal is formed from compacted plant debris; about 5 feet of this
-material is needed to form 1 inch of coal. Thus, lush vegetation must
-have flourished for long periods of time, probably in a hot wet climate
-similar to that now prevailing in the Florida Everglades.
-
-Sporadically throughout Cretaceous time fine-grained ash was blown out
-of volcanoes to the west and northwest and deposited in quiet shallow
-water. Subsequently the ash was altered to a type of clay called
-_bentonite_ that is used in the foundry industry and in oil well
-drilling muds. In Jackson Hole, the elk and deer lick bentonite
-exposures to get a bitter salt and, where the beds are water-saturated,
-enjoy “stomping” on them. Bentonite swells when wet and causes many
-landslides along access roads into Jackson Hole (fig. 17).
-
-The Cretaceous rocks in the Teton region are part of an enormous
-east-thinning wedge that here is nearly 2 miles thick. Most of the
-debris was derived from slowly rising mountains to the west.
-
-Cretaceous sedimentary rocks are much more than of just scientific
-interest; they contain mineral deposits important to the economy of
-Wyoming and of the nation. Wyoming leads the States in production of
-bentonite, all of it from Cretaceous rocks. These strata have yielded
-far more oil and gas than any other geologic system in the State and the
-production is geographically widespread. They also contain enormous coal
-reserves, some in beds between 50 and 100 feet thick. The energy
-resources alone of the Cretaceous System in Wyoming make it invaluable
-to our industrialized society.
-
-    [Illustration: Figure 40. _The yardstick and the sea. The shaded
-    part of the yardstick shows the 500-million-year interval during
-    which Paleozoic and Mesozoic seas swept intermittently across the
-    future site of the Tetons. When they finally withdrew about 85
-    million years ago, a little more than 5/8 of an inch of the
-    yardstick remained to be accounted for._]
-
-                 ABSOLUTE TIME (Millions of years ago)      INCHES
-
-  {submerged}                    85-585                      ⅝-4⅝
-  CENOZOIC                        0-80                       0-½
-  MESOZOIC                       80-180                      ½-⅞
-  PALEOZOIC                     180-570                      ⅞-4⅞
-  PRECAMBRIAN                     570-                       4⅞-
-
-As the end of the Cretaceous Period approached, slightly more than 80
-million years ago, the flat monotonous landscape (fig. 41) which had
-prevailed during most of Late Cretaceous time gave little hint that the
-stage was set for one of the most exciting and important chapters in the
-geologic history of North America.
-
-
-                      Birth of the Rocky Mountains
-
-The episode of mountain building that resulted in formation of the
-ancestral Rocky Mountains has long been known as the _Laramide
-Revolution_. West and southwest of Wyoming, mountains had already
-formed, the older ones as far away as Nevada and as far back in time as
-Jurassic, the younger ones rising progressively farther east, like giant
-waves moving toward a coast. The first crustal movement in the Teton
-area began in latest Cretaceous time when a broad low northwest-trending
-arch developed in the approximate area of the present Teton Range and
-Gros Ventre Mountains. However, this uplift bore no resemblance to the
-Tetons as we know them today for the present range formed 70 million
-years later.
-
-    [Illustration: Figure 41. _Grand Teton National Park region slightly
-    more than 80 million years ago, just before onset of Laramide
-    Revolution. The last Cretaceous sea still lingered in central
-    Wyoming._]
-
-One bit of evidence (there are others) of the first Laramide mountain
-building west of the Tetons is a tremendous deposit of quartzite boulder
-debris (several hundred cubic miles in volume) derived from the _Targhee
-uplift_ (fig. 42). Nowhere is the uplift now exposed, but from the size,
-composition, and distribution of rock fragments that came from it, we
-know that it was north and west of the northern end of the present-day
-Teton Range. Powerful streams carried boulders, sand, and clay eastward
-and southeastward across the future site of Jackson Hole and deposited
-them in the Harebell Formation (table 4). Mingled with this sediment
-were tiny flakes of gold and a small amount of mercury. Fine-grained
-debris was carried still farther east and southeast into two enormous
-depositional troughs in central and southern Wyoming. Most of the large
-rock fragments were derived from Precambrian and possibly lower
-Paleozoic quartzites. This means that at least 15,000 feet of overlying
-Paleozoic and Mesozoic strata must first have been stripped away from
-the Targhee uplift before the quartzites were exposed to erosion.
-
-    [Illustration: Figure 42. _Teton region at the end of Cretaceous
-    time about 65 million years ago. The ancestral Teton-Gros Ventre
-    uplift had risen and prominent southeastward drainage from the
-    Targhee uplift was well established. See figure 41 for State lines
-    and location map._]
-
-Remains of four-legged horned ceratopsian dinosaurs, possibly
-_Triceratops_ (fig. 43), reflecting the last population explosion of
-these reptiles, have been found in pebbly sandstone of the Harebell
-Formation in highway cuts on the Togwotee Pass road 8 miles east of the
-park.
-
-    [Illustration: Figure 43. _Triceratops, a horned dinosaur of the
-    type that inhabited Jackson Hole about 65 million years ago. Sketch
-    by S. H. Knight._]
-
-Near the end of Cretaceous time, broad gentle uplifts also began to stir
-at the sites of future mountain ranges in many parts of Wyoming. The
-ancestral Teton-Gros Ventre arch continued to grow. Associated with and
-parallel to it was a series of sharp steepsided elongated
-northwest-trending upfolds (_anticlines_). One of these can be seen
-where it crosses the highway at the Lava Creek Campground near the
-eastern margin of Grand Teton National Park.
-
-During these episodes of mountain building, erosion, and deposition, the
-dinosaurs became extinct all over the world. The “Age of Mammals” was
-about to begin.
-
-
-
-
-       TERTIARY—TIME OF MAMMALS, MOUNTAINS, LAKES, AND VOLCANOES
-
-
-    [Illustration: Figure 44. _The last inch of the yardstick, enlarged
-    to show subdivisions of the Cenozoic Era._]
-
-  STRATIGRAPHIC SCALE        THE LAST INCH OF    ABSOLUTE TIME (million
-                             THE YARDSTICK       years ago)
-
-  CENOZOIC
-     QUATERNARY
-          Recent and         0                   0
-          Pleistocene
-     TERTIARY
-          Pliocene           0                   0
-          Miocene            ⅛                   12
-          Oligocene          ¼                   25
-          Eocene             ⅜                   40
-          Paleocene          ⁷/₁₆                55
-  MESOZOIC
-     CRETACEOUS              ½                   65
-
-The Cenozoic (table 1), last and shortest of the geologic eras,
-comprises the Tertiary and Quaternary Periods. It began about 65 million
-years ago and is represented by only the final one-half inch of our
-imaginary yardstick of time (fig. 19). Nevertheless, it is the era
-during which the Tetons rose in their present form and the landscape was
-sculptured into the panorama of beauty that we now see. In order to show
-the many Tertiary and Quaternary events in the Teton region, it is
-necessary to enlarge greatly the last part of the yardstick (fig. 44).
-There are two reasons for the extraordinarily clear and complete record.
-First, the Teton region was a relatively active part of the earth’s
-crust, characterized by many downdropped blocks. The number of events is
-great and their records are preserved in sediments trapped in the
-subsiding basins. Second, the geologically recent past is much easier to
-see than the far dimmer, distant past; the rocks that record later
-events are fresher, less altered, more complete, and more easily
-interpreted than are those that tell us of older events.
-
-    [Illustration: Table 5.—Cenozoic sedimentary rocks and
-    unconsolidated deposits in the Teton region.]
-
- Age   Formation      Thickness   Description          Where exposed
-                      (feet)
-
- QUATERNARY
-    Recent
-       Modern         0-200±      Sand, gravel, and    Floor of Jackson
-       stream,                    silt along present   Hole and in canyons
-       landslide,                 streams; jumbled     and on
-       glacial and                broken rock in       mountainsides
-       talus deposits             landslides and on    throughout the
-                                  talus slopes;        region.
-                                  debris around
-                                  existing glaciers.
-    Pleistocene
-       Glacial        0-200±      Gravel, sand, silt,  Floor of Jackson
-       deposits and               and glacial debris.  Hole.
-       loess
-       Unnamed upper  0-500       Shale, brown-gray,   Gros Ventre River
-       lake sequence              sandstone, and       Valley.
-                                  conglomerate.
-       Unnamed lower  0-200       Shale, siltstone,    National Elk Refuge.
-       lake sequence              and sandstone,
-                                  gray, green, and
-                                  red.
- ?  Pleistocene or Pliocene
-       Bivouac        0-1,000     Conglomerate, with   Signal Mountain and
-       Formation                  purplish-gray        West Gros Ventre
-                                  welded tuff in       Butte.
-                                  upper part.
- TERTIARY
-    Pliocene
-       Teewinot       0-6,000     Limestone, tuff,     National Elk
-       Formation                  and claystone,       Refuge, Blacktail
-                                  white, soft.         Butte, and eastern
-                                                       margin of Antelope
-                                                       Flat.
-       Camp Davis     0-5,500     Conglomerate, red    Southernmost tip of
-       Formation                  and gray, with       Jackson Hole.
-                                  white tuff,
-                                  diatomite, and red
-                                  and white claystone.
-    Miocene
-       Colter         0-7,000     Volcanic             Pilgrim and Ditch
-       Formation                  conglomerate, tuff,  Creeks, and north
-                                  and sandstone,       end of Teton Range.
-                                  white to
-                                  green-brown, with
-                                  locally-derived
-                                  basalt and andesite
-                                  rock fragments.
-    Oligocene
-       Wiggins        0-3,000     Volcanic             Eastern margin of
-       Formation                  conglomerate, gray   Jackson Hole.
-                                  to brown, with
-                                  white tuff layers.
-    Eocene
-       Unnamed upper  0-1,000     Tuff, conglomerate,  Eastern margin of
-       and middle                 sandstone, and       Jackson Hole.
-       Eocene                     claystone, green,
-       sequence                   underlain by
-                                  variegated
-                                  claystone and
-                                  quartzite pebble
-                                  conglomerate.
-       Wind River     2,000-3,000 Claystone and        Eastern margin of
-       and Indian                 sandstone,           Jackson Hole.
-       Meadows                    variegated, and
-       Formations                 locally-derived
-                                  conglomerate;
-                                  persistent coal and
-                                  gray shale zone in
-                                  middle.
-    Paleocene
-       Unnamed        1,000-2,000 Sandstone and        Eastern margin of
-       greenish-gray              claystone,           Jackson Hole.
-       and brown                  greenish-gray and
-       sandstone and              brown,
-       claystone                  intertonguing at
-       sequence                   base with quartzite
-                                  pebble conglomerate.
-       Pinyon         500-5,000   Conglomerate,        Eastern part of
-       Conglomerate               brown, chiefly of    Jackson Hole, Mt.
-                                  rounded quartzite;   Leidy and Pinyon
-                                  coal and claystone   Peak Highlands, and
-                                  locally at base.     north end of Teton
-                                                       Range.
-
-    [Illustration: Figure 45. _Pinyon Conglomerate of Paleocene age,
-    along the northwest margin of the Teton Range._]
-
-During the early part of the Tertiary Period, mountain building and
-basin subsidence were the dominant types of crustal movement. Seas
-retreated southward down the Mississippi Valley and never again invaded
-the Teton area. Environments on the recently uplifted land were diverse
-and favorable for the development of new forms of plants and animals.
-
-
-                      Rise and burial of mountains
-
-The enormous section of Tertiary sedimentary rocks in the Jackson Hole
-area (table 5) is one of the most impressive in North America. If the
-maximum thicknesses of all formations were added, they would total more
-than 6 miles, but nowhere did this amount of rock accumulate in a single
-unbroken sequence. No other region in the United States contains a
-thicker or more complete nonmarine Tertiary record; many areas have
-little or none. The accumulation in Jackson Hole reflects active uplifts
-of nearby mountains that supplied abundant rock debris, concurrent
-sinking of nearby basins in which the sediments could be preserved, and
-proximity to the great Yellowstone-Absaroka volcanic area, one of the
-most active continental volcanic fields in the United States. The volume
-and composition of the Tertiary strata are, therefore, clear evidence of
-crustal and subcrustal instability.
-
-    [Illustration: Figure 46. _Teton region near end of deposition of
-    Paleocene rocks, slightly less than 60 million years ago. The
-    ancestral Teton-Gros Ventre uplift formed a partial barrier between
-    the Jackson Hole and Green River depositional basins; major
-    drainages from the Targhee uplift spread an enormous sheet of gravel
-    for 100 miles to the east. See figure 41 for State lines and
-    location map._]
-
-The many thick layers of conglomerate are evidence of rapid erosion of
-nearby highlands. The Pinyon Conglomerate (fig. 45), for example,
-contains zones as much as 2,500 feet thick of remarkably well-rounded
-pebbles, cobbles, and boulders, chiefly of quartzite identical with that
-in the underlying Harebell Formation and derived from the same source,
-the Targhee uplift. Like the Harebell the matrix contains small amounts
-of gold and mercury. Rock fragments increase in size northwestward
-toward the source area (fig. 46) and most show percussion scars,
-evidence of ferocious pounding that occurred during transport by
-powerful, swift rivers and steep gradients.
-
-    [Illustration: Figure 47. _Teton region at climax of Laramide
-    Revolution, between 50 and 55 million years ago. See figure 41 for
-    State lines and location map._]
-
-Conglomerates such as the Pinyon are not the only clue to the time of
-mountain building. Another type of evidence—faults—is demonstrated in
-figure 16. The youngest rocks cut by a fault are always older than the
-fault. Many faults and the rocks on each side are covered by still
-younger unbroken sediments. These must, therefore, have been deposited
-after fault movement ceased. By dating both the faulted and the
-overlying unbroken sediments, the time of fault movement can be
-bracketed.
-
-Observations of this type in western Wyoming indicate that the Laramide
-Revolution reached a climax during earliest Eocene time, 50 to 55
-million years ago. Mountain-producing upwarps formed during this episode
-were commonly bounded on one side by either reverse or thrust faults
-(fig. 16B and 16C) and intervening blocks were downfolded into large,
-very deep basins. The amount of movement of the mountain blocks over the
-basins ranged from tens of miles in the Snake River, Salt River,
-Wyoming, and Hoback Ranges directly south of the Tetons to less than 5
-miles on the east margin of Jackson Hole (the west flank of the Washakie
-Range shown in figure 1). The ancestral Teton-Gros Ventre uplift
-continued to rise but remained one of the less conspicuous mountain
-ranges in the region (fig. 47).
-
-The Buck Mountain fault, the great reverse fault which lies just west of
-the highest Teton peaks (see geologic map and cross section), was formed
-either at this time or during a later episode of movement that also
-involved the southwest margin of the Gros Ventre Mountains. The Buck
-Mountain fault is of special importance because it raised a segment of
-Precambrian rocks several thousand feet. Later, when the entire range as
-we now know it was uplifted by movement along the Teton fault, the hard
-basement rocks in this previously upfaulted segment continued to stand
-much higher than those in adjacent parts of the range. All of the major
-peaks in the Tetons are carved from this doubly uplifted block.
-
-The brightly colored sandstone, mudstone, and claystone in the Indian
-Meadows and Wind River Formations (lower Eocene) in the eastern part of
-Jackson Hole were derived from variegated Triassic, Jurassic, and Lower
-Cretaceous rocks exposed on the adjacent mountain flanks. Fossils in
-these Eocene Formations show that it took less than 10 million years for
-the uplifts to be deeply eroded and partially buried in their own
-debris.
-
-The Laramide Revolution in the area of Grand Teton National Park ended
-during Eocene time between 45 and 50 million years ago, and as the
-mountains and basins became stabilized a new element was added.
-Volcanoes broke through to the surface in many parts of the
-Yellowstone-Absaroka area and the constantly increasing volume of their
-eruptive debris was a major factor in the speed of filling of basins and
-burial of mountains throughout Wyoming. This entire process only took
-about 20 million years, and along the east margin of Jackson Hole it was
-largely completed during Oligocene time (fig. 48). However, east and
-northeast of Jackson Lake a Miocene downwarp subsequently formed and in
-it accumulated at least 7,000 feet of locally derived sediments of
-volcanic origin.
-
-    [Illustration: Figure 48. _Teton region near the close of Oligocene
-    deposition, between 25 and 30 million years ago, showing areas of
-    major volcanoes and lava flows. See figure 41 for State lines and
-    location map._]
-
-
-                           The First Big Lake
-
-_Teewinot Lake_ (fig. 49), the first big freshwater lake in Jackson
-Hole, was formed during Pliocene time, about 10 million years ago, and
-in it the Teewinot Formation was deposited. These lake strata consist of
-more than 5,000 feet of white limestone, thin-bedded claystone, and
-_tuff_ (solidified ash made up of tiny fragments of volcanic rock and
-splinters of volcanic glass). The claystones contain fossil snails,
-clams, beaver bones and teeth, aquatic mice, suckers, and other fossils
-that indicate deposition in a shallow freshwater lake environment. These
-beds underlie Jackson Lake Lodge, the National Elk Refuge, part of
-Blacktail Butte, and are conspicuously exposed in white outcrops that
-look like snowbanks on the upper slopes along the east margin of the
-park across the valley from the Grand Teton.
-
-    [Illustration: Figure 49. _Teton region near close of middle
-    Pliocene time, about 5 million years ago, showing areas of major
-    volcanoes and lava flows. See figure 41 for State lines and location
-    map._]
-
-Teewinot Lake was formed on a down-faulted block and was dammed behind
-(north of) a fault that trends east across the floor of Jackson Hole at
-the south boundary of the park. Lakes are among the most short-lived of
-earth features because the forces of nature soon conspire to fill them
-up or empty them. This lake existed for perhaps 5 million years during
-middle Pliocene time; it was shallow, and remained so despite the
-pouring in of a mile-thick layer of sediment. This indicates that
-downdropping of the lake floor just about kept pace with deposition.
-
-    [Illustration: Figure 50. _Restoration of a middle Eocene landscape
-    showing some of the more abundant types of mammals. Mural painting
-    by Jay H. Matterness; photo courtesy of the Smithsonian
-    Institution._]
-
-  _Uintatherium_             6-horned, saber-toothed plant eater
-  _Stylinodon_               gnawing-toothed mammal
-  _Palaeosyops_              early titanothere
-  _Helaletes_                primitive tapir
-  _Sciuravus_                squirrel-like rodent
-  _Smilodectes_              lemurlike monkey
-  _Trogosus_                 gnawing-toothed mammal
-  _Hyrachyus_                fleet-footed rhinoceros
-  _Ischyrotomus_             marmotlike rodent
-  _Homacodon_                even-toed hoofed animal
-  _Orohippus_                ancestral horse
-  _Patriofelis_              large flesh eater
-  _Mesonyx_                  hyenalike mammal
-  _Helohyus_                 even-toed hoofed mammal
-  _Metacheiromys_            armadillolike edentate
-  _Machaeroides_             saber-toothed mammal
-  _Hyopsodus_                clawed, plant-eating mammal
-  _Saniwa_                   monitorlike lizard
-  _Crocodilus_               crocodile
-  _Echmatemys_               turtle
-
-Other lakes formed in response to similar crustal movements in nearby
-places. One such lake, _Grand Valley Lake_ (fig. 49), formed about 25
-miles southwest of Teewinot Lake; both contained sediments with nearly
-the same thickness, composition, appearance, age, and fossils. Although
-these two lakes are on opposite sides of the Snake River Range, the
-ancestral Snake River apparently flowed through a canyon previously cut
-across the range and provided a direct connection between them.
-
-
-                         Development of mammals
-
-The Cenozoic Era is known as the “Age of Mammals.” Small mammals had
-already existed, though quite inconspicuously, in Wyoming for about 90
-million years before Paleocene time. Then about 65 million years ago
-their proliferation began as a result of the extinction of dinosaurs,
-obliteration of seaways that were barriers to distribution, and the
-development of new and varied types of environment. These new
-environments included savannah plains, low hills and high mountains,
-freshwater lakes and swamps, and extensive river systems. The mammals
-increased in size and, for the first time, became abundant in numbers of
-both species and individuals. The development and widespread
-distribution of grasses and other forage on which many of the animals
-depended were highly significant. Successful adaptation of _herbivores_
-(vegetation-eating animals) led, in turn, to increased varieties and
-numbers of predatory _carnivores_ (meat-eating animals).
-
-During early Eocene time, coal swamps formed in eastern Jackson Hole and
-persisted for thousands of years, as is shown by 60 feet of coal in a
-single bed at one locality. Continuing on into middle Eocene time, the
-climate was subtropical and humid, and the terrain was near sea level.
-Tropical breadfruits, figs, and magnolias flourished along with a more
-temperate flora of redwood, hickory, maple, and oak. Horses the size of
-a dog and many other small mammals were abundant. Primates, thriving in
-an ideal forest habitat, were numerous. Streams contained gar fish and
-crocodiles (fig. 50).
-
-    [Illustration: Figure 51. _A typical Oligocene landscape showing
-    some of the more abundant types of mammals. Mural painting by Jay H.
-    Matterness; photo courtesy of Smithsonian Institution._]
-
-  _Trigonias_                early rhinoceros
-  _Perchoerus_               early peccary
-  _Mesohippus_               3-toed horse
-  _Aepinacodon_              remote relative of hippopotamus
-  _Archaeotherium_           giant piglike mammal
-  _Protoceras_               bizarre horned ruminant
-  _Hesperocyon_              ancestral dog
-  _Hyracodon_                small fleet-footed rhinoceros
-  _Poëbrotherium_            ancestral camel
-  _Hypisodus_                very small chevrotainlike ruminant
-  _Ictops_                   small insect-eating mammal
-  _Brontotherium_            titanothere
-  _Protapirus_               ancestral tapir
-  _Glyptosaurus_             extinct lizard
-  _Hoplophoneus_             saber-toothed cat
-  _Subhyracodon_             early rhinoceros
-  _Merycoidodon_             sheeplike grazing mammal
-  _Hyaenodon_                archaic hyenalike mammal
-  _Hypertragulus_            chevrotainlike ruminant
-
-Early in the Oligocene Epoch, between 30 and 35 million years ago, the
-climate in Jackson Hole became cooler and drier, and the subtropical
-plants gave way to the warm temperate flora of oak, beech, maple, alder,
-and ash. The general land surface rose higher above sea level, perhaps
-by accumulation of several thousand feet of Oligocene volcanic rocks
-(fig. 52) rather than by continental uplift. _Titanotheres_ (large
-four-legged mammals with the general size and shape of a rhinoceros)
-flourished in great numbers for a few million years and then abruptly
-vanished. Horses by now were about the size of a very small modern colt.
-Rabbits, rodents, carnivores, tiny camels, and other mammals were
-abundant in Jackson Hole, and the fauna, surprisingly, was essentially
-the same as that 500 miles to the east, at a much lower elevation, on
-the plains of Nebraska and South Dakota (fig. 51).
-
-The Miocene Epoch (15 to 25 million years ago) was the time of such
-intense volcanic activity in the Teton region that animals must have
-found survival very difficult. A few skeletons and fragmentary parts of
-camels about the size of a small horse and other piglike animals called
-_oreodonts_ comprise our only record of mammals; nothing is known of the
-plants. Farther east the climate fluctuated from subtropical to warm
-temperate, gradually becoming cooler toward the end of the epoch.
-
-Fossils in the Pliocene lake deposits (8 to 10 million years old; see
-description of Teewinot Formation) include shallow-water types of
-snails, clams, diatoms, and ostracodes, as well as beavers, mice,
-suckers, and frogs. Pollen in these beds show that adjacent upland areas
-supported fir, spruce, pine, juniper, sage, and other trees and shrubs
-common to the area today. Therefore, the climate must have been much
-cooler than in Miocene time. No large mammals of Pliocene age have been
-found in Jackson Hole. The record of life during Quaternary time is
-discussed later.
-
-    [Illustration: Figure 52. _Layers of volcanic conglomerate separated
-    by thin white tuff beds in Wiggins Formation. These cliffs, on the
-    north side of Togwotee Pass, are about 1,100 feet high and represent
-    a cross section of part of the enormous blanket of waterlaid debris
-    that spread south and east from the Yellowstone-Absaroka volcanic
-    area. These and younger deposits from the same general source filled
-    the basins and almost completely buried the mountains in this part
-    of Wyoming._]
-
-
-                               Volcanoes
-
-Volcanoes are one of the most interesting parts of the geologic story of
-the Teton region. Although ash from distant volcanoes had settled in
-northwestern Wyoming at least as far back in time as Jurassic, the first
-nearby active volcanoes (since the Precambrian) erupted in the
-Yellowstone-Absaroka region during the early Eocene, about 50 million
-years ago. From then on, the volcanic area grew in size and the violence
-of eruptions and volume of debris increased until Pliocene time. This
-debris had a profound influence on the color and composition of the
-sediments and on the environment and types of plants and animals.
-
-The color of the volcanic rocks and the sediments derived from them
-varies significantly from one epoch to another. For example, the middle
-Eocene rocks are white to light-green, red, and purple, upper Eocene are
-dark-green, Oligocene are light-gray, white, and brown, Miocene are
-dark-green, brown, and gray, and Pliocene are white to red-brown.
-
-    [Illustration: Figure 53. _Air oblique view south, showing the north
-    end of the Teton Range disappearing beneath Pleistocene lava flows.
-    Light-colored bare area at lower left is vertical Paleozoic
-    limestone surrounded on three sides by nearly horizontal rhyolite
-    lava flows. Bare slope at lower right is west-dipping Pinyon
-    Conglomerate, also overlapped by lava. Grand Teton is on right
-    skyline and Mt. Moran is rounded summit on middle skyline._]
-
-As mentioned earlier, it is probable that the vast outpouring of
-volcanic rocks during late Tertiary time in the Teton region and to the
-north and northeast is directly related to the subsidence of Jackson
-Hole and the rise of the Tetons.
-
-The spectacular banded cliffs of the Wiggins Formation on both sides of
-Togwotee Pass (fig. 52) and farther north in the Absaroka Range are
-remnants of Oligocene volcanic conglomerate and tuff that once spread as
-a blanket several thousand feet thick across eastern Jackson Hole and
-partially or completely buried the nearby older folded mountain ranges.
-
-    [Illustration: Figure 54. _Obsidian, a volcanic glass less than 10
-    million years old, especially prized by Indians who used it for
-    spear and arrow points and for tools._]
-
-About 25 million years ago, with the start of the Miocene Epoch,
-volcanic vents opened up within, and along the borders of, Grand Teton
-National Park. Major centers of eruption were at the north end of the
-Teton Range, east of Jackson Lake, and south of Spread Creek. They
-emitted a prodigious amount of volcanic ash and fragments of congealed
-lava. For example, adjacent to one vent a mile in diameter, about 4
-miles north-northeast of Jackson Lake Lodge, is a continuous section,
-7,000 feet thick, of waterlaid strata derived in large part from this
-volcanic source. These sedimentary rocks comprise the Colter Formation
-which is darker colored and contains more iron and magnesium than the
-Wiggins Formation. The site of deposition at this locality was a
-north-trending trough that represented an early stage in the downwarping
-of Jackson Hole.
-
-Pliocene volcanoes erupted in southern and central Yellowstone Park. The
-volcanoes emitted viscous, frothy, pinkish-gray and brown lava called
-_rhyolite_. This is an extrusive igneous rock that has the same
-composition as granite, but is much finer grained. In several places,
-lava apparently flowed into the north end of Teewinot Lake, chilled
-suddenly, and solidified into a black volcanic glass called _obsidian_.
-Because it chips easily into thin flakes having a smooth surface,
-obsidian was prized by the Indians, who used it for spear and arrow
-points (fig. 54). Some of this obsidian has a potassium-argon date of 9
-million years.
-
-    [Illustration: Figure 55. _East face of Signal Mountain showing
-    Bivouac Formation (upper Pliocene or Pleistocene). Tilted ledge is
-    rhyolitic welded tuff 2.5 million years old, and slopes above and
-    below it are conglomerate. National Park Service photo by W. E.
-    Dilley._]
-
-After Teewinot Lake was filled with sediment, the floor of Jackson Hole
-became a flat boulder-covered surface. Nearby vents erupted heavy fiery
-clouds of gaseous molten rock that rolled across this plain and then
-congealed into hard layers with the general appearance of lava flows.
-Under a microscope, however, the rock is seen to be made up of
-compressed fragments of glass that matted down and solidified when the
-clouds stopped moving. This kind of rock is called a _welded tuff_. One
-of these forms the conspicuous ledge in the Bivouac Formation on the
-north and east sides of Signal Mountain (fig. 55), and is especially
-important because it has a potassium-argon date of 2.5 million years.
-More of this _welded tuff_ flowed southward from Yellowstone National
-Park, engulfed the north end of the Teton Range (fig. 53), and continued
-southward along the west side of the mountains for 35 miles and along
-the east side for 25 miles.
-
-    [Illustration: Figure 56. _The final 3 million years on our
-    yardstick of time, enlarged to show approximate dates of major
-    events._]
-
-  THE LAST HUNDREDTHS      ABSOLUTE TIME  IMPORTANT EVENTS
-   OF AN INCH OF THE         (Years ago)
-       YARDSTICK
-           0                           0  Last glaciation followed by
-                                          faulting
-         ¹/₁₀₀₀                    50000  Second glaciation
-         ²/₁₀₀₀                   100000  ?—First glaciation
-         ⁶/₁₀₀₀                   700000  ?—Second Quaternary lake
-         ⁸/₁₀₀₀                1 million  ?—Tilting and faulting of
-                                          southern part of Jackson Hole
-        ¹¹/₁₀₀₀              1.3 million  ?—First Quaternary lake
-        ¹²/₁₀₀₀              1.5 million  } Complex series of volcanic
-                                          eruptions in southern Jackson
-                                          Hole
-        ¹⁵/₁₀₀₀              1.9 million  }
-        ¹⁶/₁₀₀₀                2 million  ?—Development of Hoback
-                                          normal fault
-         ²/₁₀₀               2.5 million  Eruption of welded tuff in
-                                          Bivouac Formation
-        ²⁴/₁₀₀₀                3 million
-
-
-
-
- QUATERNARY—TIME OF ICE, MORE LAKES, AND CONTINUED CRUSTAL DISTURBANCE
-
-
-The Quaternary Period is represented by less than 15-thousandths of the
-last inch on our yardstick of time (fig. 56) and the entire Ice Age
-takes up less than 2-thousandths of an inch (less than the thickness of
-this page). Nevertheless, the spectacular effects of various forces of
-nature on the Teton landscape during this short interval of time are of
-such significance that they warrant a separate discussion. The role of
-glaciers in carving the rugged Teton peaks and shaping the adjacent
-valleys was mentioned in the first part of this booklet, but is
-discussed in more detail here. The magnitude and complexity of crustal
-movements increased during the final 2 million years of time—so much so
-that the beginning of Quaternary time has not yet been identified with
-any single event. Figure 56 shows the major events described below.
-
-
-                          Hoback normal fault
-
-The _Hoback normal fault_, 30 miles long, with a mile or more
-displacement, developed in the southernmost part of Jackson Hole about 2
-million years ago. This fault is on the east side of the valley. Thus,
-the valley block was downdropped between this fault and the Teton fault
-that borders the west side.
-
-
-                           Volcanic activity
-
-During or shortly after major movement on the Hoback fault, and perhaps
-related to it, there was a complex series of volcanic eruptions west and
-north of the town of Jackson, along the south boundary of the park. In
-rapid succession, lavas of many types, with a combined thickness of more
-than 1,000 feet, were extruded and volcanic plugs intruded into the
-near-surface sedimentary rocks. These volcanic rocks can be seen on the
-East and West Gros Ventre Buttes.
-
-There are no active volcanoes in the Teton region today and no
-postglacial lava flows or cinder cones. Five miles north of Grand Teton
-National Park are boiling springs (Flagg Ranch hot springs) that are
-associated with the youngest (late Quaternary) lavas in southern
-Yellowstone Park. Elsewhere in Jackson Hole are a number of lukewarm
-springs but their relation to volcanic rocks has not been determined.
-
-What happened to the vast thicknesses of volcanic debris? We know they
-existed because sections of them have been measured on the eroded edges
-of uptilted folds and fault blocks. Many cubic miles of these rocks are
-now buried beneath the floor of Jackson Hole, but a much greater volume
-was carried completely out of the region by water, ice, and wind during
-the final chapter of geologic history.
-
-
-                            Preglacial lakes
-
-Remnants of two sets of lake deposits in Jackson Hole record preglacial
-events in Quaternary time. Downdropping of southern Jackson Hole along
-the Hoback and Teton faults blocked the southwestward drainage of the
-Snake River, and a new lake formed overlapping and extending south of
-the site of the long-vanished Teewinot Lake. Incorporated in the lake
-sediments are fragments of lava like that in nearby Quaternary flows.
-From this we know that the lake formed after at least some of the lava
-was emplaced. Apparently subsidence was more rapid than filling, for a
-time, at least, because this new lake was deep. Fossil snails preserved
-in olive-drab to gray fine-grained claystone overlying lava flows at the
-north end of East Gros Ventre Butte are the kind now living at depths of
-120 to 300 feet in Lake Tahoe, California-Nevada. Near the margins of
-the lake, pink and green claystone and soft sandstone were deposited.
-The duration of this lake is not known but it lasted long enough for 200
-feet of beds to accumulate. Subsequent faulting and warping destroyed
-the lake, left tilted remnants of the beds perched 1,000 feet up on the
-east side of Jackson Hole, and permitted the Snake River to reestablish
-its course across the mountains to the southwest.
-
-Later downdropping of Jackson Hole impounded a second preglacial lake.
-Little is known about its extent because nearly everywhere the soft
-brown and gray shale, claystone, and sandstone deposited in it were
-scooped out and washed away during subsequent glaciations. A few
-remnants of the lake deposits are preserved in protected places,
-however; two are within the Gros Ventre River Valley—one downstream from
-Lower Slide Lake about a mile east of the park and the other 4 miles
-farther east. The latter remnant is nearly 500 feet thick and the upper
-half is largely very fine grained shale and claystone. This fine texture
-suggests that the lake existed for a good many thousand years, for such
-deposits commonly accumulate more slowly than coarser grained debris.
-
-    [Illustration: Figure 57. _Map showing extent and direction of
-    movement of first and largest ice sheet. See figure 41 for State
-    lines and location map._]
-
-
-                              The Ice Age
-
-With the uplift of the Teton Range and the formation of Jackson Hole
-late in Cenozoic time the landscape gradually began to assume the
-general outlines that we see today. Rain, wind, snow, and frost shaped
-the first crude approximations of the present ridges and peaks. Streams
-cut into the rising Teton fault block, eroding the ancestral canyons
-deeper and deeper as the uplift continued. The most recent great chapter
-in the story of the Teton landscape, however, remained to be written by
-the glaciers of the _Ice Age_.
-
-The reasons for the climatic changes that caused the Ice Age are still a
-matter of much scientific debate. Various theories have been advanced
-that attribute them to changes in solar radiation, changes in the
-earth’s orbit and inclination to the sun, variations in the amount of
-carbon dioxide in the atmosphere, shifts in the positions of the
-continents or the poles, and to many other factors, but none has met
-with universal acceptance. No doubt the explanation lies in some unusual
-combination of circumstances, for widespread glaciation occurred only
-twice before in the earth’s history—once in the late Precambrian and
-once during the Permian. It is quite clear, however, that the glaciers
-did not form in response to any local cause such as the uplift of the
-Teton Range, for concurrent climatic changes and ice advance took place
-throughout many parts of the world.
-
-At least three times in the last 250,000 years glaciers from the
-surrounding highlands invaded Jackson Hole. The oldest and most
-widespread glaciation probably took place about 200,000 years ago; it
-was called the _Buffalo Glaciation_ by Prof. Eliot Blackwelder in 1915
-(see selected references). The age estimate is based on measurements of
-the thickness of the decomposed layer on the surface of obsidian pebbles
-in the glacial debris. Major sources of ice were the Beartooth Mountains
-(fig. 1), the Absaroka Range, and the Wind River Range. The Gros Ventre
-Mountains and Teton Range furnished lesser amounts of ice.
-
-The ice from the Beartooth and Absaroka centers of ice accumulation
-converged in the northeastern part of Grand Teton National Park and
-flowed south along the face of the Teton Range in a giant stream that in
-many places was 2,000 feet thick (fig. 57). All but the highest parts of
-the Pinyon Peak and Mount Leidy Highlands were buried and scoured.
-Signal Mountain, Blacktail Butte, and the Gros Ventres Buttes were
-overridden and shaped by ice at this time. Another glacier, this one
-from the Wind River Range, flowed northwest along the Continental
-Divide, then down the Gros Ventre River Valley, and merged with the
-southward-moving main ice stream west of Lower Slide Lake. Where Jackson
-Hole narrows southward, the glacier became more and more confined, but
-nevertheless flowed all the way through the Snake River Canyon and on
-into Idaho.
-
-    [Illustration: Figure 58. _Glacial deposits, outwash, and loess
-    exposed along Boyle Ditch in Jackson Hole National Elk Refuge.
-    Indicated are middle Pliocene Teewinot formation (A), oldest till
-    (B), Bull Lake outwash gravel (C), and post-Bull Lake loess (D),
-    which here contains snail shells dated by Carbon-14 as 15,000 years
-    old. Height of cliff is about 30 feet._]
-
-The volume of this great ice mass was probably considerably more than
-1,000 cubic miles. When it melted, nearly all the previously accumulated
-soil in Jackson Hole was washed away and a pavement of quartzite
-boulders mantled much of the glaciated surface. In areas not
-subsequently glaciated, the lack of soil and abundance of quartzite
-boulders drastically influenced the topography, later drainage,
-distribution of all types of vegetation, especially conifers and grass,
-and the pattern of human settlement and industry.
-
-    [Illustration: Figure 59. _View west from the Snake River overlook
-    showing at upper right the Burned Ridge moraine (with trees) merging
-    southward with the highest (oldest) Pinedale outwash plain. The next
-    lower surface is composed of outwash from the Jackson Lake moraine
-    which lies to the right, out of the picture. At the bottom is
-    Deadman’s Bar, a gravel deposit at the present river level. Photo by
-    H. D. Pownall._]
-
-The second glaciation, named _Bull Lake_, was less than half as
-extensive as the first. A large tongue of ice from the Absaroka center
-of accumulation flowed down the Buffalo River Valley and joined ice from
-the Tetons on the floor of Jackson Hole. An enormous outwash fan of
-quartzite boulders extended from near Blacktail Butte southward
-throughout most of southern Jackson Hole. Glaciers in the Gros Ventre
-Mountains did not advance beyond the east margin of the valley floor.
-Carbon-14 ages and data from weathered obsidian pebbles suggest that
-this glaciation took place between 35,000 and 80,000 years ago.
-
-Bull Lake moraines and outwash deposits are overlain directly in the
-southern part of Jackson Hole by fine silt, rather than by deposits of
-the third glaciation (fig. 58). This silt, of windblown origin, is
-called _loess_ and contains fossil shells dated by Carbon-14 as between
-13,000 and 19,000 years old. Wherever the loess occurs, it is marked by
-abundant modern coyote dens and badger burrows.
-
-    [Illustration: Figure 60. _Air oblique view west toward the Teton
-    Range, showing effects of Pinedale Glaciation on the landscape. Mt.
-    Moran is at top left; the mountain front is broken by U-shaped
-    valleys from which ice emerged into the area now occupied by Jackson
-    Lake. The timbered area bordering Jackson Lake is the Jackson Lake
-    moraine. One of the braided outlet channels breaching the Jackson
-    Lake moraine can be seen crossing the outwash plain at the left
-    center. Lakes at lower right occupy “potholes” near where the
-    9,000-year-old snail shells occur. Snake River is in foreground.
-    Photo by R. L. Casebeer._]
-
-The third and last glaciation, named the _Pinedale_, was even less
-extensive than the others. Nevertheless it was of great importance for
-it added the final touches to the present landscape. The jagged
-intricately ice-carved peaks (fig. 4) and the glittering lakes and broad
-gravelly plains are vivid reminders of this recent chapter in geologic
-history.
-
-Pinedale glaciers advanced down Cascade, Garnet, Avalanche, and Death
-Canyons and spilled out onto the floor of Jackson Hole, where they built
-the outermost loops of the conspicuous terminal moraines that now
-encircle Jenny, Bradley, Taggart, and Phelps Lakes (fig. 13). Ice
-streams from Glacier Gulch and Open Canyon also left prominent moraines
-on the valley floor, but these do not contain lakes. Ice from Leigh
-Canyon and all of the eastward-draining valleys to the north combined to
-form a large glacier in roughly the present position of Jackson Lake.
-This ice entirely surrounded Signal Mountain, leaving only the upper few
-hundred feet projecting as an island or _nunatak_.
-
-    [Illustration: Figure 61. _The Pinedale Glaciers in the central part
-    of Jackson Hole as they might have appeared at the time the Jackson
-    Lake moraine was built. Solid color areas are lakes; dark irregular
-    pattern shows areas of moraine deposited during the maximum advance
-    of the Pinedale Glaciers. Pattern of open circles shows older
-    Pinedale outwash plains; pattern of fine dots shows outwash plains
-    built at the time the glaciers were in the positions shown in the
-    drawing. Coarser dots near the margins of the glaciers represent
-    concentrations of rock debris in the ice._]
-
-The southernmost major advance of Pinedale ice from Jackson Lake is
-marked by a series of densely timbered moraines that cross the Snake
-River Valley. This series is collectively named the _Burned Ridge
-moraine_ (fig. 61). Extending southward for 10 miles from this moraine
-is a remarkably flat surfaced gravelly outwash deposit. It was spread by
-streams that poured from the glacier at the time the moraine was being
-built (fig. 59). East of the Snake River, the main highway from a point
-just north of Blacktail Butte to the Snake River overlook is built on
-this flat untimbered surface. We assume that the outwash is younger than
-15,000 years because it apparently overlies loess of that age.
-
-The glacier withdrew rapidly northward from the Burned Ridge moraine,
-leaving behind many large irregular masses of stagnant, debris-covered
-ice. The sites of these became kettles, locally known as “The Potholes”
-(fig. 12). The main glacier retreated to a position marked by the loop
-of moraines just south of Jackson Lake (fig. 60). Figure 61 is a sketch
-map showing how the glaciers in this part of Jackson Hole might have
-appeared at the time the Jackson Lake moraine was built.
-
-Abundant snail shells have been found in lake sediments in the bottoms
-of the kettles north of the Burned Ridge moraine (fig. 60) as well as on
-low ridges between them. Carbon-14 age determinations indicate that the
-snails lived about 9,000 years ago, either in a lake already present
-before the Pinedale ice advanced and formed the Burned Ridge moraine or
-in ponds that filled kettles left as the ice melted behind this moraine.
-
-In either case, the shells indicate that the Pinedale glaciers probably
-existed on the floor of Jackson Hole as recently as 9,000 years ago, at
-a time when Indians were already living in the area. We can easily
-imagine the fascination with which these primitive peoples may have
-watched as year after year the glaciers wasted away, slowly retreating
-back into the canyons, then withdrawing into the sheltered recesses of
-the high mountains, eventually to dwindle and disappear.
-
-Many bits of evidence, both from North America and Europe, indicate that
-there was a period called the _climatic optimum_ about 6,000 years ago
-when the climate was significantly warmer and drier than at present. We
-suspect, though there is as yet no direct proof, that the Pinedale
-glaciers wasted away entirely during this interval.
-
-The modern pattern of vegetation in Jackson Hole is strongly influenced
-by the distribution of Pinedale glacial moraines and outwash deposits.
-Almost without exception the moraines are heavily forested, whereas the
-nearby outwash deposits are covered only by a sparse growth of
-sagebrush. This is probably because the moraines contain large amounts
-of clay and silt produced by the grinding action of the glaciers.
-Material of this type retains water much better and, because of the
-greater variety of chemical elements, is more fertile than the porous
-quartzite gravel and sand on the outwash plains.
-
-
-                            Modern glaciers
-
-About a dozen small rapidly dwindling glaciers exist today in shaded
-reentrants high in the Teton Range. They are probably vestiges of ice
-masses built up since the climatic optimum, during the so-called
-“_Little Ice Age_.” These glaciers, while insignificant compared to
-those still present in many other mountain ranges, are fascinating
-working models of the great ice streams that shaped the Tetons during
-Pleistocene time.
-
-The Teton Glacier (fig. 6) is one of the best known. It is an ice body
-about 3,500 feet long and 1,100 feet wide that lies at the head of
-Glacier Gulch, shaded by the encircling ridges of the Grand Teton, Mount
-Owen, and Mount Teewinot. Ice in the central part is moving at a rate of
-more than 30 feet a year.
-
-
-
-
-                       THE PRESENT AND THE FUTURE
-
-
-The geologic story of the Teton country from the time the earth was new
-to the present day has been summarized. What can we learn from it? We
-become aware that events recorded in the rocks are not a chaotic jumble
-of random accidents but came in an orderly, logical succession. We see
-the majestic parade of life evolving from simple to complex types,
-overcoming all natural disasters, and adapting to ever-changing
-environments. We can only speculate as to the motivating force that
-launched this fascinating geologic and biologic venture and what the
-ultimate goal may be. New facts and new ideas are added to the story
-each year, but many unknown chapters remain to be studied; these offer
-an irresistible, continuing challenge to inquisitive minds, strong
-bodies, and restless, adventurous spirits.
-
-Most geologic processes that developed the Teton landscape have been
-beneficial to man; a few have interfered with his activities, cost him
-money, time, effort, and on occasion, his life. Postglacial faulting and
-tilting along the southern margin of Grand Teton National Park diverted
-drainage systems (such as Flat Creek, southwest of the Flat Creek fault
-on the south edge of the geologic map), raised hills, dropped valleys,
-and made steep slopes unstable. Flood-control engineers wage a
-never-ending struggle to keep the Snake River from shifting to the west
-side of Jackson Hole as the valley tilts westward in response to
-movement along the Teton fault. Each highway into Jackson Hole has been
-blocked by a landslide at one time or another and maintenance of roads
-across slide areas requires much ingenuity. We see one slide (the Gros
-Ventre) that blocked a river; larger slides have occurred in the past,
-and more can be expected. Abundant fresh fault scarps are a constant
-reminder that public buildings, campgrounds, dams, and roads need to be
-designed to withstand the effects of earthquakes. Some of these problems
-have geologic solutions; others can be avoided or minimized as further
-study increases our understanding of this region.
-
-Man appeared during the last one-fiftieth of an inch on our yardstick of
-time gone by. In this short span he has had more impact on the earth and
-its inhabitants than any other form of life. Will he use wisely the
-lessons of the past as a guide while he writes his record on the
-yardstick of the future?
-
-
-
-
-                                APPENDIX
-
-
-                            Acknowledgements
-
-This booklet could not have been prepared without the cooperation and
-assistance of many individuals and organizations. We are indebted to the
-National Park Service for the use of facilities, equipment, and
-photographs, and for the enthusiasm and interest of all of the park
-staff. We especially appreciate the cooperation, advice, and assistance
-rendered by the late Fred C. Fagergren, former superintendent of Grand
-Teton National Park; Willard E. Dilley, former chief park naturalist;
-and R. Alan Mebane, former assistant chief park naturalist.
-
-Profs. Charles C. Bradley and John Montagne of Montana State University
-and Bruno J. Giletti of Brown University generously provided us with
-unpublished data. Cooperators during the years of background research
-were the late Dr. H. D. Thomas, State Geologist of Wyoming, and Dr. D.
-L. Blackstone, Jr., Chairman, Department of Geology, University of
-Wyoming.
-
-Helpful suggestions were made by many of our colleagues with the U. S.
-Geological Survey; S. S. Oriel, in particular, gave unstintingly of his
-time and talents in the review and revision of an early version of the
-manuscript. A later version had the further benefit of critical review
-by three other people, all experienced in presenting various types of
-scientific data to public groups: John M. Good, former chief park
-naturalist of Yellowstone National Park; Bryan Harry, former assistant
-chief park naturalist of Grand Teton National Park; and Richard Klinck,
-“1965 National Teacher of the Year.”
-
-We are indebted to Ann C. Christiansen, Geologic Map Editor, for advice
-and guidance on the illustrations and to R. C. Fuhrmann and his staff
-for preparation of many of the line drawings. Block diagrams and photo
-artwork were prepared by J. R. Stacy and R. A. Reilly. All photographs
-without specific credit lines are by the authors. From the beginning of
-the Teton field study to editing and proofing of the final manuscript,
-our wives, Jane M. Love and Linda H. Reed, have been enthusiastic and
-indispensable participants.
-
-
-            Selected references—if you wish to read further
-
-
-  Blackwelder, Eliot, 1915, Post-Cretaceous history of the mountains of
-          central western Wyoming: Jour. Geology, v. 23, p. 97-117,
-          193-217, 307-340.
-  Bradley, F. H., 1873, Report on the geology of the Snake River
-          district: U.S. Geol. Survey Terr. 6th Ann. Rept. (Hayden), p.
-          190-271.
-  Edmund, R. W., 1951, Structural geology and physiography of the
-          northern end of the Teton Range, Wyoming: Augustana Library
-          Pub. 23, 82 p.
-  Fryxell, F. M., 1930, Glacial features of Jackson Hole, Wyoming:
-          Augustana Library Pub. 13, 129 p.
-  ——, 1938, The Tetons, interpretations of a mountain landscape: Univ.
-          California Press, Berkeley, Calif., 77 p.
-  Hague, Arnold, 1904, Atlas to accompany U.S. Geol. Survey Monograph 32
-          on the geology of Yellowstone National Park.
-  ——, Iddings, J. P., Weed, W. H., and others, 1899, Geology of the
-          Yellowstone National Park: U.S. Geol. Survey Monograph 32, Pt.
-          2, 893 p.
-  Harry, Bryan, 1963, Teton trails, a guide to the trails of Grand Teton
-          National Park: Grand Teton Natural History Association, Moose,
-          Wyo., 56 p.
-  Horberg, Leland, 1938, The structural geology and physiography of the
-          Teton Pass area, Wyoming: Augustana Library Pub. 16, 86 p.
-  Hurley, P. M., 1959, How old is the earth?: Anchor Books, Garden City,
-          N. Y., 160 p.
-  Ortenburger, Leigh, 1965, A climber’s guide to the Teton Range: Sierra
-          Club, San Francisco, 336 p.
-  St. John, O. H., 1883, Report on the geology of the Wind River
-          district: U.S. Geol. Geog. Survey Terr. 12th Ann. Rept.
-          (Hayden), Pt. 1, p. 173-270.
-  Wyoming Geological Association, 1956, Guidebook, 11th annual field
-          conf., Jackson Hole, Wyoming, 1956, Casper, Wyo., 256 p.,
-          incl. sketch maps, diagrams, tables, and illus., also geol.
-          map, sections, and charts. Composed of a series of individual
-          papers by various authors.
-
-
-                           About the authors
-
-J. D. Love, a native of Wyoming, received his bachelor and master of
-arts degrees from the University of Wyoming and his doctor of philosophy
-degree from Yale University. His first field season in the Teton
-country, in 1933, was financed by the Geological Survey of Wyoming.
-After 12 years of geologic work ranging from New England to Utah and
-Michigan to Mississippi, he returned to the Teton region. Beginning in
-1945, he spent parts or all of 20 field seasons in and near the Tetons.
-He compiled the first geologic map of Teton County. He is the senior
-author of the geologic map of Wyoming, and author or co-author of more
-than 70 other published maps and papers on the geology of Wyoming. In
-1961, the University of Wyoming awarded him an honorary doctor of laws
-degree for his work on uranium deposits that “led to the development of
-the uranium industry in Wyoming.” The Wyoming Geological Association
-made him an honorary life member and gave him a special award for his
-geologic studies of the Teton area. He is a Fellow of the Geological
-Society of America and is active in various other geological
-organizations, as well as having been president of the Wyoming Chapters
-of Sigma Xi (scientific honorary) and Phi Beta Kappa (scholastic
-honorary) societies.
-
-John C. Reed, Jr., joined the U.S. Geological Survey in 1953 after
-receiving his doctor of philosophy degree from the John Hopkins
-University. His principal geologic work before coming to the Teton
-region was in Alaska and in the southern Appalachians. Beginning in
-1961, he spent five field seasons studying and mapping the Precambrian
-rocks in Grand Teton National Park, including all the high peaks in the
-Teton Range. He is a noted mountaineer, a Fellow of the Geological
-Society of America, a member of the Arctic Institute of North America,
-and the American Alpine Club. His numerous publications, in addition to
-those on the Tetons, describe the geology of mountainous areas in
-Alaska, the Appalachians, and Utah.
-
-
-
-
-                  Index of selected terms and features
-
-
-  _Term_                              _Defined or described on page_
-
-
-                                    A
-  amphibolite                                                     51
-  anticlines                                                      85
-
-
-                                    B
-  badlands                                                        14
-  bentonite                                                       81
-  biotite                                                         51
-  brachiopods                                                     70
-  Buffalo Glaciation                                             106
-  Bull Lake Glaciation                                           108
-  Burned Ridge moraine                                           111
-  buttes                                                          18
-
-
-                                    C
-  Carbon-14                                                       48
-  carnivores                                                      95
-  chlorite                                                        56
-  cirque                                                          30
-  climatic optimum                                               112
-  Cordilleran trough                                              69
-
-
-                                    D
-  diabase                                                         59
-  dikes                                                           56
-  dipping                                                         39
-  dolomite                                                        75
-
-
-                                    E
-  “edgewise” conglomerate                                         73
-  epochs                                                          46
-  eras                                                            46
-  erosion                                                         27
-  erratics                                                        31
-  extrusive igneous rocks                                         46
-
-
-                                    F
-  fault                                                            9
-  fault block mountain range                                      37
-  fault scarps                                                    37
-  formations                                                      66
-  frost wedging                                                   25
-
-
-                                    G
-  geologic                                                        10
-  glacial striae                                                  30
-  gradients                                                       28
-  Grand Valley Lake                                               95
-  granite                                                         55
-  granite gneiss                                                  54
-  groups                                                          47
-  gypsum                                                          79
-
-
-                                    H
-  herbivores                                                      95
-  Hoback normal fault                                            103
-  hole                                                             8
-  hornblende                                                      51
-
-
-                                    I
-  Ice Age                                                        105
-  igneous rocks                                                   46
-  intrusive igneous rocks                                         46
-
-
-                                    J
-  Jackson Hole                                                     8
-  jade                                                            55
-
-
-                                    K
-  kettle                                                          31
-
-
-                                    L
-  Laramide Revolution                                             82
-  lateral moraine                                                 30
-  layered gneisses                                                51
-  Little Ice Age                                                 112
-  loess                                                          108
-
-
-                                    M
-  magma                                                           60
-  magnetite                                                       52
-  marine sedimentary rocks                                        21
-  metamorphic rocks                                               53
-  muscovite                                                       55
-
-
-                                    N
-  normal fault                                                    39
-  nunatak                                                        111
-
-
-                                    O
-  obsidian                                                       101
-  oreodonts                                                       97
-  outwash                                                         31
-  outwash plain                                                   31
-  outwash terraces                                                34
-
-
-                                    P
-  pegmatite                                                       56
-  period                                                          46
-  Pinedale Glaciation                                            109
-
-
-                                    Q
-  quartzite                                                       63
-
-
-                                    R
-  reverse fault                                                   39
-  rhyolite                                                       100
-  rock glaciers                                                   26
-
-
-                                    S
-  schist                                                          51
-  sedimentary rocks                                               45
-  series                                                          47
-  serpentine                                                      55
-  “soapstone”                                                     55
-  Sundance Sea                                                    79
-  systems                                                         46
-
-
-                                    T
-  talus                                                           24
-  Targhee uplift                                                  83
-  Teewinot Lake                                                   92
-  terminal moraine                                                30
-  Tetons                                                           8
-  Teton fault                                                     37
-  thrust fault                                                    39
-  timberline                                                      15
-  titanothere                                                     97
-  treeline                                                        15
-  Triceratops                                                     85
-  trilobites                                                      70
-  tuff                                                            92
-
-
-                                    W
-  welded tuff                                                    101
-
-
-
-
-              The GRAND TETON NATURAL HISTORY ASSOCIATION
-
-
-The Grand Teton Natural History Association assists the National Park
-Service in the development of a broad public understanding of the
-geology, plant and animal life, history, and related subjects pertaining
-to Grand Teton National Park. It aids in the development of museums and
-wayside exhibits, offers for sale publications on natural and human
-history, and cooperates with the Government in the interest of Grand
-Teton National Park.
-
-_Mail orders_: For a publication list, write the Grand Teton Natural
-History Association, Moose, Wyoming 83012.
-
-                      _Creative Director_:  Century III Advertising. Inc.
-                               _Designer_:  Les Hays Studios, Inc.
-  _Color Separations_—_Assembly_—_Plates_:  Orent Graphic Arts, Inc.
-                                   _Type_:  Bodoni and Gothic
-                                _Printer_:  Omaha Printing Co.
-                               _Printing_:  Offset Lithography.
-                                            Six Colors on Covers
-                                            Two Colors on Body
-
-    [Illustration: GEOLOGIC MAP OF GRAND TETON NATIONAL PARK]
-
-    [Illustration: EXPLANATION]
-
-
-  CENOZOIC
-    QUATERNARY
-      Sand, gravel, and talus
-        _Includes glacial outwash and materials deposited by present
-              streams_
-      Landslide deposits
-      Moraine deposits of Pinedale glaciers
-      Moraine deposits of Bull Lake and older glaciers
-    TERTIARY
-      Volcanic rocks
-        _Lava flows and volcanic ash_
-      Conglomerate, sandstone, shale, claystone, marl, and pumice
-        _Deposited on land or in shallow lakes_
-  MESOZOIC
-    Conglomerate, sandstone, shale, and coal
-      _Deposited on land_
-    Shale, sandstone, and limestone
-      _Mostly deposited in shallow seas_
-  PALEOZOIC
-    Limestone, shale, and sandstone
-      _Deposited in shallow seas_
-  PRECAMBRIAN
-    Diabase dikes
-    Granite, gneiss, and schist
-  Fault
-    _Dashed where approximately located; dotted where concealed beneath
-          unfaulted younger deposits. U is on the side that moved up; D,
-          on the side that moved down_
-  Geologic contact
-
-
-    [Illustration: View southwest from Lake Solitude toward the Grand
-    Teton (right), Mt. Owen, and Mt. Teewinot. _Wyoming Travel
-    Commission photo by J. R. Simon._]
-
-    [Illustration: Grand Teton, Mt. Owen, and Mt. Teewinot from Jenny
-    Lake Flat. _National Park Service photo by W. E. Dilley._]
-
-
-
-
-                          Transcriber’s Notes
-
-
-—Retained publication information from the printed edition: this eBook
-  is public-domain in the country of publication.
-
-—Corrected a few palpable typos.
-
-—Re-arranged text in captions closer to the corresponding image.
-
-—Expanded ambiguous references to illustrations, _e.g._ “Figure D” to
-   “Figure 16D”
-
-—Added one section heading, “The First Big Lake” to match the table of
-  contents.
-
-—Included a transcription of the text within some images, with estimated
-  scale readings from charts.
-
-—In the text versions only, text in italics is delimited by
-  _underscores_.
-
-
-
-
-
-
-
-End of the Project Gutenberg EBook of Creation of the Teton Landscape, by 
-J. D. Love and John C. Reed
-
-*** END OF THIS PROJECT GUTENBERG EBOOK CREATION OF THE TETON LANDSCAPE ***
-
-***** This file should be named 52838-0.txt or 52838-0.zip *****
-This and all associated files of various formats will be found in:
-        http://www.gutenberg.org/5/2/8/3/52838/
-
-Produced by Stephen Hutcheson, Dave Morgan and the Online
-Distributed Proofreading Team at http://www.pgdp.net
-
-Updated editions will replace the previous one--the old editions will
-be renamed.
-
-Creating the works from print editions not protected by U.S. copyright
-law means that no one owns a United States copyright in these works,
-so the Foundation (and you!) can copy and distribute it in the United
-States without permission and without paying copyright
-royalties. Special rules, set forth in the General Terms of Use part
-of this license, apply to copying and distributing Project
-Gutenberg-tm electronic works to protect the PROJECT GUTENBERG-tm
-concept and trademark. Project Gutenberg is a registered trademark,
-and may not be used if you charge for the eBooks, unless you receive
-specific permission. If you do not charge anything for copies of this
-eBook, complying with the rules is very easy. You may use this eBook
-for nearly any purpose such as creation of derivative works, reports,
-performances and research. They may be modified and printed and given
-away--you may do practically ANYTHING in the United States with eBooks
-not protected by U.S. copyright law. Redistribution is subject to the
-trademark license, especially commercial redistribution.
-
-START: FULL LICENSE
-
-THE FULL PROJECT GUTENBERG LICENSE
-PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK
-
-To protect the Project Gutenberg-tm mission of promoting the free
-distribution of electronic works, by using or distributing this work
-(or any other work associated in any way with the phrase "Project
-Gutenberg"), you agree to comply with all the terms of the Full
-Project Gutenberg-tm License available with this file or online at
-www.gutenberg.org/license.
-
-Section 1. General Terms of Use and Redistributing Project
-Gutenberg-tm electronic works
-
-1.A. By reading or using any part of this Project Gutenberg-tm
-electronic work, you indicate that you have read, understand, agree to
-and accept all the terms of this license and intellectual property
-(trademark/copyright) agreement. If you do not agree to abide by all
-the terms of this agreement, you must cease using and return or
-destroy all copies of Project Gutenberg-tm electronic works in your
-possession. If you paid a fee for obtaining a copy of or access to a
-Project Gutenberg-tm electronic work and you do not agree to be bound
-by the terms of this agreement, you may obtain a refund from the
-person or entity to whom you paid the fee as set forth in paragraph
-1.E.8.
-
-1.B. "Project Gutenberg" is a registered trademark. It may only be
-used on or associated in any way with an electronic work by people who
-agree to be bound by the terms of this agreement. There are a few
-things that you can do with most Project Gutenberg-tm electronic works
-even without complying with the full terms of this agreement. See
-paragraph 1.C below. There are a lot of things you can do with Project
-Gutenberg-tm electronic works if you follow the terms of this
-agreement and help preserve free future access to Project Gutenberg-tm
-electronic works. See paragraph 1.E below.
-
-1.C. The Project Gutenberg Literary Archive Foundation ("the
-Foundation" or PGLAF), owns a compilation copyright in the collection
-of Project Gutenberg-tm electronic works. Nearly all the individual
-works in the collection are in the public domain in the United
-States. If an individual work is unprotected by copyright law in the
-United States and you are located in the United States, we do not
-claim a right to prevent you from copying, distributing, performing,
-displaying or creating derivative works based on the work as long as
-all references to Project Gutenberg are removed. Of course, we hope
-that you will support the Project Gutenberg-tm mission of promoting
-free access to electronic works by freely sharing Project Gutenberg-tm
-works in compliance with the terms of this agreement for keeping the
-Project Gutenberg-tm name associated with the work. You can easily
-comply with the terms of this agreement by keeping this work in the
-same format with its attached full Project Gutenberg-tm License when
-you share it without charge with others.
-
-1.D. The copyright laws of the place where you are located also govern
-what you can do with this work. Copyright laws in most countries are
-in a constant state of change. If you are outside the United States,
-check the laws of your country in addition to the terms of this
-agreement before downloading, copying, displaying, performing,
-distributing or creating derivative works based on this work or any
-other Project Gutenberg-tm work. The Foundation makes no
-representations concerning the copyright status of any work in any
-country outside the United States.
-
-1.E. Unless you have removed all references to Project Gutenberg:
-
-1.E.1. The following sentence, with active links to, or other
-immediate access to, the full Project Gutenberg-tm License must appear
-prominently whenever any copy of a Project Gutenberg-tm work (any work
-on which the phrase "Project Gutenberg" appears, or with which the
-phrase "Project Gutenberg" is associated) is accessed, displayed,
-performed, viewed, copied or distributed:
-
-  This eBook is for the use of anyone anywhere in the United States and
-  most other parts of the world at no cost and with almost no
-  restrictions whatsoever. You may copy it, give it away or re-use it
-  under the terms of the Project Gutenberg License included with this
-  eBook or online at www.gutenberg.org. If you are not located in the
-  United States, you'll have to check the laws of the country where you
-  are located before using this ebook.
-
-1.E.2. If an individual Project Gutenberg-tm electronic work is
-derived from texts not protected by U.S. copyright law (does not
-contain a notice indicating that it is posted with permission of the
-copyright holder), the work can be copied and distributed to anyone in
-the United States without paying any fees or charges. If you are
-redistributing or providing access to a work with the phrase "Project
-Gutenberg" associated with or appearing on the work, you must comply
-either with the requirements of paragraphs 1.E.1 through 1.E.7 or
-obtain permission for the use of the work and the Project Gutenberg-tm
-trademark as set forth in paragraphs 1.E.8 or 1.E.9.
-
-1.E.3. If an individual Project Gutenberg-tm electronic work is posted
-with the permission of the copyright holder, your use and distribution
-must comply with both paragraphs 1.E.1 through 1.E.7 and any
-additional terms imposed by the copyright holder. Additional terms
-will be linked to the Project Gutenberg-tm License for all works
-posted with the permission of the copyright holder found at the
-beginning of this work.
-
-1.E.4. Do not unlink or detach or remove the full Project Gutenberg-tm
-License terms from this work, or any files containing a part of this
-work or any other work associated with Project Gutenberg-tm.
-
-1.E.5. Do not copy, display, perform, distribute or redistribute this
-electronic work, or any part of this electronic work, without
-prominently displaying the sentence set forth in paragraph 1.E.1 with
-active links or immediate access to the full terms of the Project
-Gutenberg-tm License.
-
-1.E.6. You may convert to and distribute this work in any binary,
-compressed, marked up, nonproprietary or proprietary form, including
-any word processing or hypertext form. However, if you provide access
-to or distribute copies of a Project Gutenberg-tm work in a format
-other than "Plain Vanilla ASCII" or other format used in the official
-version posted on the official Project Gutenberg-tm web site
-(www.gutenberg.org), you must, at no additional cost, fee or expense
-to the user, provide a copy, a means of exporting a copy, or a means
-of obtaining a copy upon request, of the work in its original "Plain
-Vanilla ASCII" or other form. Any alternate format must include the
-full Project Gutenberg-tm License as specified in paragraph 1.E.1.
-
-1.E.7. Do not charge a fee for access to, viewing, displaying,
-performing, copying or distributing any Project Gutenberg-tm works
-unless you comply with paragraph 1.E.8 or 1.E.9.
-
-1.E.8. You may charge a reasonable fee for copies of or providing
-access to or distributing Project Gutenberg-tm electronic works
-provided that
-
-* You pay a royalty fee of 20% of the gross profits you derive from
-  the use of Project Gutenberg-tm works calculated using the method
-  you already use to calculate your applicable taxes. The fee is owed
-  to the owner of the Project Gutenberg-tm trademark, but he has
-  agreed to donate royalties under this paragraph to the Project
-  Gutenberg Literary Archive Foundation. Royalty payments must be paid
-  within 60 days following each date on which you prepare (or are
-  legally required to prepare) your periodic tax returns. Royalty
-  payments should be clearly marked as such and sent to the Project
-  Gutenberg Literary Archive Foundation at the address specified in
-  Section 4, "Information about donations to the Project Gutenberg
-  Literary Archive Foundation."
-
-* You provide a full refund of any money paid by a user who notifies
-  you in writing (or by e-mail) within 30 days of receipt that s/he
-  does not agree to the terms of the full Project Gutenberg-tm
-  License. You must require such a user to return or destroy all
-  copies of the works possessed in a physical medium and discontinue
-  all use of and all access to other copies of Project Gutenberg-tm
-  works.
-
-* You provide, in accordance with paragraph 1.F.3, a full refund of
-  any money paid for a work or a replacement copy, if a defect in the
-  electronic work is discovered and reported to you within 90 days of
-  receipt of the work.
-
-* You comply with all other terms of this agreement for free
-  distribution of Project Gutenberg-tm works.
-
-1.E.9. If you wish to charge a fee or distribute a Project
-Gutenberg-tm electronic work or group of works on different terms than
-are set forth in this agreement, you must obtain permission in writing
-from both the Project Gutenberg Literary Archive Foundation and The
-Project Gutenberg Trademark LLC, the owner of the Project Gutenberg-tm
-trademark. Contact the Foundation as set forth in Section 3 below.
-
-1.F.
-
-1.F.1. Project Gutenberg volunteers and employees expend considerable
-effort to identify, do copyright research on, transcribe and proofread
-works not protected by U.S. copyright law in creating the Project
-Gutenberg-tm collection. Despite these efforts, Project Gutenberg-tm
-electronic works, and the medium on which they may be stored, may
-contain "Defects," such as, but not limited to, incomplete, inaccurate
-or corrupt data, transcription errors, a copyright or other
-intellectual property infringement, a defective or damaged disk or
-other medium, a computer virus, or computer codes that damage or
-cannot be read by your equipment.
-
-1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES - Except for the "Right
-of Replacement or Refund" described in paragraph 1.F.3, the Project
-Gutenberg Literary Archive Foundation, the owner of the Project
-Gutenberg-tm trademark, and any other party distributing a Project
-Gutenberg-tm electronic work under this agreement, disclaim all
-liability to you for damages, costs and expenses, including legal
-fees. YOU AGREE THAT YOU HAVE NO REMEDIES FOR NEGLIGENCE, STRICT
-LIABILITY, BREACH OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE
-PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE FOUNDATION, THE
-TRADEMARK OWNER, AND ANY DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE
-LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT, CONSEQUENTIAL, PUNITIVE OR
-INCIDENTAL DAMAGES EVEN IF YOU GIVE NOTICE OF THE POSSIBILITY OF SUCH
-DAMAGE.
-
-1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you discover a
-defect in this electronic work within 90 days of receiving it, you can
-receive a refund of the money (if any) you paid for it by sending a
-written explanation to the person you received the work from. If you
-received the work on a physical medium, you must return the medium
-with your written explanation. The person or entity that provided you
-with the defective work may elect to provide a replacement copy in
-lieu of a refund. If you received the work electronically, the person
-or entity providing it to you may choose to give you a second
-opportunity to receive the work electronically in lieu of a refund. If
-the second copy is also defective, you may demand a refund in writing
-without further opportunities to fix the problem.
-
-1.F.4. Except for the limited right of replacement or refund set forth
-in paragraph 1.F.3, this work is provided to you 'AS-IS', WITH NO
-OTHER WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED, INCLUDING BUT NOT
-LIMITED TO WARRANTIES OF MERCHANTABILITY OR FITNESS FOR ANY PURPOSE.
-
-1.F.5. Some states do not allow disclaimers of certain implied
-warranties or the exclusion or limitation of certain types of
-damages. If any disclaimer or limitation set forth in this agreement
-violates the law of the state applicable to this agreement, the
-agreement shall be interpreted to make the maximum disclaimer or
-limitation permitted by the applicable state law. The invalidity or
-unenforceability of any provision of this agreement shall not void the
-remaining provisions.
-
-1.F.6. INDEMNITY - You agree to indemnify and hold the Foundation, the
-trademark owner, any agent or employee of the Foundation, anyone
-providing copies of Project Gutenberg-tm electronic works in
-accordance with this agreement, and any volunteers associated with the
-production, promotion and distribution of Project Gutenberg-tm
-electronic works, harmless from all liability, costs and expenses,
-including legal fees, that arise directly or indirectly from any of
-the following which you do or cause to occur: (a) distribution of this
-or any Project Gutenberg-tm work, (b) alteration, modification, or
-additions or deletions to any Project Gutenberg-tm work, and (c) any
-Defect you cause.
-
-Section 2. Information about the Mission of Project Gutenberg-tm
-
-Project Gutenberg-tm is synonymous with the free distribution of
-electronic works in formats readable by the widest variety of
-computers including obsolete, old, middle-aged and new computers. It
-exists because of the efforts of hundreds of volunteers and donations
-from people in all walks of life.
-
-Volunteers and financial support to provide volunteers with the
-assistance they need are critical to reaching Project Gutenberg-tm's
-goals and ensuring that the Project Gutenberg-tm collection will
-remain freely available for generations to come. In 2001, the Project
-Gutenberg Literary Archive Foundation was created to provide a secure
-and permanent future for Project Gutenberg-tm and future
-generations. To learn more about the Project Gutenberg Literary
-Archive Foundation and how your efforts and donations can help, see
-Sections 3 and 4 and the Foundation information page at
-www.gutenberg.org
-
-
-
-Section 3. Information about the Project Gutenberg Literary Archive Foundation
-
-The Project Gutenberg Literary Archive Foundation is a non profit
-501(c)(3) educational corporation organized under the laws of the
-state of Mississippi and granted tax exempt status by the Internal
-Revenue Service. The Foundation's EIN or federal tax identification
-number is 64-6221541. Contributions to the Project Gutenberg Literary
-Archive Foundation are tax deductible to the full extent permitted by
-U.S. federal laws and your state's laws.
-
-The Foundation's principal office is in Fairbanks, Alaska, with the
-mailing address: PO Box 750175, Fairbanks, AK 99775, but its
-volunteers and employees are scattered throughout numerous
-locations. Its business office is located at 809 North 1500 West, Salt
-Lake City, UT 84116, (801) 596-1887. Email contact links and up to
-date contact information can be found at the Foundation's web site and
-official page at www.gutenberg.org/contact
-
-For additional contact information:
-
-    Dr. Gregory B. Newby
-    Chief Executive and Director
-    gbnewby@pglaf.org
-
-Section 4. Information about Donations to the Project Gutenberg
-Literary Archive Foundation
-
-Project Gutenberg-tm depends upon and cannot survive without wide
-spread public support and donations to carry out its mission of
-increasing the number of public domain and licensed works that can be
-freely distributed in machine readable form accessible by the widest
-array of equipment including outdated equipment. Many small donations
-($1 to $5,000) are particularly important to maintaining tax exempt
-status with the IRS.
-
-The Foundation is committed to complying with the laws regulating
-charities and charitable donations in all 50 states of the United
-States. Compliance requirements are not uniform and it takes a
-considerable effort, much paperwork and many fees to meet and keep up
-with these requirements. We do not solicit donations in locations
-where we have not received written confirmation of compliance. To SEND
-DONATIONS or determine the status of compliance for any particular
-state visit www.gutenberg.org/donate
-
-While we cannot and do not solicit contributions from states where we
-have not met the solicitation requirements, we know of no prohibition
-against accepting unsolicited donations from donors in such states who
-approach us with offers to donate.
-
-International donations are gratefully accepted, but we cannot make
-any statements concerning tax treatment of donations received from
-outside the United States. U.S. laws alone swamp our small staff.
-
-Please check the Project Gutenberg Web pages for current donation
-methods and addresses. Donations are accepted in a number of other
-ways including checks, online payments and credit card donations. To
-donate, please visit: www.gutenberg.org/donate
-
-Section 5. General Information About Project Gutenberg-tm electronic works.
-
-Professor Michael S. Hart was the originator of the Project
-Gutenberg-tm concept of a library of electronic works that could be
-freely shared with anyone. For forty years, he produced and
-distributed Project Gutenberg-tm eBooks with only a loose network of
-volunteer support.
-
-Project Gutenberg-tm eBooks are often created from several printed
-editions, all of which are confirmed as not protected by copyright in
-the U.S. unless a copyright notice is included. Thus, we do not
-necessarily keep eBooks in compliance with any particular paper
-edition.
-
-Most people start at our Web site which has the main PG search
-facility: www.gutenberg.org
-
-This Web site includes information about Project Gutenberg-tm,
-including how to make donations to the Project Gutenberg Literary
-Archive Foundation, how to help produce our new eBooks, and how to
-subscribe to our email newsletter to hear about new eBooks.
-
diff --git a/old/52838-0.zip b/old/52838-0.zip
deleted file mode 100644
index 3535af7..0000000
--- a/old/52838-0.zip
+++ /dev/null
diff --git a/old/52838-h.zip b/old/52838-h.zip
deleted file mode 100644
index 1e32b95..0000000
--- a/old/52838-h.zip
+++ /dev/null
diff --git a/old/52838-h/52838-h.htm b/old/52838-h/52838-h.htm
deleted file mode 100644
index 998b932..0000000
--- a/old/52838-h/52838-h.htm
+++ /dev/null
@@ -1,4423 +0,0 @@
-<?xml version="1.0" encoding="utf-8"?>
-<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Strict//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-strict.dtd">
-<html xmlns="http://www.w3.org/1999/xhtml" xml:lang="en" lang="en">
-<head>
-<meta http-equiv="Content-Type" content="text/html;charset=utf-8" />
-<meta http-equiv="Content-Style-Type" content="text/css" />
-<title>Creation of the Teton Landscape; The Geologic Story of Grand Teton National Park, by J. D. Love and John C. Reed, Jr.: a Project Gutenberg eBook</title>
-<meta name="author" content="J. D. Love and John C. Reed, Jr." />
-<link rel="schema.DC" href="http://dublincore.org/documents/1998/09/dces/" />
-<meta name="DC.Creator" content="J. D. Love (****-****)" />
-<meta name="DC.Creator" content="John C. Reed, Jr. (****-****)" />
-<meta name="DC.Creator" content="United States Geological Survey" />
-<meta name="DC.Title" content="Creation of the Teton Landscape; The Geologic Story of Grand Teton National Park" />
-<meta name="DC.Language" content="en" />
-<meta name="DC.Format" content="text/html" />
-<meta name="DC.Created" content="1971" />
-<meta name="pss.pubdate" content="1971" />
-<style type="text/css">
-large { font-size:125%; }
-sc    { font-variant:small-caps; font-style: normal; }
-
-/* == GLOBAL MARKUP == */
-body, table.twocol tr td  { margin-left:2em; margin-right:2em; }   /* BODY */
-.box     { border-style:double; margin-bottom:2em; max-width:30em; margin-right:auto; margin-left:auto; margin-top:2em; }
-.box p   { margin-right:1em; margin-left:1em; }
-.box dl  { margin-right:1em; margin-left:1em; }
-h1, h6, .titlepg p { text-align:center; clear:both; }   /* HEADINGS */
-h2                { margin-top:1.5em; margin-bottom:1em; font-family:sans-serif; text-align:left; color:blue; }
-h2 span.center, h2.center         { font-family:serif; color:black; }
-h1                { margin-top:3em; }
-div.box h1        { margin-top:1em; }
-h3                { margin-top:2.5em; font-family:sans-serif; font-size:120%; text-align:left; color:blue; }
-h4                { font-size:100%; text-align:left; margin-top:1em; margin-bottom:.5em; }
-h5                { font-size:100%; text-align:right; clear:right; }
-h6                { font-size:100%; }
-h6.var            { font-size:80%; font-style:normal; }
-.titlepg          { margin-left:auto; margin-right:auto; border-style:double; clear:both; }
-span.chaptertitle { font-style:normal; display:block; text-align:center; font-size:150%; }
-.tblttl           { text-align:center; }
-.tblsttl          { text-align:center; font-variant:small-caps; }
-
-pre sub.ms { width:4em; letter-spacing:1em; }
-table.fmla { text-align:center; margin-top:0em; margin-bottom:0em; margin-left:0em; margin-right:0em; }
-table.inline, table.symbol { display: inline-table; vertical-align: middle; }
-td.cola           { text-align:left; vertical-align:100%; }
-td.colb           { text-align:justify; }
-
-p, blockquote, div.p, div.bq { text-align:justify; }                              /* PARAGRAPHS */
-div.p, div.bq   { margin-top:1em; margin-bottom:1em; }
-blockquote, .bq { margin-left:1em; margin-right:0em; }
-.verse    { font-size:100%; }
-p.indent  {text-indent:2em; text-align:left; }
-p.tb, p.tbcenter, verse.tb, blockquote.tb      { margin-top:2em; }
-
-span.pb, div.pb, dt.pb, p.pb                                      /* PAGE BREAKS */
-{ text-align:right; float:right; margin-right:0em; clear:right; }
-div.pb { display:inline; }
-.pb, dt.pb, dl.toc dt.pb, dl.tocl dt.pb, dl.index dt.pb, dl.undent dt.pb
-       { text-align:right; float:right; margin-left: 1.5em;
-         margin-top:.5em; margin-bottom:.5em; display:inline; text-indent:0;
-         font-size:80%; font-style:normal; font-weight:bold;
-         color:gray; border:1px solid gray;padding:1px 3px; }
-div.index .pb  { display:block; }
-.bq  div.pb, .bq span.pb  { font-size:90%; margin-right:2em; }
-
-div.img, body a img  {text-align:center; margin-left:auto; margin-right:auto; margin-top:2em; margin-bottom:2em; clear:right; }
-
-sup, a.fn { font-size:75%; vertical-align:100%; line-height:50%; font-weight:normal; font-family:normal; }
-h2   a.fn { font-size:55%; line-height:75%; }
-h3   a.fn { font-size:65%; }
-sub { font-size:75%; }
-.center, .tbcenter       { text-align:center; clear:both; }                  /* TEXTUAL MARKUP */
-span.center              { display:block; }
-table.center { clear:both; margin-right:auto; margin-left:auto; font-family:sans-serif; font-weight:normal; }
-table.center tr td.l  {text-align:left; }
-table.center tr td.lt {text-align:left; width:2em; }
-table.center tr td.t  {text-align:left; text-indent:1em; }
-table.center tr td.t2 {text-align:left; text-indent:2em; }
-table.center tr td.r  {text-align:right; }
-table.center tr th    {vertical-align:bottom; }
-table.center tr td    {vertical-align:top; }
-table.inline, table.symbol { display: inline-table; vertical-align: middle; }
-
-p           { clear:left; }
-.small, .lsmall      { font-size:90%; }
-.smaller    { font-size:80%; }
-.smallest   { font-size:67%; }
-.larger     { font-size:150%; }
-.large      { font-size:125%; }
-.xlarge     { font-size:200%; line-height:60%; }
-.xxlarge    { font-size:200%; line-height:60%; }
-.gs         { letter-spacing:1em; }
-.gs3        { letter-spacing:2em; }
-.gslarge    { letter-spacing:.3em; font-size:110%; }
-.sc         { font-variant:small-caps; font-style:normal; }
-.unbold     { font-weight:normal; }
-.xo         { position:relative; left:-.3em; }
-.over, over { text-decoration: overline; display:inline; }
-hr          { width:20%; }
-.jl         { text-align:left; }
-.jr         { text-align:right; min-width:2em; display:inline-block; float:right; }
-.jr1        { text-align:right; margin-right:2em; }
-h1 .jr      { margin-right:.5em; }
-.ind1       { text-align:left;  margin-left:2em; }
-.u          { text-decoration:underline; }
-.hst        { margin-left:2em; }
-.hst2       { margin-left:4em; }
-.rubric     { color:red; }
-.cnwhite    { color:white; background-color:black; min-width:2em; display:inline-block;
-              text-align:center; font-weight:bold; font-family:sans-serif; }
-.cwhite     { color:white; background-color:black; text-align:center; font-weight:bold;
-              font-family:sans-serif; }
-ul  li      { text-align:justify; }
-.ss         { font-family:sans-serif; font-weight:bold; font-size:90%; }
-
-dd.t           { text-align:left; margin-left: 5.5em; }
-dl.toc         { clear:both; margin-top:1em; }                    /* CONTENTS (.TOC) */
-.toc  dt       { margin-top:1em; }
-.toc  dt.center    { text-align:center; clear:both; margin-top:3em; margin-bottom:1em;}
-.toc  dt      { text-align:right; clear:left; }
-.toc  dd      { text-align:right; clear:both; margin-left:2em; }
-.toc  dd.ddt  { text-align:right; clear:both; margin-left:4em; }
-.toc  dd.ddt2 { text-align:right; clear:both; margin-left:5em; }
-.toc  dd.ddt3 { text-align:right; clear:both; margin-left:6em; }
-.toc  dd.ddt4 { text-align:right; clear:both; margin-left:7em; }
-.toc  dd.ddt5 { text-align:right; clear:both; margin-left:8em; }
-.toc  dd.note { text-align:justify; clear:both; margin-left:5em; text-indent:-1em; margin-right:3em; }
-.toc  dt .xxxtest {width:17em; display:block; position:relative; left:4em; }
-.toc  dt  a,
-.toc  dd  a,
-.toc dt span.left,
-.toc dt span.lsmall,
-.toc dd span.left { text-align:left; clear:right; float:left; }
-.toc  dt  a  span.cn { width:4em; text-align:right; margin-right:.7em;  float:left; }
-.toc  dt.sc   { text-align:right;  clear:both; }
-.toc  dt.scl  { text-align:left;   clear:both; font-variant:small-caps; }
-.toc  dt.sct  { text-align:right;  clear:both; font-variant:small-caps; margin-left:1em; }
-.toc  dt.jl   { text-align:left;   clear:both; font-variant:normal; }
-.toc  dt.scc  { text-align:center; clear:both; font-variant:small-caps; }
-.toc  dt span.lj { text-align:left; display:block; float:left; }
-.toc  dd.center { text-align:center; }
-dd.tocsummary {text-align:justify; margin-right:2em; margin-left:2em; }
-dd.center sc  {display:block; text-align:center; }
-/* BOX CELL */
-td.top { border-top:1px    solid; width:.5em; height:.8em; }
-td.bot { border-bottom:1px solid; width:.5em; height:.8em; }
-td.rb  { border:1px solid; border-left:none;  width:.5em; height:.8em;  }
-td.lb  { border:1px solid; border-right:none; width:.5em; height:.8em;  }
-
-
-
-                                                   /* INDEX (.INDEX) */
-dl.index   { clear:both; }
-.index dd  { margin-left:4em; text-indent:-2em; text-align:left; clear:both; }
-.index dd.ddt  { margin-left:6em; text-indent:-2em; text-align:left; }
-.index dt  { margin-left:2em; text-indent:-2em; text-align:left; clear:both; }
-.index dt.center {text-align:center; }
-.index dt.jr { text-align:right; text-indent:0; margin-left:0; margin-right:0; }
-
-.ab, .abl {
-font-weight:bold; text-decoration:none;
-border-style:solid; border-color:gray; border-width:1px;
-margin-right:0px; margin-top:5px; display:inline-block; text-align:center; }
-.ab { width:1em; }
-
-                                                           /* FOOTNOTE BLOCKS */
-div.notes p  { margin-left:1em; text-indent:-1em; text-align:justify; }
-
-dl.undent dt    { margin-left:3em;  text-indent:-3em; text-align:justify; }
-dl.undent dd    { margin-left:4em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t  { margin-left:5em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t2 { margin-left:6em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t3 { margin-left:7em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t4 { margin-left:8em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t5 { margin-left:9em;  text-indent:-3em; text-align:justify; }
-dl.undent dd.t6 { margin-left:10em; text-indent:-3em; text-align:justify; }
-                                                           /* POETRY LINE NUMBER */
-.lnum   { text-align:right; float:right; margin-left:.5em; display:inline; }
-
-.hymn     { text-align:left; }                                  /*  HYMN AND VERSE: HTML  */
-.verse    { text-align:left; margin-top:1em; margin-bottom:1em; margin-left:0em; }
-.versetb  { text-align:left; margin-top:2em; margin-bottom:1em; margin-left:0em; }
-.originc  { text-align:center; }
-.subttl   { text-align:center; font-size:80%; }
-.srcttl   { text-align:center; font-size:80%; font-weight:bold; }
-p.t0, p.l { margin-left:4em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.lb                 { margin-left:4em;  text-indent:-3em; margin-top:2em; margin-bottom:0; text-align:left; }
-p.tw, div.tw, .tw    { margin-left:1em;  text-indent:-1em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t,  div.t,  .t     { margin-left:5em;  text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t2,  div.t2,  .t2  { margin-left:6em;  text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t3,  div.t3,  .t3  { margin-left:7em;  text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t4,  div.t4,  .t4  { margin-left:8em;  text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t5,  div.t5,  .t5  { margin-left:9em;  text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t6,  div.t6,  .t6  { margin-left:10em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t7,  div.t7,  .t7  { margin-left:11em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t8,  div.t8,  .t8  { margin-left:12em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t9,  div.t9,  .t9  { margin-left:13em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t10, div.t10,.t10  { margin-left:14em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t11, div.t11,.t11  { margin-left:15em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t12, div.t12,.t12  { margin-left:16em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t13, div.t13,.t13  { margin-left:17em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t14, div.t14,.t14  { margin-left:18em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.t15, div.t15,.t15  { margin-left:19em; text-indent:-3em; margin-top:0; margin-bottom:0; text-align:left; }
-p.lr, div.lr, span.lr { display:block; margin-left:0em; margin-right:1em; margin-top:0; margin-bottom:0; text-align:right; }
-dt.lr                { width:100%; margin-left:0em; margin-right:0em; margin-top:0; margin-bottom:0; margin-top:1em; text-align:right; }
-dl dt.lr a           { text-align:left; clear:left; float:left; }
-
-.fnblock   { margin-top:2em; }
-.fndef     { text-align:justify; margin-top:1.5em; margin-left:1.5em; text-indent:-1.5em; }
-.fndef p.fncont, .fndef dl { margin-left:0em; text-indent:0em; }
-dl.catalog dd { font-style:italic; }
-dl.catalog dt { margin-top:1em; }
-.author { text-align:right; margin-top:0em; margin-bottom:0em; display:block; }
-
-dl.biblio  dt        { margin-top:.6em; margin-left:2em; text-indent:-2em; text-align:justify; clear:both; }
-dl.biblio  dt  div   { display:block; float:left; margin-left:-6em; width:6em; clear:both; }
-dl.biblio  dt.center { margin-left:0em; text-align:center; }
-dl.biblio  dd        { margin-top:.3em; margin-left:3em; text-align:justify; font-size:90%; }
-.clear     { clear:both; }
-p.book     { margin-left:2em; text-indent:-2em; }
-p.review   { margin-left:2em; text-indent:-2em; font-size:80%; }
-p.pcap, p.pcapc, p.ccap { margin-top:0em; font-weight:bold; font-size:90%; max-width:40em; margin-right:auto; margin-left:auto; }
-p.pcap     { text-align:justify; }
-p.ccap    { text-align:center; }
-span.pn    { display:inline-block; width:4.7em; text-align:left; margin-left:0; text-indent:0; }</style>
-</head>
-<body>
-
-
-<pre>
-
-The Project Gutenberg EBook of Creation of the Teton Landscape, by 
-J. D. Love and John C. Reed
-
-This eBook is for the use of anyone anywhere in the United States and most
-other parts of the world at no cost and with almost no restrictions
-whatsoever.  You may copy it, give it away or re-use it under the terms of
-the Project Gutenberg License included with this eBook or online at
-www.gutenberg.org.  If you are not located in the United States, you'll have
-to check the laws of the country where you are located before using this ebook.
-
-Title: Creation of the Teton Landscape
-       The Geologic Story of Grand Teton National Park
-
-Author: J. D. Love
-        John C. Reed
-
-Release Date: August 18, 2016 [EBook #52838]
-
-Language: English
-
-Character set encoding: UTF-8
-
-*** START OF THIS PROJECT GUTENBERG EBOOK CREATION OF THE TETON LANDSCAPE ***
-
-
-
-
-Produced by Stephen Hutcheson, Dave Morgan and the Online
-Distributed Proofreading Team at http://www.pgdp.net
-
-
-
-
-
-
-</pre>
-
-<div id="cover" class="img">
-<img id="coverpage" src="images/cover.jpg" alt="Creation of the Teton Landscape; The Geologic Story of Grand Teton National Park" width="500" height="764" />
-</div>
-<p class="pcap">View west toward Grand Teton on skyline. Hedrick&rsquo;s
-Pond surrounded by &ldquo;knob and kettle&rdquo;
-topography is in foreground, tree-covered Burned
-Ridge moraine is in middle distance, and extending
-from it to foot of mountains is gray flat treeless
-glacial outwash plain. <b><i>National Park Service
-photo by W. E. Dilley.</i></b></p>
-<div class="img" id="pic1">
-<img src="images/p03.jpg" alt="" width="635" height="1000" />
-<p class="pcap">View west up Cascade Canyon, with north face of
-Mt. Owen in center. <b><i>National Park Service
-photo by H. D. Pownall.</i></b></p>
-</div>
-<p class="center"><span class="large"><i>To Fritiof M. Fryxell, geologist, teacher,
-<br />writer, mountaineer, and the first ranger-naturalist
-<br />in Grand Teton National Park.</i></span></p>
-<p class="center"><span class="large"><i>All who love and strive to understand
-<br />the Teton landscape follow in his footsteps.</i></span></p>
-<div class="box">
-<h1><i>CREATION OF THE
-<br />TETON LANDSCAPE</i>
-<br /><span class="smaller">The Geologic Story of
-<br />Grand Teton National Park</span></h1>
-<p class="center"><i>By
-<br />J. D. LOVE AND JOHN C. REED, JR.
-<br />U.S. Geological Survey</i></p>
-<p class="center"><i>Library of Congress Catalogue Card No.</i>: 68-20628
-<br /><i>ISBN</i> O-931895-08-1</p>
-<p class="center">1st Edition
-<br />1968</p>
-<p class="center">1st Revised Edition
-<br />1971</p>
-<p class="center">Reprinted 1979
-<br />Reprinted 1984
-<br />Reprinted 1989</p>
-<p class="center">Grand Teton Natural History Association
-<br />Moose, Wyoming 83012</p>
-</div>
-<div class="pb" id="Page_4">4</div>
-<h2>CONTENTS</h2>
-<dl class="toc">
-<dt><a href="#c1">Foreword</a> 6</dt>
-<dt><a href="#c2"><b>THE STORY BEGINS</b></a> 8</dt>
-<dd><a href="#c3">First questions, brief answers</a> 9</dd>
-<dd><a href="#c4">An extraordinary story</a> 10</dd>
-<dd><a href="#c5">An astronaut&rsquo;s view</a> 12</dd>
-<dd><a href="#c6">A pilot&rsquo;s view</a> 14</dd>
-<dd><a href="#c7">A motorist&rsquo;s view</a> 15</dd>
-<dd class="ddt"><a href="#c8">View north</a> 15</dd>
-<dd class="ddt"><a href="#c9">View west</a> 18</dd>
-<dd class="ddt"><a href="#c10">View south</a> 19</dd>
-<dd><a href="#c11">A mountaineer&rsquo;s view</a> 20</dd>
-<dt><a href="#c12"><b>CARVING THE RUGGED PEAKS</b></a> 24</dt>
-<dd><a href="#c13">Steep mountain slopes&mdash;the perpetual battleground</a> 24</dd>
-<dd><a href="#c14">Rock disintegration and gravitational movement</a> 24</dd>
-<dd><a href="#c15">Running water cuts and carries</a> 26</dd>
-<dd><a href="#c16">Glaciers scour and transport</a> 28</dd>
-<dd><a href="#c17">Effects on Jackson Hole</a> 30</dd>
-<dt><a href="#c18"><b>MOUNTAIN UPLIFT</b></a> 36</dt>
-<dd><a href="#c19">Kinds of mountains</a> 36</dd>
-<dd><a href="#c20">Anatomy of faults</a> 38</dd>
-<dd><a href="#c21">Time and rate of uplift</a> 40</dd>
-<dd><a href="#c22">Why are mountains here?</a> 41</dd>
-<dd><a href="#c23">The restless land</a> 43</dd>
-<dt><a href="#c24"><b>ENORMOUS TIME AND DYNAMIC EARTH</b></a> 45</dt>
-<dd><a href="#c25">Framework of time</a> 45</dd>
-<dd><a href="#c26">Rocks and relative age</a> 45</dd>
-<dd><a href="#c27">Fossils and geologic time</a> 46</dd>
-<dd><a href="#c28">Radioactive clocks</a> 47</dd>
-<dd><a href="#c29">The yardstick of geologic time</a> 48</dd>
-<dt><a href="#c30"><b>PRECAMBRIAN ROCKS&mdash;THE CORE OF THE TETONS</b></a> 51</dt>
-<dd><a href="#c31">Ancient gneisses and schists</a> 51</dd>
-<dd><a href="#c32">Granite and pegmatite</a> 55</dd>
-<dd><a href="#c33">Black dikes</a> 58</dd>
-<dd><a href="#c34">Quartzite</a> 63</dd>
-<dd><a href="#c35">A backward glance</a> 64</dd>
-<dd><a href="#c36">The close of the Precambrian&mdash;end of the beginning</a> 64</dd>
-<dt><a href="#c37"><b>THE PALEOZOIC ERA&mdash;TIME OF LONG-VANISHED SEAS AND THE DEVELOPMENT OF LIFE</b></a> 66</dt>
-<dd><a href="#c38">The Paleozoic sequence</a> 66</dd>
-<dd><a href="#c39">Alaska Basin&mdash;site of an outstanding rock and fossil record</a> 66</dd>
-<dd><a href="#c40">Advance and retreat of Cambrian seas; an example</a> 69</dd>
-<dd><a href="#c41">Younger Paleozoic formations</a> 74</dd>
-<dt><a href="#c42"><b>THE MESOZOIC&mdash;ERA OF TRANSITION</b></a> 79</dt>
-<dd><a href="#c43">Colorful first Mesozoic strata</a> 79</dd>
-<dd><a href="#c44">Drab Cretaceous strata</a> 81</dd>
-<dd><a href="#c45">Birth of the Rocky Mountains</a> 82</dd>
-<dt><a href="#c46"><b>TERTIARY&mdash;TIME OF MAMMALS, MOUNTAINS, LAKES, AND VOLCANOES</b></a> 86</dt>
-<dd><a href="#c47">Rise and burial of mountains</a> 88</dd>
-<dd><a href="#c48">The first big lake</a> 92</dd>
-<dd><a href="#c49">Development of mammals</a> 95</dd>
-<dd><a href="#c50">Volcanoes</a> 98</dd>
-<dt><a href="#c51"><b>QUATERNARY&mdash;TIME OF ICE, MORE LAKES, AND CONTINUED CRUSTAL DISTURBANCE</b></a> 102</dt>
-<dd><a href="#c52">Hoback normal fault</a> 103</dd>
-<dd><a href="#c53">Volcanic activity</a> 103</dd>
-<dd><a href="#c54">Preglacial lakes</a> 104</dd>
-<dd><a href="#c55">The Ice Age</a> 105</dd>
-<dd><a href="#c56">Modern glaciers</a> 112</dd>
-<dt><a href="#c57"><b>THE PRESENT AND THE FUTURE</b></a> 113</dt>
-<dt><a href="#c58"><b>APPENDIX</b></a> 115</dt>
-<dd><a href="#c59">Acknowledgements</a> 115</dd>
-<dd><a href="#c60">Selected references&mdash;if you wish to read further</a> 116</dd>
-<dd><a href="#c61">About the authors</a> 117</dd>
-<dd><a href="#c62">Index of selected terms and features</a> 118</dd>
-</dl>
-<div class="pb" id="Page_6">6</div>
-<h2 id="c1"><br /><span class="small"><i><span class="center">FOREWORD</span></i></span></h2>
-<p>Geology is the science of the Earth&mdash;the study of
-the forces, processes, and past life that not only shape our
-land but influence our daily lives and our Nation&rsquo;s welfare.
-This booklet, prepared by two members of the U.S.
-Geological Survey, discusses how geologic phenomena are
-responsible for the magnificent scenery of the Teton region.</p>
-<p>Recognition of the complex geologic history of our
-Earth is vital to the enjoyment and appreciation of beautiful
-landscapes and other natural wonders, to the planning
-of our cities and highway systems, to the wise use of our
-water supplies, to the study of earthquake and landslide
-areas, to the never-ending search for new mineral deposits,
-and to the conservation and development of our known
-natural resources. Who can say, in the long run, which of
-the many uses of this knowledge is the most compelling
-reason to seek an understanding of the Earth?</p>
-<div class="img">
-<img src="images/p05.jpg" alt="Signature" width="200" height="72" />
-</div>
-<p class="jr1">W. T. Pecora, <i>Director</i>
-<br />U.S. Geological Survey</p>
-<p class="center small"><i>This booklet is based on geologic investigations by the
-<br />U. S. Geological Survey in cooperation with the National Park Service,
-<br />U. S. Department of Interior.</i></p>
-<div class="pb" id="Page_7">7</div>
-<div class="verse">
-<p class="t0"><span class="large">&ldquo;<i>Something hidden. Go and find it.</i></span></p>
-<p class="t0"><span class="large"><i>Go and look behind the Ranges&mdash;</i></span></p>
-<p class="t0"><span class="large"><i>Something lost behind the Ranges.</i></span></p>
-<p class="t0"><span class="large"><i>Lost and waiting for you. Go.</i>&rdquo;</span></p>
-<p class="lr"><span class="small">KIPLING&mdash;<i>THE EXPLORER</i></span></p>
-</div>
-<div class="pb" id="Page_8">8</div>
-<h2 id="c2"><br /><span class="small">THE STORY BEGINS</span></h2>
-<p>The Teton Range is one of the most magnificent
-mountain ranges on the North American Continent. Others
-are longer, wider, and higher, but few can rival the breath-taking
-alpine grandeur of the eastern front of the Tetons.
-Ridge after jagged ridge of naked rock soar upward into
-the western sky, culminating in the towering cluster of
-peaks to which the early French voyageurs gave the name
-&ldquo;<i>les Trois Tetons</i>&rdquo; (the three breasts). The range hangs
-like a great stone wave poised to break across the valley at
-its base. To the south and east are lesser mountains, interesting
-and scenic but lacking the magic appeal of the
-Tetons.</p>
-<p>This is a range of many moods and colors: stark and
-austere in morning sun, but gold and purple and black in
-the softly lengthening shadows of afternoon; somber and
-foreboding when the peaks wrap themselves in the tattered
-clouds of an approaching storm, but tranquil and ethereal
-blue and silver beneath a full moon.</p>
-<p>These great peaks and much of the floor of the valley
-to the east, <i>Jackson Hole</i> (a <i>hole</i> was the term used by pioneer
-explorers and mountain men to describe any open valley
-encircled by mountains), lie within Grand Teton National
-Park, protected and preserved for the enjoyment of
-present and future generations. Each year more than 3
-million visitors come to the park. Many pause briefly and
-pass on. Others stay to explore its trails, fish its streams,
-study the plants and wildlife that abound within its borders,
-or to savor the colorful human history of this area.</p>
-<p>Most visitors, whatever their interests and activities,
-are probably first attracted to the park by its unsurpassed
-mountain scenery. The jagged panorama of the Tetons is
-the backdrop to which they may turn again and again, asking
-questions, seeking answers. How did the mountains
-form? How long have they towered into the clouds, washed
-by rain, riven by frost, swept by wind and snow? What
-enormous forces brought them forth and raised them skyward?
-<span class="pb" id="Page_9">9</span>
-What stories are chronicled in their rocks, what
-epics chiseled in the craggy visage of this mountain landscape?
-Why are the Tetons different from other mountains?</p>
-<h3 id="c3">First questions, brief answers</h3>
-<p><i>How did the Tetons and Jackson Hole form?</i> They
-are both tilted blocks of the earth&rsquo;s crust that behaved like
-two adjoining giant trapdoors hinged so that they would
-swing in opposite directions. The block on the west, which
-forms the Teton Range, was hinged along the Idaho-Wyoming
-State line; the eastern edge was uplifted along a fault
-(a fracture along which displacement has occurred). This
-is why the highest peaks and steepest faces are near the east
-margin of the range. The hinge line of the eastern block,
-which forms Jackson Hole, was in the highlands to the east.
-The western edge of the block is downdropped along the
-fault at the base of the Teton Range. As a consequence, the
-floor of Jackson Hole tilts westward toward the Tetons (see
-cross section inside back cover).</p>
-<p><i>When did the Tetons and Jackson Hole develop the
-spectacular scenery we see today?</i> The Tetons are the
-youngest of all the mountain ranges in the Rocky Mountain
-chain. Most other mountains in the region are at least 50
-million years old but the Tetons are less than 10 million
-and are still rising. Jackson Hole is of the same age and is
-still sinking. The Teton landscape is the product of many
-earth processes, the most recent of which is cutting by
-water and ice. Within the last 15,000 years, ice sculpturing
-of peaks and canyons and impounding of glacial lakes have
-added finishing touches to the scenic beauty.</p>
-<p><i>Why did the Tetons rise and Jackson Hole sink?</i> For
-thousands of years men have wondered about the origin of
-mountains and their speculations have filled many books.
-Two of the more popular theories are: (1) continental drift
-(such as South America moving away from Africa), with
-the upper lighter layer of the earth&rsquo;s crust moving over the
-lower denser layer and wrinkling along belts of weakness;
-and (2) convection currents within the earth, caused by
-heat transfer, resulting in linear zones of wrinkling, uplift,
-and collapse.</p>
-<div class="pb" id="Page_10">10</div>
-<p>These concepts were developed to explain the origin of
-mountainous areas hundreds or thousands of miles long but
-they do not answer directly the question of why the Tetons
-rose and Jackson Hole sank. As is discussed in the chapter
-on mountains, it is probable that semifluid rock far below
-the surface of Jackson Hole flowed north into the Yellowstone
-Volcanic Plateau-Absaroka Range volcanic area, perhaps
-taking the place of the enormous amount of ash and
-lava blown out of volcanoes during the last 50 million
-years. The origin of the line of weakness that marks the
-Teton fault along the east face of the Teton Range may go
-back to some unknown inequality in the earth&rsquo;s composition
-several billion years ago. Why it suddenly became active
-late in the earth&rsquo;s history is an unanswered question.</p>
-<p>The ultimate source of heat and energy that caused the
-mountains and basins to form probably is disintegration of
-radioactive materials deep within the earth. The Tetons are
-a spectacular demonstration that the enormous energy
-necessary to create mountains is not declining, even though
-our planet is several billion years old.</p>
-<h3 id="c4">An extraordinary story</h3>
-<p>Visitors whose curiosity is whetted by this unusual and
-varied panorama are not satisfied with only a few questions
-and answers. They sense that here for the asking is an
-extraordinary <i>geologic</i> (<i>geo</i>&mdash;earth; <i>logic</i>&mdash;science) story.
-With a little direction, many subtle features become evident&mdash;features
-that otherwise might escape notice. Here, for
-example, is a valley with an odd U-shape. There is a sheer
-face crisscrossed with light- and dark-colored rocks. On the
-valley floor is a tuft of pine trees that seem to be confined
-to one particular kind of rock. On the rolling hills is a layer
-of peculiar white soil&mdash;the only soil in which coyote
-dens are common. All these are geologically controlled
-phenomena. In short, with a bit of initial guidance, the
-viewer gains an ability to observe and to understand so
-much that the panorama takes on new depth, vividness, and
-excitement. It changes from a flat, two-dimensional picture
-to a colorful multi-dimensional exhibit of the earth&rsquo;s
-history.</p>
-<div class="pb" id="Page_11">11</div>
-<div class="img" id="fig1">
-<img src="images/map1_lr.jpg" alt="" width="600" height="805" />
-<p class="pcap">Figure 1. <i>The Tetons from afar&mdash;an astronaut&rsquo;s view of the range and adjacent mountains, basins,
-and plateaus. Width of area shown in photo is about 100 miles. Stippled pattern marks boundary
-of Grand Teton National Park.</i><br /><span class="center"><a class="abl" href="images/map1_hr.jpg">High-resolution Map</a></span></p>
-</div>
-<div class="pb" id="Page_12">12</div>
-<div class="img" id="fig2">
-<img src="images/p07.jpg" alt="" width="1000" height="491" />
-<p class="pcap">Figure 2. <i>Sketch of the Teton Range
-and Jackson Hole, southwest view.
-Drawing by J. R. Stacy.</i></p>
-<p class="pcap"><span class="ss">BLOCK DIAGRAM VIEW SOUTHWEST SHOWING
-THE TETON RANGE AND JACKSON HOLE</span></p>
-</div>
-<h3 id="c5">An astronaut&rsquo;s view</h3>
-<p>The Tetons are a short, narrow, and high mountain
-range, distinctive in the midst of the great chain of the
-Rocky Mountains, the backbone of western North America.
-<a href="#fig1">Figure 1</a> shows how the Tetons and their surroundings
-might appear if you viewed them from a satellite at an altitude
-of perhaps a hundred miles. The U.&nbsp;S. Geological Survey
-topographic map of Grand Teton National Park shows
-the names of many features not indicated on <a href="#fig1">figure 1</a> or on
-the <a href="#fig62">geologic map</a> inside the back cover. The Teton Range is
-a rectangular mountain block about 40 miles long and 10-15
-miles wide. It is flanked on the east and west by flat-floored
-valleys. Jackson Hole is the eastern one and Teton
-Basin (called Pierre&rsquo;s Hole by the early trappers) is the
-western.</p>
-<p>The Teton Range is not symmetrical. The highest
-peaks lie near the eastern edge of the mountain block,
-rather than along its center, as is true in conventional
-mountains, and the western slopes are broad and gentle in
-<span class="pb" id="Page_13">13</span>
-contrast to the precipitous eastern slopes. The northern end
-of the range disappears under enormous lava flows that
-form the Yellowstone Volcanic Plateau. Even from this
-altitude the outlines of some of these flows can be seen.</p>
-<p>On the south the Teton Range abuts almost at right
-angles against a northwest-trending area of lower and less
-rugged mountains (the Snake River, Wyoming, and Hoback
-Ranges). These mountains appear altogether different
-from the Tetons. They consist of a series of long parallel
-ridges cut or separated by valleys and canyons. This pattern
-is characteristic of mountains composed of crumpled,
-steeply tilted rock layers&mdash;erosion wears away the softer
-layers, leaving the harder ones standing as ridges.</p>
-<p>On the east and northeast, Jackson Hole is bounded by
-the Gros Ventre and Washakie Ranges, which are composed
-chiefly of folded hard and soft sedimentary rocks. In contrast,
-<span class="pb" id="Page_14">14</span>
-between these mountains and the deepest part of Jackson
-Hole to the west, thick layers of soft nearly flat-lying
-sedimentary rocks have been sculptured by streams and ice
-into randomly oriented knife-edge ridges and rolling hills
-separated by broad valleys. The hills east of the park are
-called the Mount Leidy Highlands and those northeast are
-the Pinyon Peak Highlands.</p>
-<h3 id="c6">A pilot&rsquo;s view</h3>
-<p>If you descend from 100 miles to about 5 miles above
-the Teton region, the asymmetry of the range, the extraordinary
-variety of landscapes, and the vivid colors of
-rocks become more pronounced.</p>
-<p><a href="#fig2">Figure 2</a> shows a panorama of the Teton Range and
-Jackson Hole from a vantage point over the Pinyon Peak
-Highlands. The rough steep slopes and jagged ridges along
-the east front of the range contrast with smoother slopes
-and more rounded ridges on the western side. Nestled at
-the foot of the mountains and extending out onto the floor
-of Jackson Hole are tree-rimmed sparkling lakes of many
-sizes and shapes. Still others lie in steep-sided rocky
-amphitheaters near the mountain crests.</p>
-<p>One of the most colorful flight routes into Jackson
-Hole is from the east, along the north flank of the Gros
-Ventre Mountains. For 40 miles this mountain range is
-bounded by broad parallel stripes of bright-red, pink, purple,
-gray, and brown rocks. Some crop out as cliffs or
-ridges, and others are <i>badlands</i> (bare unvegetated hills and
-valleys with steep slopes and abundant dry stream channels).
-In places the soft beds have broken loose and flowed
-down slopes like giant varicolored masses of taffy. These
-are mudflows and landslides. The colorful rocks are
-bounded on the south by gray and yellow tilted layers forming
-snowcapped peaks of the Gros Ventre Mountains.</p>
-<p>These landscapes are the product of many natural
-forces acting on a variety of rock types during long or short
-intervals of geologic time. Each group of rocks records a
-chapter in the geologic story of the region. Other chapters
-can be read from the tilting, folding, and breaking of the
-rocks. The latest episodes are written on the face of the
-land itself.</p>
-<div class="pb" id="Page_15">15</div>
-<h3 id="c7">A motorist&rsquo;s view</h3>
-<p>Most park visitors first see the Teton peaks from the
-highway. Whether they drive in from the south, east, or
-north, there is one point on the route at which a spectacular
-panorama of the Tetons and Jackson Hole suddenly appears.
-Part of the thrill of these three views is that they are
-so unexpected and so different. The geologic history is
-responsible for these differences.</p>
-<h4 id="c8"><i>View north.</i>&mdash;</h4>
-<p>Throughout the first 4 miles north of
-the town of Jackson, the view of the Tetons from U.&nbsp;S.
-26-89 is blocked by East Gros Ventre Butte. At the north
-end of the butte, the highway climbs onto a flat upland
-at the south boundary of Grand Teton National Park.
-Without any advance warning, the motorist sees the whole
-east front of the Teton Range rising steeply from the amazingly
-flat floor of Jackson Hole.</p>
-<p>From the park boundary turnout no lakes or rivers are
-visible to the north but the nearest line of trees in the direction
-of the highest Teton peaks marks the approximate position
-of the Gros Ventre River. The elevation of this river is
-surprising, for the route has just come up a 150-foot hill,
-out of the flat valley of a much smaller stream, yet here at
-eye-level is a major river perched on an upland plain. The
-reason for these strange relations is that the hill is a fault
-scarp (see <a href="#fig16A">fig. 16A</a> for a diagram) and the valley in which
-the town of Jackson is located was dropped 150 feet or
-more in the last 15,000 years.</p>
-<p>On the skyline directly west of the turnout are horizontal
-and inclined layers of rocks. These once extended
-over the tops of the highest peaks but were worn away from
-some parts as the mountains rose. All along the range, trees
-grow only up to <i>treeline</i> (also called <i>timberline</i>&mdash;a general
-elevation above which trees do not grow) which here is
-about 10,500 feet above the sea. To the southeast and east,
-beyond the sage-covered floor of Jackson Hole, are rolling
-partly forested slopes marking the west end of the Gros
-Ventre Mountains. They do not look at all like the Tetons
-because they were formed in a very different manner. The
-Gros Ventres are folded mountains that have foothills; the
-Tetons are faulted mountains that do not.</p>
-<div class="pb" id="Page_16">16</div>
-<div class="img" id="fig3">
-<p class="pcap">Figure 3. <i>The Teton landscape as seen from Signal Mountain.</i></p>
-</div>
-<div class="img" id="fig3A">
-<img src="images/v1_lr.jpg" alt="" width="1000" height="282" />
-<p class="pcap">A. <i>View west across Jackson Lake. Major peaks, canyons,
-and outcrops of sedimentary rocks are indicated by <span class="ss">&ldquo;s.&rdquo;</span></i><br /><span class="center"><a class="abl" href="images/v1_hr.jpg">High-resolution View</a></span></p>
-</div>
-<div class="pb" id="Page_17">17</div>
-<div class="img" id="fig3B">
-<img src="images/v2_lr.jpg" alt="" width="1000" height="308" />
-<p class="pcap">B. <i>View northeast; a study in contrast with the panorama above.</i><br /><span class="center"><a class="abl" href="images/v2_hr.jpg">High-resolution View</a></span></p>
-</div>
-<div class="pb" id="Page_18">18</div>
-<p>Three steepsided hills called <i>buttes</i> rise out of the flat
-floor of Jackson Hole. They are tilted and faulted masses
-of hard, layered rock that have been shaped by southward-moving
-glaciers. Six miles north of the boundary turnout
-is Blacktail Butte, on the flanks of which are west-dipping
-white beds. Southwest of the turnout is East Gros Ventre
-Butte, composed largely of layered rocks that are exposed
-along the road from Jackson almost to the turnout. These
-are capped by very young lava that forms the brown cliff
-overlooking the highway at the north end of the butte. To
-the southwest is West Gros Ventre Butte, composed of similar
-rocks.</p>
-<h4 id="c9"><i>View west.</i>&mdash;</h4>
-<p>The motorist traveling west along U.&nbsp;S.
-26-287 is treated to two magnificent views of the Teton
-Range. The first is 8 miles and the second 13 miles west
-of Togwotee Pass. At these vantage points, between 20
-and 30 miles from the mountains, the great peaks seem half
-suspended between earth and sky&mdash;too close, almost, to
-believe, but too distant to comprehend.</p>
-<p>Only from closer range can the motorist begin to appreciate
-the size and steepness of the mountains and to discern
-the details of their architecture. The many roads on
-the floor of Jackson Hole furnish ever-changing vistas, and
-signs provided by the National Park Service at numerous
-turnouts and scenic overlooks help the visitor to identify
-quickly the major peaks and canyons and the principal features
-of the valley floor. Of all these roadside vantage
-points, the top of Signal Mountain, an isolated hill rising
-nearly 1,000 feet out of the east margin of Jackson Lake,
-probably offers the best overall perspective (<a href="#fig3">fig. 3</a>). To the
-west, across the shimmering blue waters of Jackson Lake,
-the whole long parade of rugged peaks stretches from the
-north horizon to the south, many of the higher ones wearing
-the tattered remnants of winter snow. From here, only 8
-miles away, the towering pinnacles, saw-toothed ridges, and
-deep U-shaped canyons are clearly visible.</p>
-<p>Unlike most other great mountain ranges, the Tetons rise
-steeply from the flat valley floor in a straight unbroken
-line. The high central peaks tower more than a mile above
-the valley, but northward and southward the peaks diminish
-<span class="pb" id="Page_19">19</span>
-in height and lose their jagged character, gradually giving
-way to lower ridges and rounded hills. Some of the details
-of the mountain rock can be seen&mdash;gnarled gray rocks of
-the high peaks threaded by a fine white lacework of dikes,
-the dark band that cleaves through Mount Moran from base
-to summit, and the light brown and gray layers on the
-northern and southern parts of the range.</p>
-<p>At first glance the floor of Jackson Hole south of Signal
-Mountain seems flat, smooth, and featureless, except
-for the Snake River that cuts diagonally across it. Nevertheless,
-even the flats show a variety of land forms. The
-broad sage-covered areas, low isolated hills, and hummocky
-tree-studded ridges that form the foreground are all parts
-of the Teton landscape, and give us clues to the natural processes
-that shaped it. A critical look to the south discloses
-more strange things. We take for granted the fact that the
-sides of normal valleys slope inward toward a central major
-stream. South of Signal Mountain, however, the visitor
-can see that the Snake River Valley does not fit this description.
-The broad flat west of the river should slope east but
-it does not. Instead, it has been tilted westward by downward
-movement along the Teton fault at the base of the
-mountains.</p>
-<h4 id="c10"><i>View south.</i>&mdash;</h4>
-<p>About a million motorists drive south
-from Yellowstone to Grand Teton National Park each year.
-As they wind along the crooked highway on the west brink
-of Lewis River Canyon (<a href="#fig1">fig. 1</a>), the view south is everywhere
-blocked by dense forest. Then, abruptly the road
-leaves the canyon, straightens out, and one can look south
-down a 3-mile sloping avenue cut through the trees. There,
-20 to 30 miles away, framed by the roadway, are the snow-capped
-Tetons, with Jackson Lake, luminous in reflected
-light, nestled against the east face. This is one of the loveliest
-and most unusual views of the mountains that is available
-to the motorist, partly because he is 800 feet above the
-level of Jackson Lake and partly because this is the only
-place on a main highway where he can see clearly the third
-dimension (width) of the Tetons. The high peaks are on
-the east edge; they rise 7,000 feet above the lake but other
-peaks and precipitous ridges, progressively diminishing in
-<span class="pb" id="Page_20">20</span>
-height, extend on to the west for a dozen miles (<a href="#fig14">fig. 14</a>).
-Giant, relatively young lava flows, into which the Lewis
-River Canyon was cut, poured southward all the way to the
-shore of Jackson Lake and buried the north end of the Teton
-Range (figs. <a href="#fig13">13</a> and <a href="#fig53">53</a>). South of Yellowstone Park these
-flows were later tilted and broken by the dropping of Jackson
-Hole and the rise of the mountains.</p>
-<h3 id="c11">A mountaineer&rsquo;s view</h3>
-<p>As in many pursuits in life, the greatest rewards of a
-visit to the Tetons come to those who expend a real effort to
-earn them. Only by leaving the teeming valley and going
-up into the mountains to hike the trails and climb the peaks
-can the visitor come to know the Tetons in all their moods
-and changes and view close at hand the details of this
-magnificent mountain edifice.</p>
-<p>Even a short hike to Hidden Falls and Inspiration
-Point affords an opportunity for a more intimate view
-of the mountains. Along the trail the hiker can examine
-outcrops of sugary white granite, glittering mica-studded
-dikes, and dark intricately layered rocks. Nearby are
-great piles of broken fragments that have fallen from
-the cliffs above, and the visitor can begin to appreciate how
-vulnerable are the towering crags to the relentless onslaught
-of frost and snow. The roar of the foaming stream and the
-thunder of the falls are constant reminders of the patient
-work of running water in wearing away the &ldquo;everlasting
-hills.&rdquo; Running his hand across one of the smoothly polished
-rock faces below Inspiration Point, the hiker gains an
-unforgettable concept of the power of glacial ice and its
-importance in shaping this majestic landscape. Looking
-back across Jenny Lake at the encircling ridge of glacial
-debris, he can easily comprehend the size of the ancient
-glacier that once flowed down Cascade Canyon and
-emerged onto the floor of Jackson Hole.</p>
-<p>The more ambitious hiker or mountaineer can seek out
-the inner recesses of the range and explore other facets of
-its geology. He can visit the jewel-like mountain lakes&mdash;Solitude,
-Holly, and Amphitheater are just a few&mdash;cradled
-in high remote basins left by the Ice Age glaciers. He can
-<span class="pb" id="Page_21">21</span>
-get a closeup view of the Teton Glacier above Amphitheater
-Lake, or explore the Schoolroom Glacier, the tiny ice body
-below Hurricane Pass. He may follow the trail into Garnet
-Canyon to see the crystals from which the canyon takes its
-name and to examine the soaring ribbonlike black dike near
-the end of the trail. In Alaska Basin he can study the gently
-tilted layers of sandstone, limestone, and shale that once
-blanketed the entire Teton Range and can search for the
-fossils that help determine their age and decipher their history.
-From Hurricane Pass he can see how these even layers
-of sedimentary rock have been broken and displaced
-and how the older harder rocks that form the highest Teton
-peaks have been raised far above them along the Buck
-Mountain fault.</p>
-<p>Of all those who explore the high country, it is the
-mountaineer who has perhaps the greatest opportunity to
-appreciate its geologic story. Indeed, the success of his
-climb and his very life may depend on an intuitive grasp of
-the mountain geology and the processes that shaped the
-peaks. He observes the most intimate details&mdash;the inclination
-of the joints and fractures, which gullies are swept by
-falling rocks, which projecting knobs are firm, and which
-cracks will safely take a piton. To many climbers the ascent
-of a peak is a challenge to technical competence, endurance,
-and courage, but to those endowed with curiosity and a
-sharp eye it can be much more. As he stands shoulder to
-shoulder with the clouds on some windswept peak, such as
-the Grand Teton, with the awesome panorama dropping
-away on all sides, he can hardly avoid asking how this came
-to be. What does the mountaineer see that inspires this
-curiosity? From the very first glance, it is apparent that
-the scenes to the north, south, east, and west are startlingly
-different.</p>
-<p>Looking west from the rough, narrow, weather-ravaged
-granite summit of the Grand Teton, one sees far below
-him the layered gray cliffs of <i>marine sedimentary rocks</i>
-(solidified sediment originally deposited in a shallow arm
-of the ocean) overlapping the granite and dipping gently
-west, finally disappearing under the checkerboard farmland
-of Teton Basin. Still farther west are the rolling timbered
-<span class="pb" id="Page_22">22</span>
-slopes of the Big Hole Range in Idaho. A glance at
-the foreground, 3,000 feet below, shows some unusual relations
-of the streams to the mountains. The watershed divide
-of the Teton Range is not marked by the highest peaks as
-one would expect. Streams in Cascade Canyon and in other
-canyons to the north and south begin west of the peaks, bend
-around them, then flow eastward in deep narrow gorges cut
-through the highest part of the range, and emerge onto the
-flat floor of Jackson Hole.</p>
-<p>In the view north along the crest of the Teton Range,
-the asymmetry of the mountains is most apparent. The
-steep east face culminating in the highest peaks contrasts
-with the lower more gentle west flank of the uplift. From
-the Grand Teton it is not possible to see the actual place
-where the mountains disappear under the lavas of Yellowstone
-Park, but the heavily timbered broad gentle surface of
-the lava plain is visible beyond the peaks and extends
-across the entire north panorama. Still farther north, 75 to
-100 miles away, rise the snowcapped peaks (from northwest
-to northeast) of the Madison, Gallatin, and Beartooth
-Mountains.</p>
-<p>The view east presents the greatest contrasts in the
-shortest distances&mdash;the flat floor of Jackson Hole is 3 miles
-away and 7,000 feet below the top of the Grand Teton.
-Along the junction of the mountains and valley floor are
-blue glacial lakes strung out like irregular beads in a necklace.
-They are conspicuously rimmed by black-appearing
-margins of pine trees that grow only on the surrounding
-glacial moraines. Beyond these are the broad treeless
-boulder-strewn plains of Jackson Hole. Fifty miles to the
-east and northeast, on the horizon beyond the rolling hills
-of the Pinyon Peak Highlands, are the horizontally layered
-volcanic rocks of the Absaroka Range. Southeast is the
-colorful red, purple, green, and gray Gros Ventre River
-Valley, with the fresh giant scar of the Lower Gros Ventre
-Slide near its mouth. Bounding the south side of this valley
-are the peaks of the Gros Ventre Mountains, whose tilted
-slabby gray cliff-forming layers resemble (and are the
-same as) those on the west flank of the Teton Range. Seventy
-miles away, in the southeast distance, beyond the Gros
-<span class="pb" id="Page_23">23</span>
-Ventre Mountains are the shining snowcapped peaks of the
-Wind River Range, the highest peak of which (Gannett
-Peak) is about 20 feet higher than the Grand Teton.</p>
-<p>Conspicuous on the eastern and southeastern skyline
-are high-level (11,000-12,000 feet) flat-topped surfaces
-on both the Wind River and Absaroka Ranges. These are
-remnants that mark the upper limit of sedimentary fill of
-the basins adjacent to the mountains. A plain once connected
-these surfaces and extended westward at least as far
-as the conspicuous flat on the mountain south of Lower
-Gros Ventre Slide. It is difficult to imagine the amount of
-rock that has been washed away from between these remnants
-in comparatively recent geologic time, during and
-after the rise of the Teton Range.</p>
-<p>From this vantage point the mountaineer also gets a
-concept of the magnitude of the first and largest glaciers
-that scoured the landscape. Ice flowed southwestward in an
-essentially unbroken stream from the Beartooth Mountains,
-100 miles away, westward from the Absaroka Range, and
-northwestward from the Wind River Range (<a href="#fig57">fig. 57</a>). Ice
-lapped up to treeline on the Teton Range and extended
-across Jackson Hole nearly to the top of the Lower Gros
-Ventre Slide. The Pinyon Peak and Mount Leidy Highlands
-were almost buried. All these glaciers came together
-in Jackson Hole and flowed south within the ever-narrowing
-Snake River Valley.</p>
-<p>The view south presents a great variety of contrasts.
-Conspicuous, as in the view north, is the asymmetry of the
-range. South of the high peaks of crystalline rocks, gray
-layered cliffs of limestone extend in places all the way to
-the steep east face of the Teton Range where they are
-abruptly cut off by the great Teton fault.</p>
-<p>The flat treeless floor of Jackson Hole narrows southward.
-Rising out of the middle are the previously described
-steepsided ice-scoured rocky buttes. Beginning near the
-town of Jackson, part of which is visible, and extending as
-far south as the eye can see are row upon row of sharp
-ridges and snowcapped peaks that converge at various
-angles. These are the Hoback, Wyoming, Salt River, and
-Snake River Ranges.</p>
-<div class="pb" id="Page_24">24</div>
-<h2 id="c12"><br /><span class="small">CARVING THE RUGGED PEAKS</span></h2>
-<p>The rugged grandeur of the Tetons is a product of
-four geologic factors: the tough hard rocks in the core, the
-amount of vertical uplift, the recency of the mountain-making
-movement, and the dynamic forces of destruction.
-Many other mountains in Wyoming have just as hard rocks
-in their cores and an equally great amount of vertical uplift,
-but they rose 50 to 60 million years ago and have been
-worn down by erosion from that time on. The Tetons, on
-the other hand, are the youngest range in Wyoming, less
-than 10 million years old, and have not had time to be so
-deeply eroded.</p>
-<h3 id="c13">Steep mountain slopes&mdash;the perpetual battleground</h3>
-<p>Any steep slope or cliff is especially vulnerable to
-nature&rsquo;s methods of destruction. In the Tetons we see the
-never-ending struggle between two conflicting factors. The
-first is the extreme toughness of the rocks and their consequent
-resistance to erosion. The second is the presence of
-efficient transporting agencies that move out and away
-from the mountains all rock debris that might otherwise
-bury the lower slopes.</p>
-<p>The rocks making up most of the Teton Range are
-among the hardest, toughest, and least porous known.
-Therefore, they resist mechanical disintegration by temperature
-changes, ice, and water. They consist predominantly
-of minerals that are subject to very little chemical decay in
-the cold climate of the Tetons.</p>
-<p>Absence of weak layers prevents breaking of the tough
-rock masses under their own weight. All these conditions,
-then, are favorable for preservation of steep walls and high
-rock pinnacles. Nevertheless, they do break down. Great
-piles of broken rock <i>(talus)</i> that festoon the slopes of all
-the higher peaks bear witness to the unrelenting assault by
-the process of erosion upon the mountain citadels (figs. <a href="#fig4">4</a>
-and <a href="#fig31">31</a>).</p>
-<h3 id="c14">Rock disintegration and gravitational movement</h3>
-<p>A great variation in both daily and annual temperatures
-results in minute amounts of contraction and expansion
-<span class="pb" id="Page_25">25</span>
-of rock particles. Repeated changes in volume produce
-stress and strain. Although the rocks in the Tetons are very
-dense, they eventually yield; a crack forms. Water which
-seeps in along this surface of weakness freezes, either overnight
-or during long cold spells, and expands, thereby prying
-a slab of rock away from the mountain wall. Repeated
-<i>frost wedging</i>, as the process is called, results eventually
-in tipping the slab so that it falls.</p>
-<div class="img" id="fig4">
-<img src="images/p09.jpg" alt="" width="600" height="488" />
-<p class="pcap">Figure 4. <i>Talus at the foot of the jagged frost-riven peaks around Ice Floe
-Lake in the south fork of Cascade Canyon. Photo by Philip Hyde.</i></p>
-</div>
-<p>What happens to the rock slab? It may fall and roll
-several hundred or thousand feet, depending on the steepness
-of the mountain surface. Pieces are broken off as it
-encounters obstacles. All the fragments find their way to a
-valley floor or slope, where they momentarily come to rest.
-<span class="pb" id="Page_26">26</span>
-Thus, rock debris is moved significant and easily observed
-distances by gravity.</p>
-<p>None of this debris is stationary. If it is mixed with
-snow or saturated with water, the whole mass may slowly
-flow in the same manner as a glacier. These are called
-<i>rock glaciers</i>; some can be seen on the south side of
-Granite Canyon and one, nearly a mile long, is in the valley
-north of Eagles Rest Peak.</p>
-<p>The countless snow avalanches that thunder down the
-mountain flanks after heavy winter snowfalls play their
-part, too, in gravitational transport. Loose rocks and debris
-are incorporated with the moving snow and borne down the
-mountainsides to the talus piles below. Trees, bushes, and
-soil are swept from the sites of the slides, leaving conspicuous
-scars down the slopes and exposing new rock surfaces
-to the attack of water and frost. Battered, broken, and uprooted
-trees along many of the canyon trails bear silent witness
-to the awesome power of snowslides.</p>
-<p>These are some of the methods used by Nature in making
-debris and then, by means of gravity, clearing it from
-the mountain slopes. There are other ways, too. A weak
-layer of rock (usually one with a lot of clay in it), parallel
-to and underlying a mountain slope, may occur between
-two hard layers. An extended rainy spell may result in
-saturation of the weak zone so that it is well lubricated;
-then an earthquake or perhaps merely the weight of the
-overlying rock sends the now unstable mass cascading down
-the slope to the valley below. The famous Lower Gros Ventre
-Slide (<a href="#fig5">fig. 5</a>) was formed in this way on June 23, 1925.</p>
-<h3 id="c15">Running water cuts and carries</h3>
-<p>Running water is another effective agent that transports
-rock debris and has helped dissect the Teton Range.
-The damage a broken water main can wreak on a roadbed
-is well known, as is the havoc of destructive floods. The
-spring floods of streams in the Tetons, swollen by melting
-snow and ice (annual precipitation, mostly snow, in the
-high parts would average a layer of water 5 feet thick),
-move some rock debris onto the adjoining floor of Jackson
-Hole.</p>
-<div class="pb" id="Page_27">27</div>
-<div class="img" id="fig5">
-<img src="images/p10.jpg" alt="" width="600" height="485" />
-<p class="pcap">Figure 5. <i>The Lower Gros Ventre slide, air oblique view south. The top of
-the scar is 2,000 feet above the river; the slide is more than a mile long and
-one-half mile wide. It dammed the Gros Ventre River in the foreground,
-impounding a lake about 200 feet deep and 5 miles long. Gros Ventre
-Mountains are in the distance. Photo by P. E. Millward.</i></p>
-</div>
-<p>Now and then the range is deluged by summer cloudbursts.
-Water funnels down the maze of gullies on the
-mountainsides, quickly gathering volume and power, and
-plunges on to the talus slopes below, as if from gigantic
-hoses. The sudden onslaught of these torrents of water on
-the saturated unstable talus may trigger enormous rock and
-mudflows that carry vast quantities of material down into
-the canyons. During the summer of 1941 more than 100 of
-these flows occurred in the park.</p>
-<p>Wherever water moves, it carries rock fragments varying
-in size from boulders to sand grains and on down to
-minute clay particles. <i>Erosion</i> (wearing away) by streams
-<span class="pb" id="Page_28">28</span>
-is conspicuous wherever the water is muddy, as it always is
-each spring in the Snake, Buffalo Fork, and Gros Ventre
-Rivers. Clear mountain streams likewise can erode. Although
-the volume of material moved and the amount of
-downcutting of the stream bottom may not seem great in a
-single stream, the cumulative effect of many streams in an
-area, year after year and century after century, is enormous.
-Streams not only transport rocks brought to them by
-gravitational movement but also continually widen and
-deepen their valleys, thereby increasing the volume of
-transported debris.</p>
-<p>The effectiveness of streams as transporting agents in
-the Tetons is enhanced by steep <i>gradients</i> (slopes); these
-increase water velocity which in turn expands the capability
-of the streams to carry larger and larger rock fragments.</p>
-<h3 id="c16">Glaciers scour and transport</h3>
-<p>Mountain landscapes shaped by frost action, gravitational
-transport, and stream erosion alone generally have
-rounded summits, smooth slopes, and V-shaped valleys. The
-jagged ridges, sharply pointed peaks, and deep U-shaped
-valleys of the Tetons show that glaciers have played an
-important role in their sculpture. The small present-day
-glaciers still cradled in shaded recesses among the higher
-peaks (<a href="#fig6">fig. 6</a>) are but miniature replicas of great ice
-streams that occupied the region during the Ice Age. Evidence
-both here and in other parts of the world confirms
-that glaciers were once far more extensive than they are
-today.</p>
-<p>Glaciers form wherever more snow accumulates during
-the winter than is melted during the summer. Gradually
-the piles of snow solidify to form ice, which begins to flow
-under its own weight. Rocks that have fallen from the surrounding
-ridges or have been picked up from the underlying
-bedrock are incorporated in the moving ice mass and
-carried along. The ability of ice to transport huge volumes
-of rock is easily observed even in the small present-day
-glaciers in the Tetons, all of which carry abundant rock
-fragments both on and within the ice.</p>
-<div class="pb" id="Page_29">29</div>
-<div class="img" id="fig6">
-<img src="images/p11.jpg" alt="" width="600" height="797" />
-<p class="pcap">Figure 6. <i>The Teton Glacier on the north side of Grand Teton, air oblique view
-west. Photo by A. S. Post, August 19, 1963.</i></p>
-</div>
-<div class="pb" id="Page_30">30</div>
-<p>Recent measurements show that the ice in the present
-Teton Glacier (<a href="#fig6">fig. 6</a>) moves nearly 30 feet per year. The
-ancient glaciers, which were much wider and deeper, may
-have moved as much as several hundred feet a year, like
-some of the large glaciers in Alaska.</p>
-<p>As the glacier moves down a valley, it scours the valley
-bottom and walls. The efficiency of ice in this process
-is greatly increased by the presence of rock fragments
-which act as abrasives. The valley bottom is plowed, quarried,
-and swept clean of soil and loose rocks. Fragments of
-many sizes and shapes are dragged along the bottom of the
-moving ice and the hard ones scratch long parallel grooves
-in the underlying tough bedrock (<a href="#fig7">fig. 7</a>). Such grooves
-(<i>glacial striae</i>) record the direction of ice movement.</p>
-<p>The effectiveness of glaciers in cutting a U-shaped
-valley is particularly striking in Glacier Gulch and Cascade
-Canyon (figs. <a href="#fig2">2</a> and <a href="#fig8">8</a>).</p>
-<p>The rock-walled amphitheater at the head of a glaciated
-valley is called a <i>cirque</i> (a good example is at the upper
-edge of the Teton Glacier, <a href="#fig6">fig. 6</a>). The steep cirque walls
-develop by frost action and by quarrying and abrasive action
-of the glacier ice where it is near its maximum thickness.
-Commonly the glacier scoops out a shallow basin in
-the floor of the cirque. Amphitheater Lake, Lake Solitude,
-Holly Lake, and many of the other small lakes high in the
-Teton Range are located in such basins.</p>
-<p>The sharp peaks and the jagged knife-edge ridges so
-characteristic of the Tetons are divides left between cirques
-and valleys carved by the ancient glaciers.</p>
-<h3 id="c17">Effects on Jackson Hole</h3>
-<p>Rock debris is carried toward the end of the glacier or
-along the margins where it is released as the ice melts. The
-semicircular ridge of rock fragments that marks the downhill
-margin of the glacier is called a <i>terminal moraine</i>;
-that along the sides is a <i>lateral moraine</i> (figs. <a href="#fig9">9</a> and <a href="#fig10">10</a>).
-These are formed by the slow accumulation of material in
-the same manner as that at the end of a conveyor belt. They
-are not built by material pushed up ahead of the ice as if by
-a bulldozer. Large boulders carried by ice are called
-<i>erratics</i>; many of these are scattered on the floor of Jackson
-Hole and on the flanks of the surrounding mountains
-(<a href="#fig11">fig. 11</a>).</p>
-<div class="pb" id="Page_31">31</div>
-<div class="img" id="fig7">
-<img src="images/p12.jpg" alt="" width="600" height="362" />
-<p class="pcap">Figure 7. <i>Rock surface polished and grooved by ice on the floor of Glacier Gulch.</i></p>
-</div>
-<p>Great volumes of water pour from melting ice near the
-lower end of a glacier. These streams, heavily laden with
-rock flour produced by the grinding action of the glacier
-and with debris liberated from the melting ice, cut channels
-through the terminal moraine and spread a broad apron of
-gravel, sand, and silt down-valley from the glacier terminus
-(end). Material deposited by streams issuing from a glacier
-is called <i>outwash</i>; the sheet of outwash in front of the
-glacier is called an <i>outwash plain</i>. If the terminus is retreating,
-masses of old stagnant ice commonly are buried
-beneath the outwash; when these melt, the space they once
-occupied becomes a deep circular or irregular depression
-called a <i>kettle</i> (<a href="#fig12">fig. 12</a>); many of these now contain small
-lakes or swamps.</p>
-<p>As a glacier retreats, it may build a series of terminal
-moraines, marking pauses in the recession of the ice front.
-Streams issuing from the ice behind each new terminal
-moraine are incised more and more deeply into the older
-moraines and their outwash plains. Thus, new and younger
-layers of bouldery debris are spread at successively lower
-and lower levels. These surfaces are called <i>outwash
-terraces</i>.</p>
-<div class="pb" id="Page_32">32</div>
-<div class="img" id="fig8">
-<img src="images/p13.jpg" alt="" width="1000" height="641" />
-<p class="pcap">Figure 8. <i>East face of the Teton Range showing some of the glacial features, air oblique view.
-Cascade Canyon, the U-shaped valley, was cut by ice. The glacier flowed toward the flats,
-occupied the area of Jenny Lake (foreground), and left an encircling ring of morainal debris,
-now covered with trees. The flat bare outwash plain in foreground was deposited by meltwater
-from the glacier. The lake occupies a depression that was left when the ice melted away.
-National Park Service photo by Bryan Harry.</i></p>
-</div>
-<div class="pb" id="Page_33">33</div>
-<div class="img" id="fig9">
-<img src="images/p13a.jpg" alt="" width="600" height="337" />
-<p class="pcap">Figure 9. <i>Cutaway view of a typical valley glacier.</i></p>
-</div>
-<div class="img" id="fig10">
-<img src="images/p13b.jpg" alt="" width="600" height="393" />
-<p class="pcap">Figure 10. <i>Recently-built terminal moraine of the Schoolroom Glacier, a small ice mass near
-the head of the south fork of Cascade Canyon. The present glacier lies to the right just out
-of the field of view. The moraine marks a former position of the ice terminus; the lake
-(frozen over in this picture) occupies the depression left when the glacier wasted back from
-the moraine to its present position. Crest of the moraine stands about 50 feet above the lake
-level. Many of the lakes along the foot of the Teton Range occupy similar depressions
-behind older moraines. Photo by Philip Hyde.</i></p>
-</div>
-<div class="pb" id="Page_34">34</div>
-<div class="img" id="fig11">
-<img src="images/p14.jpg" alt="" width="600" height="436" />
-<p class="pcap">Figure 11. <i>Large ice-transported boulder of coarse-grained pegmatite and
-granite resting on Cretaceous shale near Mosquito Creek, on the southwest
-margin of Jackson Hole. Many boulders at this locality are composed of
-pegmatite rock characteristic of the middle part of the Teton Range. This
-occurrence demonstrates that boulders 40 feet in diameter were carried
-southward 25 miles and left along the west edge of the ice stream, 1,500 feet
-above the base of the glacier on the floor of Jackson Hole.</i></p>
-</div>
-<p>Just as the jagged ridges, U-shaped valleys, and ice-polished
-rocks of the Teton Range attest the importance of
-glaciers in carving the mountain landscape, the flat gravel
-outwash plains and hummocky moraines on the floor of
-Jackson Hole demonstrate their efficiency in transporting
-debris from the mountains and shaping the scenery of the
-valley.</p>
-<p>Glaciers sculptured all sides of Jackson Hole and
-filled it with ice to an elevation between 1,000 and 2,000
-<span class="pb" id="Page_35">35</span>
-feet above the present valley floor. The visitor who looks
-eastward from the south entrance to the park can see clearly
-glacial scour lines that superficially resemble a series of
-terraces on the bare lower slopes of the Gros Ventre Mountains.
-Southward-moving ice cut these features in hard
-rocks. Elsewhere around the margins of Jackson Hole,
-especially where the rocks are soft, evidence that the landscape
-was shaped by ice has been partly or completely obliterated
-by later events. Rising 1,000 feet above the floor of
-Jackson Hole are several steepsided buttes (figs. <a href="#fig13">13</a> and
-<a href="#fig55">55</a>) described previously, that represent &ldquo;islands&rdquo; of hard
-rock overridden and abraded by the ice. After the ice melted,
-these buttes were surrounded and partly buried by outwash
-debris.</p>
-<div class="img" id="fig12">
-<img src="images/p14a.jpg" alt="" width="600" height="401" />
-<p class="pcap">Figure 12. <i>&ldquo;The Potholes,&rdquo; knob and kettle topography caused by melting
-of stagnant ice partly buried by outwash gravel. Air oblique view north
-from over Burned Ridge moraine (see <a href="#fig61">fig. 61</a> for orientation). Photo by
-W. B. Hall and J. M. Hill.</i></p>
-</div>
-<p>The story of the glaciers and their place in the geologic
-history of the Teton region is discussed in more detail later
-in this booklet.</p>
-<div class="pb" id="Page_36">36</div>
-<div class="img" id="fig13">
-<img src="images/p15.jpg" alt="" width="1000" height="293" />
-<p class="pcap">Figure 13. <i>Radar image of part of Tetons and Jackson Hole. Distance shown
-between left and right margins is 35 miles. Lakes from left to right: Phelps,
-Taggart, Bradley, Jenny, Leigh, Jackson. Blacktail Butte is at lower left.
-Channel of Snake River and outwash terraces are at lower left. Burned
-Ridge and Jackson Lake moraines are in center. Lava flows at upper right
-engulf north end of Tetons. Striated surfaces at lower right are glacial scour
-lines made by ice moving south from Yellowstone National Park. Image
-courtesy of National Aeronautics and Space Administration.</i></p>
-</div>
-<h2 id="c18"><br /><span class="small">MOUNTAIN UPLIFT</span></h2>
-<p>Mountains appear ageless, but as with people, they
-pass through the stages of birth, youth, maturity, and old
-age, and eventually disappear. The Tetons are youthful
-and steep and are, therefore, extremely vulnerable to destructive
-processes that are constantly sculpturing the
-rugged features and carrying away the debris. The mountains
-are being destroyed. Although the processes of destruction
-may seem slow to us, we know they have been operating
-for millions of years&mdash;so why have the mountains not
-been leveled? How did they form in the first place?</p>
-<h3 id="c19">Kinds of mountains</h3>
-<p>There are many kinds of mountains. Some are piles of
-lava and debris erupted from a volcano. Others are formed
-by the bowing up of the earth&rsquo;s crust in the shape of a giant
-dome or elongated arch. Still others are remnants of accumulated
-<span class="pb" id="Page_37">37</span>
-sedimentary rocks that once filled a basin between
-preexisting mountains and which are now partially
-worn away. An example of this type is the Absaroka Range
-40 miles northeast of the Tetons (figs. <a href="#fig1">1</a> and <a href="#fig52">52</a>).</p>
-<p>The Tetons are a still different kind&mdash;a <i>fault block
-mountain range</i> carved from a segment of the earth&rsquo;s crust
-that has been uplifted along a fault. The <i>Teton fault</i> is
-approximately at the break in slope where the eastern foot
-of the range joins the flats at the west edge of Jackson Hole
-(see <a href="#fig62">map</a> inside back cover), but in most places is concealed
-beneath glacial deposits and debris shed from the
-adjacent steep slopes. The shape of the range and its relation
-to Jackson Hole have already been described. Clues as
-to the presence of the fault are: (1) the straight and deep
-east face of the Teton Range, (2) absence of foothills, (3)
-asymmetry of the range (<a href="#fig14">fig. 14</a>), and (4) small <i>fault
-scarps</i> (cliffs or steep slopes formed by faulting) along
-the mountain front (<a href="#fig15">fig. 15</a>).</p>
-<div class="pb" id="Page_38">38</div>
-<div class="img" id="fig14">
-<img src="images/p16.jpg" alt="" width="600" height="332" />
-<p class="pcap">Figure 14. <i>Air oblique view
-south showing the width and
-asymmetry of Teton Range.
-Grand Teton is left of center
-and Mt. Moran is the broad
-humpy peak still farther left.
-Photo taken October 1, 1965</i>.</p>
-</div>
-<p>Recent geophysical surveys of Jackson Hole combined
-with data from deep wells drilled in search of oil and gas
-east of the park also yield valuable clues. By measuring
-variations in the earth&rsquo;s magnetic field and in the pull of
-gravity and by studying the speed of shock waves generated
-by small dynamite explosions, Dr. John C. Behrendt of the
-U.&nbsp;S. Geological Survey has determined the depth and tilt
-of rock layers buried beneath the veneer of glacial debris
-and stream-laid sand and gravel on the valley floor. This
-information was used in constructing the geologic cross section
-in the back of the booklet. The same rock layers that
-cap the summit of Mount Moran (<a href="#fig27">fig. 27</a>) are buried at
-depths of nearly 24,000 feet beneath the nearby floor of
-Jackson Hole but are cut off by the Teton fault at the west
-edge of the valley. Thus the approximate amount of movement
-along the fault here would be about 30,000 feet.</p>
-<h3 id="c20">Anatomy of faults</h3>
-<p>The preceding discussion shows that the Tetons are an
-upfaulted mountain block. Why is this significant? The
-extreme youth of the Teton fault, its large amount of displacement,
-and the fact that the newly upfaulted angular
-mountain block was subjected to intense glaciation are
-among the prime factors responsible for the development of
-the magnificent alpine scenery of the Teton Range. An understanding
-<span class="pb" id="Page_39">39</span>
-of the anatomy of faults is, therefore, pertinent.</p>
-<div class="img" id="fig15">
-<img src="images/p16a.jpg" alt="" width="600" height="494" />
-<p class="pcap">Figure 15. <i>Recent fault scarp
-(arrows indicate base)
-offsetting alluvial fan at foot
-of Rockchuck Peak. View
-west from Cathedral Group
-scenic turnout. National Park
-Service photo by W. E. Dilley
-and R. A. Mebane.</i></p>
-</div>
-<p>A fault is a plane or zone in the earth&rsquo;s crust along
-which the rocks on one side have moved in relation to the
-rocks on the other. There are various kinds of faults just as
-there are various types of mountains. Three principal types
-of faults are present in the Teton region: normal faults,
-reverse faults, and thrust faults. A <i>normal fault</i> (<a href="#fig16A">fig. 16A</a>)
-is a steeply <i>dipping</i> (steeply inclined) fault along
-which rocks above the fault have moved <i>down</i> relative to
-those beneath it. A <i>reverse fault</i> (<a href="#fig16B">fig. 16B</a>) is a steeply
-inclined fault along which the rocks above the fault have
-moved <i>up</i> relative to those below it. A <i>thrust fault</i> (<a href="#fig16C">fig. 16C</a>)
-is a gently inclined fault along which the principal
-movement has been more nearly horizontal than vertical.</p>
-<p>Normal faults may be the result of tension or pulling
-apart of the earth&rsquo;s crust or they may be caused by adjustment
-of the rigid crust to the flow of semi-fluid material below.
-The crust sags or collapses in areas from which the
-subcrustal material has flowed and is bowed up and
-stretched in areas where excess subcrustal material has
-accumulated. In both areas the adjustments may result in
-normal faults.</p>
-<p>Reverse faults are generally caused by compression of
-a rigid block of the crust, but some may also be due to lateral
-flow of subcrustal material.</p>
-<div class="pb" id="Page_40">40</div>
-<p>Thrust faults are commonly associated with tightly
-bent or folded rocks. Many of them are apparently caused
-by severe compression of part of the crust, but some are
-thought to have formed at the base of slides of large rock
-masses that moved from high areas into adjacent low areas
-under the influence of gravity.</p>
-<p>The Teton fault (see <a href="#pic2">cross section</a> inside back cover)
-is a normal fault; the Buck Mountain fault, which lies west
-of the main peaks of the Teton Range, is a reverse fault. No
-thrust faults have been recognized in the Teton Range, but
-the mountains south and southwest of the Tetons (<a href="#fig1">fig. 1</a>)
-display several enormous thrust faults along which masses
-of rocks many miles in extent have moved tens of miles eastward
-and northeastward.</p>
-<h3 id="c21">Time and rate of uplift</h3>
-<p>When did the Tetons rise?</p>
-<p>A study of the youngest sedimentary rocks on the floor
-of Jackson Hole shows that the Teton Range began to rise
-rapidly and take its present shape less than 9 million years
-ago. The towering peaks themselves are direct evidence that
-the rate of uplift far exceeded the rate at which the rising
-block was worn away by erosion. The mountains are still
-rising, and comparatively rapidly, as is indicated by small
-faults cutting the youngest deposits (<a href="#fig15">fig. 15</a>).</p>
-<p>How rapidly? Can the rate be measured?</p>
-<p>We know that in less than 9 million years (and probably
-in less than 7 million years) there has been 25,000 to
-30,000 feet of displacement on the Teton fault. This is an
-average of about 1 foot in 300-400 years. The movement
-probably was not continuous but came as a series of jerks
-accompanied by violent earthquakes. One fault on the floor
-of Jackson Hole near the southern boundary of the park
-moved 150 feet in the last 15,000 years, an average of 1
-foot per 100 years.</p>
-<p>In view of this evidence of recent crustal unrest, it is
-not surprising that small earthquakes are frequent in the
-Teton region. More violent ones can probably be expected
-from time to time.</p>
-<div class="pb" id="Page_41">41</div>
-<div class="img" id="fig16">
-<p class="pcap">Figure 16. <i>Types of faults.</i></p>
-</div>
-<div class="img" id="fig16A">
-<img src="images/p17.jpg" alt="" width="262" height="173" />
-<p class="pcap">A.&mdash;Normal fault (tensional)</p>
-</div>
-<div class="img" id="fig16B">
-<img src="images/p17a.jpg" alt="" width="276" height="173" />
-<p class="pcap">B.&mdash;Reverse fault (compressional)</p>
-</div>
-<div class="img" id="fig16C">
-<img src="images/p17b.jpg" alt="" width="303" height="164" />
-<p class="pcap">C.&mdash;Thrust fault (compressional)</p>
-</div>
-<h3 id="c22">Why are mountains here?</h3>
-<p>Why did the Tetons form where they are?</p>
-<p>At the beginning of this booklet we discussed briefly
-the two most common theories of origin of mountains: continental
-drift and convection currents. The question of why
-mountains are where they are and more specifically why
-the Tetons are here remains a continuing scientific challenge
-regardless of the wealth of data already accumulated
-in our storehouse of knowledge.</p>
-<p>The mobility of the earth&rsquo;s crust is an established fact.
-Despite its apparent rigidity, laboratory experiments demonstrate
-that rocks flow when subjected to extremely high
-pressures and temperatures. If the stress exceeds the
-strength at a given pressure and temperature, the rock
-breaks. Flowing and fracturing are two of the ways by
-which rocks adjust to the changing environments at various
-levels in the earth&rsquo;s crust. These acquired characteristics,
-some of which can be duplicated in the laboratory, are
-guides by which we interpret the geologic history of rocks
-that once were deep within the earth.</p>
-<div class="pb" id="Page_42">42</div>
-<p>The site of the Teton block no doubt reflects hidden inequalities
-at depth. We cannot see these, nor in this area
-can we drill below the outer layer of the earth; nevertheless,
-measurements of gravity and of the earth&rsquo;s magnetic
-field clearly show that they exist.</p>
-<p>We know that the Tetons rose at the time Jackson Hole
-collapsed but the volume of the uplifted block is considerably
-less than that of the downdropped block. This, then,
-was not just a simple case in which all the subcrustal material
-displaced by the sinking block was squeezed under
-the rising block (the way a hydraulic jack works). What
-happened to the rest of the material that once was under
-Jackson Hole? It could not be compressed so it had to go
-somewhere.</p>
-<p>As you look northward from the top of the Grand Teton
-or Mount Moran, or from the main highway at the north
-edge of Grand Teton National Park, you see the great
-smooth sweep of the volcanic plateau in Yellowstone National
-Park. Farther off to the northeast are the strikingly
-layered volcanic rocks of the Absaroka Range (<a href="#fig52">fig. 52</a>).
-For these two areas, an estimate of the volume of volcanic
-rock that reached the surface and flowed out, or was blown
-out and spread far and wide by wind and water, is considerably
-in excess of 10,000 cubic miles. On the other hand,
-this volume is many times more than that displaced by the
-sagging and downfaulting of Jackson Hole.</p>
-<p>Where did the rest of the volcanic material come
-from? Is it pertinent to our story? Teton Basin, on the west
-side of the Teton Range, and the broad Snake River downwarp
-farther to the northwest (<a href="#fig1">fig. 1</a>) are sufficiently large
-to have furnished the remainder of the volcanic debris. As
-it was blown out of vents in the Yellowstone-Absaroka area,
-its place could have been taken deep underground by material
-that moved laterally from below all three downdropped
-areas. The movement may have been caused by
-slow convection currents within the earth, or perhaps by
-some other, as yet unknown, force. The sagging of the
-earth&rsquo;s crust on both sides of the Teton Range as well as the
-long-continued volcanism are certainly directly related to
-the geologic history of the park.</p>
-<div class="pb" id="Page_43">43</div>
-<p>In summary, we theorize as to how the Tetons rose and
-Jackson Hole sank but are not sure why the range is located
-at this particular place, why it trends north, why it rose so
-high, or why this one, of all the mountain ranges surrounding
-the Yellowstone-Absaroka volcanic area, had such a
-unique history of uplift. These are problems to challenge
-the minds of generations of earth scientists yet to come.</p>
-<h3 id="c23">The restless land</h3>
-<p>Among the greatest of the park&rsquo;s many attractions is
-the solitude one can savor in the midst of magnificent scenery.
-Only a short walk separates us from the highway,
-torrents of cars, noise, and tension. Away from these,
-everything seems restful.</p>
-<p>Quiescent it may seem, yet the landscape is not static
-but dynamic. This is one of the many exciting ideas that
-geology has contributed to society. The concept of the
-&ldquo;everlasting hills&rdquo; is a myth. All the features around us are
-actually rather short-lived in terms of geologic time. The
-discerning eye detects again and again the restlessness of
-the land. We have discussed many bits of evidence that
-show how the landscape and the earth&rsquo;s crust beneath it are
-constantly being carved, pushed up, dropped down, folded,
-tilted, and faulted.</p>
-<p>The Teton landscape is a battleground, the scene of a
-continuing unresolved struggle between the forces that deform
-the earth&rsquo;s crust and raise the mountains and the slow
-processes of erosion that strive to level the uplands, fill the
-hollows, and reduce the landscape to an ultimate featureless
-plain. The remainder of this booklet is devoted to tracing
-the seesaw conflict between these inexorable antagonists
-through more than 2.5 billion years as they shaped the present
-landscape&mdash;and the battle still goes on.</p>
-<p>Evidence of the struggle is all around us. Even though
-to some observers it may detract from the restfulness of the
-scene, perhaps it conveys to all of us a new appreciation of
-the tremendous dynamic forces responsible for the magnificence
-of the Teton Range.</p>
-<p>The battle is indicated by the small faults that displace
-both the land surface and young deposits at the east base of
-<span class="pb" id="Page_44">44</span>
-Mount Teewinot, Rockchuck Peak (<a href="#fig15">fig. 15</a>), and other
-places along the foot of the Tetons.</p>
-<p>Jackson Hole continues to drop and tilt. The gravel-covered
-surfaces that originally sloped southward are now
-tilted westward toward the mountains. The Snake River,
-although the major stream, is not in the lowest part of Jackson
-Hole; Fish Creek, a lesser tributary near the town of
-Wilson, is 15 feet lower. For 10 miles this creek flows
-southward parallel to the Snake River but with a gentler
-gradient, thus permitting the two streams to join near the
-south end of Jackson Hole. As tilting continues, the Snake
-River west of Jackson tries to move westward but is prevented
-from doing so by long flood-control levees built
-south of the park.</p>
-<p>Recent faults also break the valley floor between the
-Gros Ventre River and the town of Jackson.</p>
-<p>The ever-changing piles of rock debris that mantle the
-slopes adjacent to the higher peaks, the creeping advance of
-rock glaciers, the devastating snow avalanches, and the
-thundering rockfalls are specific reminders that the land
-surface is restless. Jackson Hole contains more landslides
-and rock mudflows than almost any other part of the
-Rocky Mountain region. They constantly plague road
-builders (<a href="#fig17">fig. 17</a>) and add to the cost of other types of
-construction.</p>
-<p>All of these examples of the relentless battle between
-constructive and destructive processes modifying the Teton
-landscape are but minor skirmishes. The bending and
-breaking of rocks at the surface are small reflections of
-enormous stresses and strains deep within the earth where
-the major conflict is being waged. It is revealed every now
-and then by a convulsion such as the 1959 earthquake in
-and west of Yellowstone Park. Events of this type release
-much more energy than all the nuclear devices thus far
-exploded by man.</p>
-<div class="pb" id="Page_45">45</div>
-<div class="img" id="fig17">
-<img src="images/p18.jpg" alt="" width="600" height="394" />
-<p class="pcap">Figure 17. <i>Slide blocking main highway in northern part of Grand Teton
-National Park. National Park Service photo by Eliot Davis, May 1952.</i></p>
-</div>
-<h2 id="c24"><br /><span class="small">ENORMOUS TIME AND DYNAMIC EARTH</span></h2>
-<h3 id="c25">Framework of time</h3>
-<p>One of geology&rsquo;s greatest philosophical contributions
-has been the demonstration of the enormity of geologic
-time. Astronomers deal with distances so great that they are
-almost beyond understanding; nuclear physicists study objects
-so small that we can hardly imagine them. Similarly,
-the geologist is concerned with spans of time so immense
-that they are scarcely comprehensible. Geology is a science
-of time as well as rocks, and in our geologic story of the
-Teton region we must refer frequently to the geologic time
-scale, the yardstick by which we measure the vast reaches
-of time in earth history.</p>
-<h3 id="c26">Rocks and relative age</h3>
-<p>Very early in the science of geology it was recognized
-that in many places one can tell the comparative ages of
-rocks by their relations to one another. For example, most
-<i>sedimentary rocks</i> are consolidated accumulations of large
-or small rock fragments and were deposited as nearly horizontal
-<span class="pb" id="Page_46">46</span>
-layers of gravel, sand, or mud. In an undisturbed
-sequence of sedimentary rocks, the layer on the bottom was
-deposited first and the layer on top was deposited last. All
-of these must, of course, be younger than any previously
-formed rock fragments incorporated in them.</p>
-<p><i>Igneous rocks</i> are those formed by solidification of
-molten material, either as lava flows on the earth&rsquo;s surface
-(<i>extrusive igneous rocks</i>) or at depth within the earth
-(<i>intrusive igneous rocks</i>). The relative ages of extrusive
-igneous rocks can often be determined in much the same
-way as those of sedimentary strata. A lava flow is younger
-than the rocks on which it rests, but older than those that
-rest on top of it.</p>
-<p>An intrusive igneous rock must be younger than the
-rocks that enclosed it at the time it solidified. It may contain
-pieces of the enclosing rocks that broke off the walls
-and fell into the liquid. Pebbles of the igneous rock that
-are incorporated in nearby sedimentary layers indicate
-that the sediments must be somewhat younger.</p>
-<p>All of these criteria tell us only that one rock is older
-or younger than another. They tell us little about the absolute
-age of the rocks or about how much older one is than
-the other.</p>
-<h3 id="c27">Fossils and geologic time</h3>
-<p>Fossils provide important clues to the ages of the rocks
-in which they are found. The slow evolution of living things
-through geologic time can be traced by a systematic study
-of fossils. The fossils are then used to determine the relative
-ages of the rocks that contain them and to establish a
-geologic time scale that can be applied to fossil-bearing
-rocks throughout the world. <a href="#fig18">Figure 18</a> shows the major
-subdivisions of the last 600 million years of geologic time
-and some forms of life that dominated the scene during
-each of these intervals. Strata containing closely related
-fossils are grouped into <i>systems</i>; the time interval during
-which the strata comprising a particular system were deposited
-is termed a <i>period</i>. The periods are subdivisions of
-larger time units called <i>eras</i> and some are split into smaller
-time units called <i>epochs</i>. Strata deposited during an epoch
-<span class="pb" id="Page_47">47</span>
-comprise a <i>series</i>. Series are in turn subdivided into rock
-units called <i>groups</i> and formations. Expressed in tabular
-form these divisions are:</p>
-<table class="center" summary="">
-<tr class="th"><th>Subdivisions of geologic time </th><th class="l">Time-rock units </th><th class="l">Rock units</th></tr>
-<tr><td class="l">Era</td></tr>
-<tr><td class="l"><span class="hst">Period</span> </td><td class="l">System</td></tr>
-<tr><td class="l"><span class="hst2">Epoch</span> </td><td class="l"><span class="hst">Series</span></td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Group</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l"><span class="hst">Formation</span></td></tr>
-</table>
-<p>The time scale based on the study of fossil-bearing
-sedimentary rocks is called the stratigraphic time scale; it
-is given in <a href="#table1">table 1</a>. The subdivisions are arranged in the
-same order in which they were deposited, with the oldest at
-the bottom and the youngest at the top. All rocks older than
-Cambrian (the first period in the Paleozoic Era) are
-classed as Precambrian. These rocks are so old that fossils
-are rare and therefore cannot be conveniently used as a
-basis for subdivision.</p>
-<p>The stratigraphic time scale is extremely useful, but it
-has serious drawbacks. It can be applied only to fossil-bearing
-strata or to rocks whose ages are determined by
-their relation to those containing fossils. It cannot be used
-directly for rocks that lack fossils, such as igneous rocks,
-or metamorphic rocks in which fossils have been destroyed
-by heat or pressure. It is used to establish the relative ages
-of sedimentary strata throughout the world, but it gives no
-information as to how long ago a particular layer was
-deposited or how many years a given period or era lasted.</p>
-<h3 id="c28">Radioactive clocks</h3>
-<p>The measurement of geologic time in terms of years
-was not possible until the discovery of natural radioactivity.
-It was found that certain atoms of a few elements spontaneously
-throw off particles from their nuclei and break
-down to form atoms of other elements. These decay processes
-take place at constant rates, unaffected by heat, pressure,
-or chemical conditions. If we know the rate at which
-a particular radioactive element decays, the length of time
-that has passed since a mineral crystal containing the elements
-formed can be calculated by comparing the amount
-of the radioactive element remaining in the crystal with the
-amount of disintegration products present.</p>
-<div class="pb" id="Page_48">48</div>
-<div class="img" id="fig18">
-<img src="images/p19.jpg" alt="" width="700" height="440" />
-<p class="pcap">Figure 18. <i>Major subdivisions of the last 600 million years of geologic time
-and some of the dominant forms of life.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>MILLIONS OF YEARS AGO</th></tr>
-<tr><td class="r">0 </td><td class="l"> </td><td class="l"> </td><td class="l">Man</td></tr>
-<tr><td class="r">0-60 </td><td class="l">CENOZOIC </td><td class="l">QUATERNARY and TERTIARY </td><td class="l">Mammals</td></tr>
-<tr><td class="r">60-130 </td><td class="l">MESOZOIC </td><td class="l">CRETACEOUS</td></tr>
-<tr><td class="r">130-180 </td><td class="l"> </td><td class="l">JURASSIC </td><td class="l">Dinosaurs</td></tr>
-<tr><td class="r">180-220 </td><td class="l"> </td><td class="l">TRIASSIC</td></tr>
-<tr><td class="r">220-260 </td><td class="l">PALEOZOIC </td><td class="l">PERMIAN </td><td class="l">Reptiles</td></tr>
-<tr><td class="r">260-350 </td><td class="l"> </td><td class="l">PENNSYLVANIAN, MISSISSIPPIAN </td><td class="l">Amphibians</td></tr>
-<tr><td class="r">350-400 </td><td class="l"> </td><td class="l">DEVONIAN </td><td class="l">Fishes</td></tr>
-<tr><td class="r">400-440 </td><td class="l"> </td><td class="l">SILURIAN </td><td class="l">Sea scorpions</td></tr>
-<tr><td class="r">440-500 </td><td class="l"> </td><td class="l">ORDOVICIAN </td><td class="l">Nautiloids</td></tr>
-<tr><td class="r">500-530 </td><td class="l"> </td><td class="l">CAMBRIAN </td><td class="l">Trilobites</td></tr>
-<tr><td class="r">530- </td><td class="l">PRECAMBRIAN </td><td class="l"> </td><td class="l">Soft-bodied creatures</td></tr>
-</table>
-<p>Three principal radioactive clocks now in use are
-based on the decay of uranium to lead, rubidium to strontium,
-and potassium to argon. They are effective in dating
-minerals millions or billions of years old. Another clock,
-based on the decay of one type of carbon (<i>Carbon-14</i>) to
-nitrogen, dates organic material, but only if it is less than
-about 40,000 years old.</p>
-<p>The uranium, rubidium, and potassium clocks are
-especially useful in dating igneous rocks. By determining
-the absolute ages of igneous rocks whose stratigraphic relations
-to fossil-bearing strata are known, it is possible to
-estimate the number of years represented by the various
-subdivisions of the stratigraphic time scale.</p>
-<h3 id="c29">The yardstick of geologic time</h3>
-<p>Recent estimates suggest that the earth was formed at
-least 4.5 billion years ago. To visualize the length of geologic
-time and the relations between the stratigraphic and
-absolute time scales, let us imagine a yardstick as representing
-the length of time from the origin of the earth to the
-present (<a href="#fig19">fig. 19</a>). On one side of the yardstick we plot time
-<span class="pb" id="Page_49">49</span>
-in years; on the other, we plot the divisions of the stratigraphic
-time scale according to the most reliable absolute
-age determinations.</p>
-<div class="img" id="table1">
-<img src="images/p19a.jpg" alt="" width="600" height="583" />
-<p class="pcap"><span class="ss">Table 1. The stratigraphic time scale.</span></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>Era </th><th class="l">System or period </th><th class="l">Series or epoch</th></tr>
-<tr><td class="l">Cenozoic </td><td class="l">Quaternary </td><td class="l">Recent</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Pleistocene</td></tr>
-<tr><td class="l"> </td><td class="l">Tertiary </td><td class="l">Pliocene</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Miocene</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Oligocene</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Eocene</td></tr>
-<tr><td class="l"> </td><td class="l"> </td><td class="l">Paleocene</td></tr>
-<tr><td class="l">Mesozoic </td><td class="l">Cretaceous</td></tr>
-<tr><td class="l"> </td><td class="l">Jurassic</td></tr>
-<tr><td class="l"> </td><td class="l">Triassic</td></tr>
-<tr><td class="l">Paleozoic </td><td class="l">Permian</td></tr>
-<tr><td class="l"> </td><td class="l">Pennsylvanian</td></tr>
-<tr><td class="l"> </td><td class="l">Mississippian</td></tr>
-<tr><td class="l"> </td><td class="l">Devonian</td></tr>
-<tr><td class="l"> </td><td class="l">Silurian<a class="fn" id="fr_1" href="#fn_1">[1]</a></td></tr>
-<tr><td class="l"> </td><td class="l">Ordovician</td></tr>
-<tr><td class="l"> </td><td class="l">Cambrian</td></tr>
-<tr><td class="l">&mdash; </td><td class="l">Precambrian</td></tr>
-</table>
-<div class="fnblock"><div class="fndef"><a class="fn"  id="fn_1" href="#fr_1">[1]</a><i>The Silurian is the only major subdivision of the stratigraphic time scale not represented in Grand Teton National Park.</i>
-</div>
-</div>
-<p>We are immediately struck by the fact that all of the
-subdivisions of the stratigraphic time scale since the beginning
-of the Paleozoic are compressed into the last 5 inches
-of our yardstick! All of the other 31 inches represent Precambrian
-time. We also see that subdivisions of the stratigraphic
-time scale do not represent equal numbers of years.
-We use smaller and smaller subdivisions as we approach
-the present. (Notice the subdivisions of the Tertiary and
-Quaternary in <a href="#table1">table 1</a> that are too small to show even in the
-enlarged part of <a href="#fig19">figure 19</a>). This is because the record of
-earth history is more vague and incomplete the farther back
-in time we go. In effect, we are very nearsighted in our
-view of time. This &ldquo;geological myopia&rdquo; becomes increasingly
-evident throughout the remainder of this booklet.</p>
-<div class="pb" id="Page_50">50</div>
-<div class="img" id="fig19">
-<img src="images/p20.jpg" alt="" width="634" height="600" />
-<p class="pcap">Figure 19. <i>The geologic time scale&mdash;our yardstick in time.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>ABSOLUTE TIME (Years ago) </th><th class="r">INCHES </th><th class="l">STRATIGRAPHIC TIME SCALE</th></tr>
-<tr><td class="r">First man &rarr; </td><td class="r">0 </td><td class="l">CENOZOIC</td></tr>
-<tr><td class="r"> </td><td class="r">1 </td><td class="l">MESOZOIC</td></tr>
-<tr><td class="r">First dinosaurs &rarr; </td><td class="r">2 </td><td class="l">PALEOZOIC</td></tr>
-<tr><td class="r"> </td><td class="r">3</td></tr>
-<tr><td class="r">500 million </td><td class="r">4</td></tr>
-<tr><td class="r">First abundant fossils &rarr; </td><td class="r">5 </td><td class="l">PRECAMBRIAN</td></tr>
-<tr><td class="r"> </td><td class="r">6</td></tr>
-<tr><td class="r"> </td><td class="r">7</td></tr>
-<tr><td class="r">1 billion </td><td class="r">8</td></tr>
-<tr><td class="r"> </td><td class="r">9</td></tr>
-<tr><td class="r"> </td><td class="r">10</td></tr>
-<tr><td class="r"> </td><td class="r">11</td></tr>
-<tr><td class="r"> </td><td class="r">12</td></tr>
-<tr><td class="r"> </td><td class="r">13</td></tr>
-<tr><td class="r"> </td><td class="r">14</td></tr>
-<tr><td class="r">Oldest known fossils &rarr; </td><td class="r">15</td></tr>
-<tr><td class="r">2 billion </td><td class="r">16</td></tr>
-<tr><td class="r"> </td><td class="r">17</td></tr>
-<tr><td class="r"> </td><td class="r">18</td></tr>
-<tr><td class="r"> </td><td class="r">19</td></tr>
-<tr><td class="r"> </td><td class="r">20</td></tr>
-<tr><td class="r"> </td><td class="r">21</td></tr>
-<tr><td class="r"> </td><td class="r">22</td></tr>
-<tr><td class="r"> </td><td class="r">23</td></tr>
-<tr><td class="r">3 billion </td><td class="r">24</td></tr>
-<tr><td class="r"> </td><td class="r">25</td></tr>
-<tr><td class="r"> </td><td class="r">26</td></tr>
-<tr><td class="r"> </td><td class="r">27</td></tr>
-<tr><td class="r">Oldest dated rocks &rarr; </td><td class="r">28</td></tr>
-<tr><td class="r"> </td><td class="r">29</td></tr>
-<tr><td class="r"> </td><td class="r">30</td></tr>
-<tr><td class="r"> </td><td class="r">31</td></tr>
-<tr><td class="r">4 billion </td><td class="r">32</td></tr>
-<tr><td class="r"> </td><td class="r">33</td></tr>
-<tr><td class="r"> </td><td class="r">34</td></tr>
-<tr><td class="r"> </td><td class="r">35</td></tr>
-<tr><td class="r">Minimum age of the earth &rarr; </td><td class="r">36</td></tr>
-</table>
-<table class="center" summary="">
-<tr class="th"><th class="r"> </th><th colspan="4">ENLARGEMENT OF THE LAST SIX INCHES</th></tr>
-<tr class="th"><th>ABSOLUTE TIME (Years Ago) </th><th class="c">INCHES </th><th colspan="2">STRATIGRAPHIC TIME SCALE</th></tr>
-<tr><td class="r">0 </td><td class="c">0 </td><td class="l">CENOZOIC </td><td class="l">QUATERNARY</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">TERTIARY</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l">MESOZOIC </td><td class="l">CRETACEOUS</td></tr>
-<tr><td class="r"> </td><td class="c">1 </td><td class="l"> </td><td class="l">JURASSIC</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">TRIASSIC</td></tr>
-<tr><td class="r"> </td><td class="c">2 </td><td class="l">PALEOZOIC </td><td class="l">PERMIAN</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">PENNSYLVANIAN</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">MISSISSIPPIAN</td></tr>
-<tr><td class="r"> </td><td class="c">3 </td><td class="l"> </td><td class="l">DEVONIAN</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">SILURIAN</td></tr>
-<tr><td class="r"> </td><td class="c"> </td><td class="l"> </td><td class="l">ORDOVICIAN</td></tr>
-<tr><td class="r"> 500 million </td><td class="c">4 </td><td class="l">CAMBRIAN</td></tr>
-<tr><td class="r"> </td><td class="c">5 </td><td class="l">PRECAMBRIAN</td></tr>
-<tr><td class="r"> </td><td class="c">6</td></tr>
-</table>
-<div class="pb" id="Page_51">51</div>
-<h2 id="c30"><br /><span class="small">PRECAMBRIAN ROCKS&mdash;THE CORE OF THE TETONS</span></h2>
-<p>The visitor who looks at the high, rugged peaks of the
-Teton Range is seeing rocks that record about seven-eighths
-of all geologic time. These Precambrian rocks are part of
-the very foundation of the continent and are therefore commonly
-referred to by geologists as basement rocks. In attempting
-to decipher their origin and history we peer backward
-through the dim mists of time, piecing together
-scattered clues to events that occurred billions of years ago,
-perhaps during the very birth of the North American Continent.
-To cite an oft-quoted example, it is as though we
-were attempting to read the history of an ancient and long-forgotten
-civilization from the scattered unnumbered pages
-of a torn manuscript, written in a language that we only
-partially understand.</p>
-<h3 id="c31">Ancient gneisses and schists</h3>
-<p>The oldest Precambrian rocks in the Teton Range are
-layered gneisses and schists exposed over wide areas in the
-northern and southern parts of the range and as scattered
-isolated masses in the younger granite that forms the high
-peaks in the central parts. The layered gneisses may be
-seen easily along the trails in the lower parts of Indian
-Paintbrush and Death Canyons, and near Static Peak.</p>
-<p>The <i>layered gneisses</i> are composed principally of
-quartz, feldspar, <i>biotite</i> (black mica), and <i>hornblende</i>
-(a very dark-green or black mineral commonly forming
-rodlike crystals). Distinct layers, a few inches to several
-feet thick, contain different proportions of these minerals
-and account for the banded appearance. Layers composed
-almost entirely of quartz and feldspar are light-gray or
-white, whereas darker gray layers contain higher proportions
-of biotite and hornblende.</p>
-<p>Some layers are dark-green to black <i>amphibolite</i>,
-composed principally of hornblende but with a little feldspar
-and quartz. In many places the gneisses include layers
-of <i>schist</i>, a flaky rock, much of which is mica. At several
-places on the east slopes of Mount Moran thin layers
-<span class="pb" id="Page_52">52</span>
-of impure gray marble are found interleaved with the
-gneisses. West of Static Peak along the Alaska Basin Trail
-a heavy dark rock with large amounts of <i>magnetite</i> (strongly
-magnetic black iron oxide) occurs as layers in the gneiss.</p>
-<p>In some places the gneiss contains dark-reddish crystals
-of garnet as much as an inch in diameter. Commonly
-the garnet crystals are surrounded by white &ldquo;halos&rdquo; which
-lack biotite or hornblende, probably because the constituents
-necessary to form these minerals were absorbed by the
-garnet crystals. In Death Canyon and on the slopes of
-Static Peak some layers of gray gneiss contain egg-shaped
-masses of magnetite as much as one-half inch in diameter
-(<a href="#fig20">fig. 20</a>). These masses are likewise surrounded by elliptical
-white halos and have the startling appearance of small
-eyes peering from the rock. Appropriately, this rock has
-been called the &ldquo;bright-eyed&rdquo; gneiss by Prof. Charles C.
-Bradley in his published study (Wyoming Geological Association,
-1956) of this area.</p>
-<p>What were the ancient rocks from which the gneisses
-of the Teton Range were formed? Most of the evidence has
-been obliterated but a few remaining clues enable us to
-draw some general conclusions. The banded appearance of
-many of the gneisses suggests that they were formed from
-sedimentary and volcanic rocks that accumulated on the sea
-floor near a chain of volcanic islands&mdash;perhaps somewhat
-similar to the modern Aleutians or the islands of Indonesia.
-When these deposits were buried deep in the earth&rsquo;s crust
-the chemical composition of some layers may have undergone
-radical changes. Other layers, however, still have
-compositions resembling those of younger rocks elsewhere
-whose origins are better known. For example, the layers
-of impure marble were probably once beds of sandy limestone,
-and the lighter colored gneiss may have been muddy
-sandstone, possibly containing volcanic ash. Some dark
-amphibolite layers could represent altered lava flows or
-beds of volcanic ash; others may have resulted from the addition
-of silica to muddy magnesium-rich limestone during
-metamorphism. The magnetite-rich gneiss probably was
-originally a sedimentary iron ore.</p>
-<div class="pb" id="Page_53">53</div>
-<div class="img" id="fig20">
-<img src="images/p21.jpg" alt="" width="600" height="439" />
-<p class="pcap">Figure 20. <i>&ldquo;Bright-eyed&rdquo;
-gneiss from Death Canyon.
-The dark magnetite spots are
-about &frac14; inch in diameter.
-The surrounding gneiss is
-composed of quartz, feldspar,
-and biotite, but biotite is
-missing in the white halos
-around the magnetite.</i></p>
-</div>
-<p>Minerals that were most easily altered at depth reacted
-with one another to form new minerals more &ldquo;at home&rdquo;
-under the high temperature and pressure in this environment
-just as the ingredients in a cake react when heated in
-an oven. Rocks formed by such processes are called <i>metamorphic
-rocks</i>; careful studies of the minerals that they contain
-suggest that the layered gneisses developed at temperatures
-as high as 1000&deg;F at depths of 5 to 10 miles. Under
-these conditions the rocks must have behaved somewhat like
-soft taffy as is shown by layers that have been folded
-nearly double without being broken (<a href="#fig21">fig. 21</a>). Folds such
-as these range from fractions of an inch to thousands of feet
-across and are found in gneisses throughout the Teton
-Range. In a few places folds are superimposed in such a
-way as to indicate that the rocks were involved in several
-episodes of deformation in response to different sets of
-stress during metamorphism.</p>
-<p>When did these gneisses form? Age determinations of
-minerals containing radioactive elements show that granite
-which was intruded into them after they were metamorphosed
-and folded is more than 2.5 billion years old. They
-must, therefore, be older than that. Thus, they probably
-are at least a billion years older than rocks containing the
-first faint traces of life on earth and 2 billion years older
-than the oldest rocks containing abundant fossils. How
-much older is not known, but the gneisses are certainly
-<span class="pb" id="Page_54">54</span>
-among the oldest rocks in North America and record some
-of the earliest events in the building of this continent.</p>
-<div class="img" id="fig21">
-<p class="pcap">Figure 21. <i>Folds in layered gneisses.</i></p>
-</div>
-<div class="img" id="fig21A">
-<img src="images/p22.jpg" alt="" width="600" height="411" />
-<p class="pcap">A. <i>North
-face of the ridge west of Eagles Rest Peak. The face
-is about 700 feet high. Notice the extreme contortion
-of the gneiss layers.</i></p>
-</div>
-<div class="img" id="fig21B">
-<img src="images/p22a.jpg" alt="" width="600" height="479" />
-<p class="pcap">B. <i>Closeup
-view of some of the folds near the bottom of the
-face in figure A. The light-colored layers are composed
-principally of quartz and feldspar. The
-darker layers are rich in hornblende.</i></p>
-</div>
-<p>Irregular bodies of granite gneiss are interleaved with
-the layered gneisses in the northern part of the Teton
-Range. The <i>granite gneiss</i> is relatively coarse grained,
-streaky gray or pink, and composed principally of quartz,
-feldspar, biotite, and hornblende. It differs from enclosing
-layered gneisses in its coarser texture, lack of layering, and
-more uniform appearance. The dark minerals (biotite and
-<span class="pb" id="Page_55">55</span>
-hornblende) are concentrated in thin discontinuous wisps
-that give the rock its streaky appearance.</p>
-<p>The largest body of granite gneiss is exposed in a belt
-1 to 2 miles wide and 10 miles long extending northeastward
-from near the head of Moran Canyon, across the upper
-part of Moose Basin, and into the lower reaches of
-Webb Canyon. This gneiss may have been formed from
-granite that invaded the ancient sedimentary and volcanic
-rocks before they were metamorphosed, or it may have been
-formed during metamorphism from some of the sediments
-and volcanics themselves.</p>
-<p>At several places in Snowshoe, Waterfalls, and Colter
-Canyons the layered gneisses contain discontinuous masses
-a few tens or hundreds of feet in diameter of heavy dark-green
-or black <i>serpentine</i>. This rock is frequently called
-&ldquo;<i>soapstone</i>&rdquo; because the surface feels smooth and soapy to
-the touch. Indians carved bowls (<a href="#fig22">fig. 22</a>) from similar material
-obtained from the west side of the Tetons and from
-the Gros Ventre Mountains to the southeast. Pebbles of serpentine
-along streams draining the west side of the Tetons
-have been cut and polished for jewelry and sold as &ldquo;<i>Teton
-jade</i>&rdquo;; it is much softer and less lustrous than real jade.
-The serpentine was formed by metamorphism of dark-colored
-igneous rocks lacking quartz and feldspar.</p>
-<h3 id="c32">Granite and pegmatite</h3>
-<p>Contrary to popular belief, <i>granite</i> (crystalline igneous
-rock composed principally of quartz and feldspar)
-forms only a part of the Teton Range. The Grand Teton
-(<a href="#fig6">fig. 6</a>) and most surrounding subsidiary peaks are sculptured
-from an irregular mass of granite exposed continuously
-along the backbone of the range from Buck Mountain
-northward toward upper Leigh Canyon. The rock is commonly
-fine grained, white or light-gray, and is largely composed
-of crystals of gray quartz and white feldspar about
-the size and texture of the grains in very coarse lump sugar.
-Flakes of black or dark-brown mica (biotite) and silvery
-white mica (<i>muscovite</i>) about the size of grains of pepper
-are scattered through the rock.</p>
-<p>From the floor of Jackson Hole the granite cliffs and
-<span class="pb" id="Page_56">56</span>
-buttresses of the high peaks appear nearly white in contrast
-to the more somber grays and browns of surrounding gneisses
-and schists. These dark rocks are laced by a network of
-irregular light-colored granite dikes ranging in thickness
-from fractions of an inch to tens of feet (<a href="#fig23">fig. 23</a>).</p>
-<div class="img" id="fig22">
-<img src="images/p23.jpg" alt="" width="600" height="280" />
-<p class="pcap">Figure 22. <i>Indian bowls carved from
-soapstone, probably from the Teton
-Range. Mouth of the unbroken bowl is
-about 4 inches in diameter.</i></p>
-</div>
-<p>The largest masses of granite contain abundant unoriented
-angular blocks and slabs of the older gneisses. These
-inclusions range from a few inches in diameter (<a href="#fig24">fig. 24</a>) to
-slabs hundreds of feet thick and thousands of feet long.</p>
-<p>Dikes or irregular intrusions of pegmatite are found
-in almost every exposure of granite. <i>Pegmatite</i> contains
-the same minerals as granite but the individual mineral
-crystals are several inches or even as much as a foot in
-diameter.</p>
-<p>Some pegmatites contain silvery plates or tabular crystals
-of muscovite mica as much as 6 inches across that can
-be split into transparent sheets with a pocket knife. Others
-have dark-brown biotite mica in crystals about the size and
-shape of the blade of a table knife.</p>
-<p>A few pegmatites contain scattered red-brown crystals
-of garnet ranging in size from that of a BB shot to a small
-marble; a few in Garnet Canyon and Glacier Gulch are
-larger than baseballs (<a href="#fig25">fig. 25</a>). The garnets are fractured
-and many are partly altered to <i>chlorite</i> (a dull-green micaceous
-mineral) so they are of no value as gems.</p>
-<div class="pb" id="Page_57">57</div>
-<div class="img" id="fig23">
-<p class="pcap">Figure 23. <i>Dikes of granite and pegmatite.</i></p>
-</div>
-<div class="img" id="fig23A">
-<img src="images/p23a.jpg" alt="" width="399" height="601" />
-<p class="pcap">A. <i>Network of light-colored granite
-dikes on the northeast face of the West
-Horn on Mt. Moran. The dikes cut
-through gneiss in which the layers slant
-steeply downward to the left. The face
-is about 700 feet high. Snowfield in the
-foreground is at the edge of the Falling
-Ice Glacier.</i></p>
-</div>
-<div class="img" id="fig23B">
-<img src="images/p23b.jpg" alt="" width="409" height="600" />
-<p class="pcap">B. <i>Irregular dike of granite and
-pegmatite cutting through dark layered
-gneisses near Wilderness Falls in
-Waterfalls Canyon. The cliff face is
-about 80 feet high. Contacts of the dike
-are sharp and angular and cut across
-the layers in the enclosing gneiss.</i></p>
-</div>
-<div class="pb" id="Page_58">58</div>
-<p>Pegmatite <i>dikes</i> (tabular bodies of rock that, while
-still molten, were forced along fractures in older rocks)
-commonly cut across granite dikes, but in many places the
-reverse is true. Some dikes are composed of layers of pegmatite
-alternating with layers of granite (<a href="#fig26">fig. 26</a>), showing
-that the pegmatite and granite are nearly contemporaneous.
-Prof. Bruno Giletti and his coworkers at Brown University,
-using the rubidium-strontium radioactive clock, determined
-that the granite and pegmatite in the Teton Range are about
-2.5 billion years old.</p>
-<div class="img" id="fig24">
-<img src="images/p24.jpg" alt="" width="600" height="424" />
-<p class="pcap">Figure 24. <i>Angular blocks of old streaky granite gneiss in fine-grained
-granite northwest of Lake Solitude. The difference in orientation of the
-streaks in the gneiss blocks indicates that the blocks have been rotated with
-respect to one another and that the fine-grained granite must therefore have
-been liquid at the time of intrusion. A small light-colored dike in the upper
-left-hand block of gneiss ends at the edge of the block; it intruded the gneiss
-before the block was broken off and incorporated in the granite. A small
-dike of pegmatite cuts diagonally through the granite just to the left of the
-hammer and extends into the blocks of gneiss at both ends. This dike was
-intruded after the granite had solidified. Thus, in this one small exposure we
-can recognize four ages of rocks: the streaky granite gneiss, the light-colored
-dike, the fine-grained granite, and the small pegmatite dike.</i></p>
-</div>
-<h3 id="c33">Black dikes</h3>
-<p>Even the most casual visitor to the Teton Range notices
-the remarkable black band that extends down the east face
-<span class="pb" id="Page_59">59</span>
-of Mount Moran (figs. <a href="#fig27">27</a> and <a href="#fig28">28</a>) from the summit and
-disappears into the trees north of Leigh Lake. This is the
-outcropping edge of a steeply inclined dike composed of
-<i>diabase</i>, a nearly black igneous rock very similar to basalt.
-Thinner diabase dikes are visible on the east face of Middle
-Teton, on the south side of the Grand Teton, and in several
-other places in the range (see <a href="#fig62">geologic map</a> inside back cover).</p>
-<div class="img" id="fig25">
-<img src="images/p24a.jpg" alt="" width="600" height="436" />
-<p class="pcap">Figure 25. <i>Garnet crystal in pegmatite. The crystal is about 6 inches in
-diameter. Other minerals are feldspar (white) and clusters of white mica
-flakes. The mica crystals appear dark in the photograph because they are
-wet.</i></p>
-</div>
-<p>The diabase is a heavy dark-greenish-gray to black
-rock that turns rust brown on faces that have been exposed
-to the weather. It is studded with small lath-shaped crystals
-of feldspar that are greenish gray in the fresh rock and
-milk white on weathered surfaces.</p>
-<p>The black dikes formed from molten rock that welled
-up into nearly vertical fissures in the older Precambrian
-<span class="pb" id="Page_60">60</span>
-rocks. Toward the edges of the dikes the feldspar laths in
-the diabase become smaller and smaller (<a href="#fig29">fig. 29</a>), indicating
-that the wall rocks were relatively cool when the
-<i>magma</i> or melted rock was intruded. Rapid chilling at the
-edges prevented growth of large crystals. In many places
-hot solutions from the dike permeated the wall rocks, staining
-them rosy red.</p>
-<div class="img" id="fig26">
-<img src="images/p25.jpg" alt="" width="600" height="397" />
-<p class="pcap">Figure 26. <i>A small dike of pegmatite and granite cutting through folded
-layered gneiss in Death Canyon. Coarse-grained pegmatite forms most of
-the dike, but fine-grained granite is found near the center. Small offshoots
-of the dike penetrate into the wall rocks. The dike cuts straight across folds
-in the enclosing gneisses and must therefore have been intruded after
-development of the folds. The white ruler is about 6 inches long.</i></p>
-</div>
-<p>The black dike on Mount Moran is about 150 feet thick
-near the summit of the peak. This dike has been traced
-westward for more than 7 miles. Where it passes out of the
-park south of Green Lakes Mountain it is 100 feet thick.
-The amount of molten material needed to form the exposed
-segment of this single dike could fill Jenny Lake three
-times over. The other dikes are thinner and not as long: the
-dike on Middle Teton is 20 to 40 feet thick, and the dike on
-Grand Teton is 40 to 60 feet thick.</p>
-<div class="pb" id="Page_61">61</div>
-<div class="img" id="fig27">
-<img src="images/p25a.jpg" alt="" width="800" height="638" />
-<p class="pcap">Figure 27. <i>Air oblique view of the east face of
-Mt. Moran, showing the great black dike. Main
-mass of the mountain is layered gneiss and
-streaky granite gneiss. White lines are dikes of
-granite and pegmatite; light-gray mound on the
-summit is about 50 feet of Cambrian sedimentary
-rock (Flathead Sandstone). Notice that
-the black dike cuts across the dikes of
-granite and pegmatite but that its upper edge is
-covered by the much younger layer of
-sandstone. Falling Ice Glacier is in the left
-center; Skillet Glacier is in the lower right center.
-Photo by A. S. Post. University of Washington, August 19, 1963.</i></p>
-</div>
-<div class="pb" id="Page_62">62</div>
-<div class="img" id="fig28">
-<img src="images/p26.jpg" alt="" width="600" height="742" />
-<p class="pcap">Figure 28. <i>The great black dike on the east face of Mt. Moran. The dike is
-about 150 feet thick and its vertical extent in the picture is about 3,000 feet.
-The fractures in the dike perpendicular to its walls are cracks formed as the
-liquified rock cooled and crystallized. Falling Ice Glacier is in the center.
-National Park Service photo by H. D. Pownall.</i></p>
-</div>
-<div class="pb" id="Page_63">63</div>
-<div class="img" id="fig29">
-<img src="images/p26a.jpg" alt="" width="600" height="419" />
-<p class="pcap">Figure 29. <i>Closeup view of the edge of the
-Middle Teton black dike exposed on the north
-wall of Garnet Canyon near the west end of the trail. Dike rock (diabase) is on the
-right; wall rock (gneiss) is on the left. Match shows scale.</i></p>
-</div>
-<p>The black dikes must be the youngest of the Precambrian
-units because they cut across all other Precambrian
-rocks. The dikes must have been intruded before the beginning
-of Cambrian deposition inasmuch as they do not cut
-the oldest Cambrian beds. Gneiss adjacent to the dike on
-Mount Moran contains biotite that was heated and altered
-about 1.3 billion years ago according to Professor Giletti.
-The alteration is believed to have occurred when the dike
-was emplaced; therefore this and similar dikes elsewhere
-in the range are probably about 1.3 billion years old.</p>
-<h3 id="c34">Quartzite</h3>
-<p>At about the same time as the dikes were being intruded
-in the Tetons, many thousands of feet of sedimentary
-rocks, chiefly sandstone, were deposited in western Montana,
-200 miles northwest of Grand Teton National Park.
-The sandstone was later recrystallized and recemented and
-became a very dense hard rock called <i>quartzite</i>. Similar
-quartzite, possibly part of the same deposit, was laid down
-west of the north end of the Teton Range, within the area
-now called the Snake River downwarp (<a href="#fig1">fig. 1</a>).</p>
-<p>The visitor who hikes or camps anywhere on the floor
-of Jackson Hole becomes painfully aware of the thousands
-upon thousands of remarkably rounded hard quartzite
-boulders. He wonders where they came from because nowhere
-in the adjacent mountains is this rock type exposed.
-The answer is that the quartzites were derived from a long-vanished
-<span class="pb" id="Page_64">64</span>
-uplift (figs. <a href="#fig42">42</a> and <a href="#fig46">46</a>), carried eastward by
-powerful rivers past the north end of the Teton Range, and
-then were deposited in a vast sheet of gravel that covered
-much of Jackson Hole 60 to 80 million years ago. Since
-then, these virtually indestructible boulders have been re-worked
-many times by streams and ice, yet still retain the
-characteristics of the original ancient sediments.</p>
-<h3 id="c35">A backward glance</h3>
-<p>So far we have seen that the Precambrian basement
-exposed in the Teton Range contains a complex array of
-rocks of diverse origins and various ages. Before passing
-on to the younger rocks, reference to our yardstick may
-help to place the Precambrian events in their proper
-perspective.</p>
-<p>In all of Precambrian time, which encompasses more
-than 85 percent of the history of the earth (31 of the 36
-inches of our yardstick), only two events are dated in the
-Teton Range: the intrusion of granite and pegmatite about
-2.5 billion years ago, and the emplacement of the black
-dikes about 1.3 billion years ago. These dates are indicated
-by heavy arrows on the time scale (<a href="#fig30">fig. 30</a>). The ancient
-gneisses and schists were formed sometime before 2.5 billion
-years ago, and probably are no older than 3.5 billion
-years, the age of the oldest rocks dated anywhere in the
-world.</p>
-<h3 id="c36">The close of the Precambrian&mdash;end of the beginning</h3>
-<p>More than 700 million years elapsed between intrusion
-of the black dikes and deposition of the first Paleozic
-sedimentary rocks&mdash;a longer period of time than has
-elapsed since the beginning of the Paleozic Era. During
-this enormous interval the Precambrian rocks were uplifted,
-exposed to erosion, and gradually worn to a nearly
-featureless plain, perhaps somewhat resembling the vast
-flat areas in which similar Precambrian rocks are now exposed
-in central and eastern Canada. At the close of Precambrian
-time, about 600 million years ago, the plain slowly
-floundered and the site of the future Teton Range disappeared
-beneath shallow seas that were to wash across it intermittently
-for the next 500 million years. It is to the
-sediments deposited in these seas that we turn to read the
-next chapter in the geologic story of the Teton Range.</p>
-<div class="pb" id="Page_65">65</div>
-<div class="img" id="fig30">
-<img src="images/p27.jpg" alt="" width="451" height="800" />
-<p class="pcap">Figure 30. <i>A glance at the yardstick.
-The geologic time scale shows positions
-of principal events recorded in the
-Precambrian rocks of the Tetons.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th class="r">ABSOLUTE TIME (Years ago) </th><th>INCHES</th></tr>
-<tr><td class="r">Beginning of the Paleozoic. First abundant fossils &rarr; </td><td class="c">4</td></tr>
-<tr><td class="r">1 billion </td><td class="c">8</td></tr>
-<tr><td class="r">Maximum age of black dikes &rarr; </td><td class="c">10</td></tr>
-<tr><td class="r">Oldest known fossils </td><td class="c">15</td></tr>
-<tr><td class="r">2 billion </td><td class="c">16</td></tr>
-<tr><td class="r">Old granite and pegmatite </td><td class="c">20</td></tr>
-<tr><td class="r">3 billion </td><td class="c">24</td></tr>
-<tr><td class="r">Gneisses and schists formed sometime in this interval </td><td class="c">20-27</td></tr>
-<tr><td class="r">Oldest dated rocks &rarr; </td><td class="c">28</td></tr>
-<tr><td class="r">4 billion &rarr; </td><td class="c">32</td></tr>
-<tr><td class="r">Minimum age of the earth </td><td class="c">36</td></tr>
-</table>
-<div class="pb" id="Page_66">66</div>
-<h2 id="c37"><br /><span class="small">THE PALEOZOIC ERA&mdash;TIME OF LONG-VANISHED SEAS AND THE DEVELOPMENT OF LIFE</span></h2>
-<h3 id="c38">The Paleozoic sequence</h3>
-<p>North, west, and south of the highest Teton peaks the
-soaring spires and knife-edge ridges of Precambrian rock
-give way to rounded spurs and lower flat-topped summits,
-whose slopes are palisaded by continuous gray cliffs that
-resemble the battlements of some ancient and long-abandoned
-fortress (<a href="#fig31">fig. 31</a>). As mentioned previously, the
-cliffs are the projecting edges of layers of sedimentary
-rocks of Paleozoic age that accumulated in or along the
-margins of shallow seas. At one time the layers formed a
-thick unbroken, nearly horizontal blanket across the Precambrian
-basement rocks, but subsequent uplift of the eastern
-edge of the Teton fault block tilted them westward.
-They were then stripped from the highest peaks.</p>
-<p>The Paleozoic and younger sedimentary rocks in the
-Teton region are subdivided into <i>formations</i>, each of which
-is named. A formation is composed of rock layers which,
-because of their similar physical characteristics, can be distinguished
-from overlying and underlying layers. They
-must be thick enough to be shown on a geologic map. <a href="#table2">Table 2</a>
-lists the various Paleozoic formations present in and adjacent
-to Grand Teton National Park and gives their thicknesses
-and characteristics. These sedimentary rocks are of
-special interest, for they not only record an important
-chapter of geologic history but elsewhere in the region they
-contain petroleum and other mineral deposits.</p>
-<p>The Paleozoic rocks can be viewed close at hand from
-the top of the Teton Village tram (<a href="#fig32">fig. 32</a>) on the south
-boundary of the park. A less accessible but equally spectacular
-exposure of Paleozoic rocks is in Alaska Basin,
-along the west margin of the park, where they are stacked
-like even layers in a gigantic cake (<a href="#fig33">fig. 33</a>).</p>
-<h3 id="c39">Alaska Basin&mdash;site of an outstanding rock and fossil record</h3>
-<p>Strata in Alaska Basin record with unusual clarity the
-opening chapters in the chronicle of seas that flowed and
-<span class="pb" id="Page_67">67</span>
-ebbed across the future site of the Teton Range during most
-of the Paleozoic Era. In the various rock layers are inscribed
-stories of the slow advance and retreat of ancient
-shorelines, of the storm waves breaking on long-vanished
-beaches, and of the slow and intricate evolution of the myriads
-of sea creatures that inhabited these restless waters.</p>
-<div class="img" id="fig31">
-<img src="images/p28.jpg" alt="" width="600" height="451" />
-<p class="pcap">Figure 31. <i>Paleozoic rocks on the west flank of the Teton Range, air oblique
-view west. Ragged peaks in the foreground (Buck Mountain on the left
-center, Mt. Wister, with top outlined by snow patch on the extreme right),
-are carved in Precambrian rocks. Banded cliffs in the background are
-sedimentary rocks. Alaska Basin is at upper right. Teton Basin, a broad,
-extensively farmed valley in eastern Idaho, is at top. Photo by A. S. Post,
-University of Washington, 1963.</i></p>
-</div>
-<p>Careful study of the fossils allows us to determine the
-age of each formation (<a href="#table3">table 3</a>). Even more revealing, the
-fossils themselves are tangible evidence of the orderly parade
-of life that crossed the Teton landscape during more
-than 250 million years. Here is a record of Nature&rsquo;s experiments
-with life, the triumphs, failures, the bizarre, the
-beautiful.</p>
-<div class="pb" id="Page_68">68</div>
-<div class="img" id="table2">
-<img src="images/p29.jpg" alt="" width="895" height="600" />
-<p class="pcap"><span class="ss">Table 2.&mdash;Paleozoic sedimentary rocks exposed in the Teton region.</span></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>Age </th><th class="l">Formation </th><th class="l">Thickness (feet) </th><th class="l">Description </th><th class="l">Where exposed</th></tr>
-<tr><td class="l">Permian </td><td class="l">Phosphoria Formation </td><td class="l">150-250 </td><td class="l">Dolomite, gray, cherty, sandy, black shale and phosphate beds; marine. </td><td class="l">North and west flanks of Teton Range, north flank of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td class="l">Pennsylvanian </td><td class="l">Tensleep and Amsden Formations </td><td class="l">600-1,500 </td><td class="l">Tensleep Sandstone, light-gray, hard, underlain by Amsden Formation, a domolite and red shale with a basal red sandstone; marine. </td><td class="l">North and west flanks of Teton Range, north flank of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td class="l">Mississippian </td><td class="l">Madison Limestone </td><td class="l">1,000-1,200 </td><td class="l">Limestone, blue-gray, hard, fossiliferous; thin red shale in places near top; marine. </td><td class="l">North and west flanks of Teton Range, north flank of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td class="l">Devonian </td><td class="l">Darby Formation </td><td class="l">200-500 </td><td class="l">Dolomite, dark-gray to brown, fetid, hard, and brown, black, and yellow shale; marine. </td><td class="l">North and west flanks of Teton Range, north flank of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td class="l">Ordovician </td><td class="l">Bighorn Dolomite </td><td class="l">300-500 </td><td class="l">Dolomite, light-gray, siliceous, very hard; white dense very fine-grained dolomite at top; marine. </td><td class="l">North and west flanks of Teton Range, north and west flanks of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td class="l">Cambrian </td><td class="l">Gallatin Limestone </td><td class="l">180-300 </td><td class="l">Limestone, blue gray, hard, thin-bedded; marine. </td><td class="l">North and west flanks of Teton Range and Gros Ventre Mountains.</td></tr>
-<tr><td class="l"> </td><td class="l">Gros Ventre Formation </td><td class="l">600-800 </td><td class="l">Shale, green, flaky, with Death Canyon Limestone Member composed of about 300 feet of hard cliff-forming limestone in middle; marine. </td><td class="l">North and west flanks of Teton Range and Gros Ventre Mountains.</td></tr>
-<tr><td class="l"> </td><td class="l">Flathead Sandstone </td><td class="l">175-200 </td><td class="l">Sandstone, reddish-brown, very hard, brittle; partly marine. </td><td class="l">North and west flanks of Teton Range and Gros Ventre Mountains.</td></tr>
-</table>
-<p>The regularity and parallel relations of the layers in
-well-exposed sections such as the one in Alaska Basin suggest
-that all these rocks were deposited in a single uninterrupted
-sequence. However, the fossils and regional distribution
-of the rock units show that this is not really the
-case. The incomplete nature of this record becomes apparent
-if we plot the ages of the various formations on the
-absolute geologic time scale (<a href="#fig34">fig. 34</a>). The length of time
-from the beginning of the Cambrian Period to the end of
-the Mississippian Period is about 285 million years. The
-strata in Alaska Basin are a record of approximately 120
-million years. More than half of the pages in the geologic
-story are missing even though, compared with most other
-areas, the book as a whole is remarkably complete! During
-these unrecorded intervals of time either no sediments were
-<span class="pb" id="Page_69">69</span>
-deposited in the area of the Teton Range or, if deposited,
-they were removed by erosion.</p>
-<div class="img" id="fig32">
-<img src="images/p29a.jpg" alt="" width="600" height="374" />
-<p class="pcap">Figure 32. <i>Paleozoic marine sedimentary rocks near south boundary of
-Grand Teton National Park. View is south from top of Teton Village tram.
-National Park Service photo by W. E. Dilley and R. A. Mebane.</i></p>
-</div>
-<dl class="undent"><dt><span class="ss">Madison Limestone</span></dt>
-<dt><span class="ss">Darby Formation</span></dt>
-<dt><span class="ss">Bighorn Dolomite</span></dt>
-<dt><span class="ss">Gallatin Limestone</span></dt></dl>
-<h3 id="c40">Advance and retreat of Cambrian seas: an example</h3>
-<p>The first invasion and retreat of the Paleozoic sea are
-sketched on <a href="#fig35">figure 35</a>. Early in Cambrian time a shallow
-seaway, called the <i>Cordilleran trough</i>, extended from
-southern California northeastward across Nevada into Utah
-and Idaho (<a href="#fig35A">fig. 35A</a>). The vast gently rolling plain on Precambrian
-rocks to the east was drained by sluggish westward-flowing
-rivers that carried sand and mud into the sea.
-Slow subsidence of the land caused the sea to spread gradually
-eastward. Sand accumulated along the beaches just
-as it does today. As the sea moved still farther east, mud
-was deposited on the now-submerged beach sand. In the
-Teton area, the oldest sand deposit is called the Flathead
-Sandstone (<a href="#fig36">fig. 36</a>).</p>
-<p>The mud laid down on top of the Flathead Sandstone
-as the shoreline advanced eastward across the Teton area is
-now called the Wolsey Shale Member of the Gros Ventre
-<span class="pb" id="Page_70">70</span>
-Formation. Some shale shows patterns of cracks that
-formed when the accumulating mud was briefly exposed to
-the air along tidal flats. Small phosphatic-shelled animals
-called <i>brachiopods</i> inhabited these lonely tidal flats (fig.
-<a href="#fig37A">37A</a> and <a href="#fig37B">37B</a>) but as far as is known, nothing lived on land.
-Many shale beds are marked with faint trails and borings
-of wormlike creatures, and a few contain the remains of
-tiny very intricately developed creatures with head, eyes,
-segmented body, and tail. These are known as trilobites
-(fig. <a href="#fig37C">37C</a> and <a href="#fig37D">37D</a>). Descendants of these lived in various
-seas that crossed the site of the dormant Teton Range for
-the next 250 million years.</p>
-<div class="img" id="fig33">
-<img src="images/p30.jpg" alt="" width="600" height="365" />
-<p class="pcap">Figure 33. <i>View southwest across Alaska Basin, showing tilted layers of
-Paleozoic sedimentary rocks on the west flank of the Teton Range. National
-Park Service photo.</i></p>
-</div>
-<dl class="undent"><dt><span class="ss">Mount Meek</span></dt>
-<dt><span class="ss">Madison Limestone</span></dt>
-<dt><span class="ss">Bighorn Dolomite</span></dt>
-<dt><span class="ss">Death Canyon Limestone Member</span></dt>
-<dt><span class="ss">Flathead Sandstone</span></dt>
-<dt><span class="ss">Precambrian Rock</span></dt></dl>
-<p>As the shoreline moved eastward, the Death Canyon
-Limestone Member of the Gros Ventre Formation (<a href="#fig33">fig. 33</a>)
-was deposited in clear water farther from shore. Following
-this the sea retreated to the west for a short time. In the
-shallow muddy water resulting from this retreat the Park
-Shale Member of the Gros Ventre Formation was deposited.
-In places underwater &ldquo;meadows&rdquo; of algae flourished on the
-sea bottom and built extensive reefs (<a href="#fig38A">fig. 38A</a>). From time
-to time shoal areas were hit by violent storm waves that tore
-loose platy fragments of recently solidified limestone and
-swept them into nearby channels where they were buried
-and cemented into thin beds of jumbled fragments (<a href="#fig38B">fig. 38B</a>)
-called <i>&ldquo;edgewise&rdquo; conglomerate</i>. These are widespread
-in the shale and in overlying and underlying limestones.</p>
-<div class="pb" id="Page_71">71</div>
-<div class="img" id="table3">
-<img src="images/p30a.jpg" alt="" width="600" height="565" />
-<p class="pcap">Table 3. <i>Formations exposed in Alaska Basin.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>AGE (Numbers show age in millions of years) </th><th colspan="2">FORMATION (Thickness) </th><th class="l">ROCKS AND FOSSILS</th></tr>
-<tr><td class="c">(310)</td></tr>
-<tr><td class="c"> MISSISSIPPIAN </td><td colspan="2" class="l">MADISON LIMESTONE (Total about 1,100 feet, but only lower 300 feet preserved in this section) </td><td class="l">Uniform thin beds of blue-gray limestone and sparse very thin layers of shale. Brachiopods, corals, and other fossils abundant.</td></tr>
-<tr><td class="c">(345)</td></tr>
-<tr><td class="c">LATE AND MIDDLE DEVONIAN </td><td colspan="2" class="l">DARBY FORMATION (About 350 feet) </td><td class="l">Thin beds of gray and buff dolomite interbedded with layers of gray, yellow, and black shale. A few fossil brachiopods, corals, and bryozoans.</td></tr>
-<tr><td class="c">(390)</td></tr>
-<tr><td class="c">(425)</td></tr>
-<tr><td class="c">LATE AND MIDDLE ORDOVICIAN </td><td colspan="2" class="l">BIGHORN DOLOMITE (About 450 feet; Leigh Dolomite Member about 40 feet thick at top) </td><td class="l">Thick to very thin beds of blue-gray or brown dolomite, white on weathered surfaces. A few broken fossil brachiopods, bryozoans, and horn corals. Thin beds of white fine-grained dolomite at top are the Leigh Member.</td></tr>
-<tr><td class="c">(440)</td></tr>
-<tr><td class="c">(500)</td></tr>
-<tr><td class="c">LATE CAMBRIAN </td><td colspan="2" class="l">GALLATIN LIMESTONE (180 feet) </td><td class="l">Blue-gray limestone mottled with irregular rusty or yellow patches. Trilobites and brachiopods.</td></tr>
-<tr><td class="c">(530)</td></tr>
-<tr><td class="c">MIDDLE CAMBRIAN </td><td colspan="2" class="l">GROS VENTRE FORMATION</td></tr>
-<tr><td class="c"> </td><td class="lt"> </td><td class="l">PARK SHALE MEMBER (220 feet) </td><td class="l">Gray-green shale containing beds of platy limestone conglomerate. Trilobites, brachiopods, and fossil algal heads.</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l">DEATH CANYON LIMESTONE MEMBER (285 feet) </td><td class="l">Two thick beds of dark-blue-gray limestone separated by 15 to 20 feet of shale that locally contains abundant fossil brachiopods and trilobites.</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l">WOLSEY SHALE MEMBER (100 feet) </td><td class="l">Soft greenish-gray shale containing beds of purple and green sandstone near base. A few fossil brachiopods.</td></tr>
-<tr><td class="c"> </td><td colspan="2" class="l">FLATHEAD LIMESTONE (175 feet) </td><td class="l">Brown, maroon, and white sandstone, locally containing many rounded pebbles of quartz and feldspar. Some beds of green shale at top.</td></tr>
-<tr><td class="c">(570)</td></tr>
-<tr><td class="c">PRECAMBRIAN </td><td class="l"> </td><td class="l"> </td><td class="l">Granite, gneiss, and pegmatite.</td></tr>
-</table>
-<div class="img" id="fig34">
-<img src="images/p30b.jpg" alt="" width="600" height="450" />
-<p class="pcap">Figure 34. <i>Absolute ages of the formations in Alaska Basin. Shaded parts of the scale show intervals for which there is no record.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th colspan="3">STRATIGRAPHIC SCALE </th><th class="l">ABSOLUTE TIME (Years ago) </th><th class="l">ENLARGED PIECE OF YARDSTICK SHOWN ON <a href="#fig19">FIGURE 19</a></th></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l"> </td><td>2</td></tr>
-<tr><td class="c">PALEZOIC </td><td class="l">PENNSYLVANIAN </td><td class="l">?</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l">300 million</td></tr>
-<tr><td class="c"> </td><td class="l">MISSISSIPPIAN </td><td class="l">MADISON</td></tr>
-<tr><td class="c"> </td><td class="l">DEVONIAN </td><td class="l">DARBY</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l"> </td><td>3</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l">400 million</td></tr>
-<tr><td class="c"> </td><td class="l">SILURIAN</td></tr>
-<tr><td class="c"> </td><td class="l">ORDOVICIAN </td><td class="l">BIGHORN</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l">500 million </td><td>4</td></tr>
-<tr><td class="c"> </td><td class="l">CAMBRIAN </td><td class="l">GALLATIN</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l">GROS VENTRE</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l">FLATHEAD</td></tr>
-<tr><td class="c"> </td><td class="l"> </td><td class="l"> </td><td class="l">600 million</td></tr>
-<tr><td class="c">PRECAMBRIAN </td><td class="l"> </td><td class="l"> </td><td class="l"> </td><td>5</td></tr>
-</table>
-<div class="pb" id="Page_72">72</div>
-<div class="img" id="fig35">
-<p class="pcap">Figure 35. <i>The first invasions of the Paleozoic sea.</i></p>
-</div>
-<div class="img" id="fig35A">
-<img src="images/p31.jpg" alt="" width="417" height="278" />
-<p class="pcap">A. <i>In Early Cambrian
-time an arm of the Pacific Ocean occupied a deep
-trough in Idaho, Nevada, and part of Utah. The
-land to the east was a broad gently rolling plain
-of Precambrian rocks drained by sluggish westward-flowing
-streams. The site of the Teton Range was part of this plain. Slow
-subsidence of the land caused the sea to move eastward during Middle
-Cambrian time flooding the Precambrian plain.</i></p>
-</div>
-<div class="img" id="fig35B">
-<img src="images/p31b.jpg" alt="" width="429" height="277" />
-<p class="pcap">B. <i>By Late Cambrian time the sea had drowned all of Montana
-and most of Wyoming. The Flathead Sandstone
-and Gros Ventre Formation were deposited as the sea
-advanced. The Gallatin Limestone was being deposited when
-the shoreline was in about the position shown in this drawing.</i></p>
-</div>
-<div class="img" id="fig35C">
-<img src="images/p31c.jpg" alt="" width="422" height="276" />
-<p class="pcap">C. <i>In Early Ordovician time uplift of
-the land caused the sea to retreat back into the trough,
-exposing the Cambrian deposits to erosion. Cambrian deposits were
-partly stripped off of some areas. The Bighorn Dolomite was deposited
-during the next advance of the sea in Middle and Late Ordovician time.</i></p>
-</div>
-<div class="pb" id="Page_73">73</div>
-<div class="img" id="fig36">
-<img src="images/p31f.jpg" alt="" width="600" height="427" />
-<p class="pcap">Figure 36. <i>Conglomeratic basal bed of Flathead Sandstone and underlying
-Precambrian granite gneiss; contact is indicated by a dark horizontal line
-about 1 foot below hammer. This contact is all that is left to mark a 2-billion
-year gap in the rock record of earth history. The locality is on the
-crest of the Teton Range 1 mile northwest of Lake Solitude.</i></p>
-</div>
-<p>Once again the shoreline crept eastward, the seas
-cleared, and the Gallatin Limestone was deposited. The
-Gallatin, like the Death Canyon Limestone Member, was
-laid down for the most part in quiet, clear water, probably
-at depths of 100 to 200 feet. However, a few beds of &ldquo;edgewise&rdquo;
-conglomerate indicate the occurrence of sporadic
-storms. At this time, the sea covered all of Idaho and Montana
-and most of Wyoming (<a href="#fig35B">fig. 35B</a>) and extended eastward
-<span class="pb" id="Page_74">74</span>
-across the Dakotas to connect with shallow seas that
-covered the eastern United States. Soon after this maximum
-stage was reached slow uplift caused the sea to retreat gradually
-westward. The site of the Teton Range emerged
-above the waves, where, as far as is now known, it may have
-been exposed to erosion for nearly 70 million years (<a href="#fig35C">fig. 35C</a>).</p>
-<p>The above historical summary of geologic events in
-Cambrian time is recorded in the Cambrian formations.
-This is an example of the reconstructions, based on the sedimentary
-rock record, that have been made of the Paleozoic
-systems in this area.</p>
-<div class="img" id="fig37">
-<p class="pcap">Figure 37. <i>Cambrian fossils in Grand Teton
-National Park.</i></p>
-<p class="pcap">A-B. <i>Phosphatic-shelled
-brachiopods, the
-oldest fossils found in the
-park. Actual width of
-specimens is about
-&frac14; inch.</i></p>
-<p class="pcap">C-D. <i>Trilobites.
-Width of C is &frac14; inch,
-D is &frac12; inch. National
-Park Service photos by
-W. E. Dilley and
-R. A. Mebane.</i></p>
-</div>
-<div class="img" id="fig37A">
-<img src="images/p32a.jpg" alt="" width="588" height="507" />
-<p class="pcap">A.</p>
-</div>
-<div class="img" id="fig37B">
-<img src="images/p32b.jpg" alt="" width="424" height="505" />
-<p class="pcap">B.</p>
-</div>
-<div class="img" id="fig37C">
-<img src="images/p32c.jpg" alt="" width="395" height="500" />
-<p class="pcap">C.</p>
-</div>
-<div class="img" id="fig37D">
-<img src="images/p32d.jpg" alt="" width="450" height="532" />
-<p class="pcap">D.</p>
-</div>
-<h3 id="c41">Younger Paleozoic formations</h3>
-<p>Formations of the remaining Paleozoic systems are
-likewise of interest because of the ways in which they differ
-from those already described.</p>
-<div class="pb" id="Page_75">75</div>
-<div class="img" id="fig38">
-<p class="pcap">Figure 38. <i>Distinctive features of Cambrian rocks.</i></p>
-</div>
-<div class="img" id="fig38A">
-<img src="images/p32g.jpg" alt="" width="700" height="418" />
-<p class="pcap">A. <i>Algal heads
-in the Park Shale Member of the Gros Ventre Formation. These
-calcareous mounds were built by algae growing in a shallow sea in
-Cambrian time. They are now exposed on the divide between
-North and South Leigh Creeks, nearly 2 miles above sea level!</i></p>
-</div>
-<div class="img" id="fig38B">
-<img src="images/p32h.jpg" alt="" width="600" height="467" />
-<p class="pcap">B. <i>Bed of &ldquo;edgewise&rdquo;
-conglomerate in the Gallatin Limestone. Angular plates of solidified
-lime-ooze were torn from the sea bottom by storm waves, swept into
-depressions, and then buried in lime mud. These fragments, seen in cross
-section, make the strange design on the rock. Thin limestone beds below
-are undisturbed. National Park Service photo by W. E. Dilley.</i></p>
-</div>
-<p>The Bighorn Dolomite of Ordovician age forms ragged
-hard massive light-gray to white cliffs 100 to 200 feet
-high (figs. <a href="#fig32">32</a> and <a href="#fig33">33</a>). <i>Dolomite</i> is a calcium-magnesium
-carbonate, but the original sediment probably was a calcium
-carbonate mud that was altered by magnesium-rich
-<span class="pb" id="Page_76">76</span>
-sea water shortly after deposition. Corals and other marine
-animals were abundant in the clear warm seas at this time.</p>
-<p>Dolomite in the Darby Formation of Devonian age differs
-greatly from the Bighorn Dolomite; that in the Darby
-is dark-brown to almost black, has an oily smell, and contains
-layers of black, pink, and yellow mudstone and thin
-sandstone. The sea bottom during deposition of these rocks
-was foul and frequently the water was turbid. Abundant
-fossil fragments indicate fishes were common for the first
-time. Exposures of the Darby Formation are recognizable
-by their distinctive dull-yellow thin-layered slopes between
-the prominent gray massive cliffs of formations below and
-above.</p>
-<p>The Madison Limestone of Mississippian age is 1,000
-feet thick and is exposed in spectacular vertical cliffs along
-canyons in the north, west, and south parts of the Tetons.
-It is noted for the abundant remains of beautifully preserved
-marine organisms (<a href="#fig39">fig. 39</a>). The fossils and the relatively
-pure blue-gray limestone in which they are embedded
-indicate deposition in warm tranquil seas. The
-beautiful Ice Cave on the west side of the Tetons and all
-other major caves in the region were dissolved out of this
-rock by underground water.</p>
-<p>The Pennsylvanian System is represented by the Amsden
-Formation and the Tensleep Sandstone. Cliffs of the
-Tensleep Sandstone can be seen along the Gros Ventre
-River at the east edge of the park. The Amsden, below the
-Tensleep, consists of red and green shale, sandstone, and
-thin limestone. The shale is especially weak and slippery
-when exposed to weathering and saturated with water.
-These are the strata that make up the glide plane of the
-Lower Gros Ventre Slide (<a href="#fig5">fig. 5</a>) east of the park.</p>
-<p>The Phosphoria Formation and its equivalents of Permian
-age are unlike any other Paleozoic rocks because of
-their extraordinary content of uncommon elements. The
-formation consists of sandy dolomite, widespread black
-phosphate beds and black shale that is unusually rich not
-only in phosphorus, but also in vanadium, uranium, chromium,
-zinc, selenium, molybdenum, cobalt, and silver. The
-<span class="pb" id="Page_77">77</span>
-formation is mined extensively in nearby parts of Idaho
-and in Wyoming for phosphatic fertilizer, for the chemical
-element phosphorus, and for some of the metals that can be
-derived from the rocks as byproducts. These elements and
-compounds are not everywhere concentrated enough to be
-of economic interest, but their dollar value is, in a regional
-sense, comparable to that of some of the world&rsquo;s greatest
-mineral deposits.</p>
-<div class="pb" id="Page_78">78</div>
-<div class="img" id="fig39">
-<p class="pcap">Figure 39. <i>A glimpse of the sea floor during deposition of the
-Madison Limestone 330 million years ago, showing the remains of brachiopods, corals, and
-other forms of life that inhabited the shallow warm water.</i></p>
-</div>
-<div class="img" id="fig39A">
-<img src="images/p33.jpg" alt="" width="600" height="444" />
-<p class="pcap">A. <i>Slab in which fossils are
-somewhat broken and scattered.
-Scale slightly reduced. National
-Park Service photo by W. E.
-Dilley and R. A. Mebane.</i></p>
-</div>
-<div class="img" id="fig39B">
-<img src="images/p33a.jpg" alt="" width="600" height="535" />
-<p class="pcap">B. <i>Slab in which fossils are
-remarkably complete. Silver
-dollar gives scale. Specimen is
-in University of Wyoming Geological
-Museum.</i></p>
-</div>
-<div class="pb" id="Page_79">79</div>
-<h2 id="c42"><br /><span class="small">THE MESOZOIC&mdash;ERA OF TRANSITION</span></h2>
-<p>The Mesozoic Era in the Teton region was a time of
-alternating marine, transitional, and continental environments.
-Moreover, the highly diversified forms of life, ranging
-from marine mollusks to tremendous, land-living dinosaurs,
-confirm and reinforce the story of the rocks. Living
-things, too, were in transition, for as environment changed,
-many forms moved from the sea to land in order to survive.
-It was the time when some of the most spectacularly colored
-rock strata of the region were deposited.</p>
-<h3 id="c43">Colorful first Mesozoic strata</h3>
-<p>Bright-red soft Triassic rocks more than 1,000 feet
-thick, known as the Chugwater Formation, comprise most
-of the basal part of the Mesozoic sequence (<a href="#table4">table 4</a>). They
-form colorful hills east and south of the park. The red color
-is caused by a minor amount of iron oxide. Mud cracks and
-the presence of fossil reptiles and amphibians indicate
-deposition in a tidal flat environment, with the sea lying
-several miles southwest of Jackson Hole. A few beds of
-white <i>gypsum</i> (calcium sulfate) are present; they were apparently
-deposited during evaporation of shallow bodies of
-salt water cut off from the open sea.</p>
-<p>As the Triassic Period gave way to the Jurassic, salmon-red
-windblown sand (Nugget Sandstone) spread
-across the older red beds and in turn was buried by thin red
-shale and thick gypsum deposits of the Gypsum Spring
-Formation. Then down from Alaska and spreading across
-most of Wyoming came the <i>Sundance Sea</i>, a warm, muddy,
-shallow body of water that teemed with marine mollusks. In
-it more than 500 feet of highly fossiliferous soft gray shale
-and thin limestones and sandstones were deposited. The
-sea withdrew and the Morrison and Cloverly Formations
-(Jurassic and Lower Cretaceous) were deposited on low-lying
-tropical humid flood plains. These rocks are colorful,
-consisting of red, pink, purple, and green badland-forming
-claystones and mudstones, and yellow to buff sandstones.
-Vegetation was abundant and large and small dinosaurs
-roamed the countryside or inhabited the swamps.</p>
-<div class="pb" id="Page_80">80</div>
-<div class="img" id="table4">
-<img src="images/p34.jpg" alt="" width="600" height="1098" />
-<p class="pcap"><span class="ss">Table 4.&mdash;Mesozoic sedimentary rocks exposed in the Teton region.</span></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>Age </th><th class="l">Formation </th><th class="l">Thickness (feet) </th><th class="l">Description </th><th class="l">Where exposed</th></tr>
-<tr><td colspan="2" class="l">CRETACEOUS</td></tr>
-<tr><td class="lt"> </td><td class="l">Harebell Formation </td><td class="l">0-5,000 </td><td class="l">Sandstone, olive drab, silty, drab siltstone, and dark-gray shale; thick beds of quartzite pebble conglomerate in upper part. </td><td class="l">Eastern and northeastern parts of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Meeteetse Formation </td><td class="l">0-700 </td><td class="l">Sandstone, gray to chalky white, blue-green to gray siltstone, thin coal, and green to yellow bentonite. </td><td class="l">Spread Creek area.</td></tr>
-<tr><td class="lt"> </td><td class="l">Mesaverde Formation </td><td class="l">0-1,000 </td><td class="l">Sandstone, white, massive, soft, thin gray shale, sparse coal. </td><td class="l">Eastern Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Unnamed sequence of lenticular sandstone, shale, and coal. </td><td class="l">3,500&plusmn; </td><td class="l">Sandstone and shale, gray to brown; abundant coal in lower 2,000 feet. </td><td class="l">Eastern Jackson Hole and eastern margin of the park.</td></tr>
-<tr><td class="lt"> </td><td class="l">Bacon Ridge Sandstone </td><td class="l">900-1,200 </td><td class="l">Sandstone, light gray, massive, marine, gray shale, many coal beds. </td><td class="l">Eastern Jackson Hole and eastern margin of the park.</td></tr>
-<tr><td class="lt"> </td><td class="l">Cody Shale </td><td class="l">1,300-2,200 </td><td class="l">Shale, gray, soft; thin green sandstone, some bentonite; marine. </td><td class="l">Eastern and northern parts of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Frontier Formation </td><td class="l">1,000 </td><td class="l">Sandstone, gray, and black to gray shale, marine; many persistent white bentonite beds in lower part. </td><td class="l">Eastern and northern parts and south-western margin of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Mowry Shale </td><td class="l">700 </td><td class="l">Shale, silvery-gray, hard, siliceous, with many fish scales; thin bentonite beds; marine. </td><td class="l">Gros Ventre River Valley, northern margin of the park, and southern part of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Thermopolis Shale </td><td class="l">150-200 </td><td class="l">Shale, black, soft, fissile, with persistent sandstone at top; marine. </td><td class="l">Gros Ventre River Valley, northern margin of the park, and southern part of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Cloverly and Morrison(?) Formations </td><td class="l">650 </td><td class="l">Sandstone, light gray, sparkly, rusty near top, underlain by variegated soft claystone; basal part is silty dully-variegated sandstone and claystone. </td><td class="l">North end of Teton Range and Gros Ventre River Valley.</td></tr>
-<tr><td colspan="2" class="l">JURASSIC</td></tr>
-<tr><td class="lt"> </td><td class="l">Sundance Formation </td><td class="l">500-700 </td><td class="l">Sandstone, green, underlain by soft gray shale and thin highly fossiliferous limestones; marine. </td><td class="l">North end of Teton Range, Blacktail Butte, Gros Ventre River Valley.</td></tr>
-<tr><td class="lt"> </td><td class="l">Gypsum Spring Formation </td><td class="l">75-100 </td><td class="l">Gypsum, white, interbedded with red shale and gray dolomite; partly marine. </td><td class="l">North end of Teton Range, Blacktail Butte, Gros Ventre River Valley.</td></tr>
-<tr><td class="lt"> </td><td class="l">Nugget Sandstone </td><td class="l">0-350 </td><td class="l">Sandstone, salmon-red, hard. </td><td class="l">North flank of Gros Ventre Mountains, southern Jackson Hole.</td></tr>
-<tr><td colspan="2" class="l">TRIASSIC</td></tr>
-<tr><td class="lt"> </td><td class="l">Chugwater Formation </td><td class="l">1,000-1,500 </td><td class="l">Siltstone and shale, red, thin-bedded; one thin marine limestone in upper third. </td><td class="l">North flank of Gros Ventre Mountains, north end of Teton Range, southernmost Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l">Dinwoody Formation </td><td class="l">200-400 </td><td class="l">Siltstone, brown, hard, thin-bedded; marine. </td><td class="l">North flank of Gros Ventre Mountains, north end of Teton Range, southernmost Jackson Hole.</td></tr>
-</table>
-<div class="pb" id="Page_81">81</div>
-<h3 id="c44">Drab Cretaceous strata</h3>
-<p>The youngest division of the <i>Mesozoic</i> Era is the
-Cretaceous Period. Near the beginning of this period,
-brightly colored rocks continued to be deposited. Then, the
-Teton region, as well as most of Wyoming, was partly, and
-at times completely, submerged by shallow muddy seas. As
-a result, the brightly variegated strata were covered by
-10,000 feet of generally drab-colored sand, silt, and clay
-containing some coal beds, volcanic ash layers, and minor
-amounts of gravel.</p>
-<p>The Cretaceous sea finally retreated eastward from
-the Teton region about 85 million years ago, following the
-deposition of the Bacon Ridge Sandstone (<a href="#fig40">fig. 40</a>). As it
-withdrew, extensive coal swamps developed along the sea
-coast. The record of these swamps is preserved in coal beds
-5 to 10 feet thick in the Upper Cretaceous deposits. The
-coal beds are now visible in abandoned mines along the east
-margin of the park. Coal is formed from compacted plant
-debris; about 5 feet of this material is needed to form 1
-inch of coal. Thus, lush vegetation must have flourished
-for long periods of time, probably in a hot wet climate similar
-to that now prevailing in the Florida Everglades.</p>
-<p>Sporadically throughout Cretaceous time fine-grained
-ash was blown out of volcanoes to the west and northwest
-and deposited in quiet shallow water. Subsequently the ash
-was altered to a type of clay called <i>bentonite</i> that is used
-in the foundry industry and in oil well drilling muds. In
-Jackson Hole, the elk and deer lick bentonite exposures to
-get a bitter salt and, where the beds are water-saturated, enjoy
-&ldquo;stomping&rdquo; on them. Bentonite swells when wet and
-causes many landslides along access roads into Jackson
-Hole (<a href="#fig17">fig. 17</a>).</p>
-<p>The Cretaceous rocks in the Teton region are part of
-an enormous east-thinning wedge that here is nearly 2 miles
-thick. Most of the debris was derived from slowly rising
-mountains to the west.</p>
-<p>Cretaceous sedimentary rocks are much more than of
-just scientific interest; they contain mineral deposits important
-to the economy of Wyoming and of the nation.
-<span class="pb" id="Page_82">82</span>
-Wyoming leads the States in production of bentonite, all of
-it from Cretaceous rocks. These strata have yielded far
-more oil and gas than any other geologic system in the State
-and the production is geographically widespread. They
-also contain enormous coal reserves, some in beds between
-50 and 100 feet thick. The energy resources alone of the
-Cretaceous System in Wyoming make it invaluable to our
-industrialized society.</p>
-<div class="img" id="fig40">
-<img src="images/p35.jpg" alt="" width="600" height="228" />
-<p class="pcap">Figure 40. <i>The yardstick and the sea. The shaded part of the yardstick
-shows the 500-million-year interval during which Paleozoic and Mesozoic
-seas swept intermittently across the future site of the Tetons. When they
-finally withdrew about 85 million years ago, a little more than 5/8 of an inch
-of the yardstick remained to be accounted for.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th class="l"> </th><th>ABSOLUTE TIME (Millions of years ago) </th><th class="c">INCHES</th></tr>
-<tr><td class="l">{submerged} </td><td class="c">85-585 </td><td class="c">&#8541;-4&#8541;</td></tr>
-<tr><td class="l">CENOZOIC </td><td class="c">0-80 </td><td class="c">0-&frac12;</td></tr>
-<tr><td class="l">MESOZOIC </td><td class="c">80-180 </td><td class="c">&frac12;-&#8542;</td></tr>
-<tr><td class="l">PALEOZOIC </td><td class="c">180-570 </td><td class="c">&#8542;-4&#8542;</td></tr>
-<tr><td class="l">PRECAMBRIAN </td><td class="c">570- </td><td class="c">4&#8542;-</td></tr>
-</table>
-<p>As the end of the Cretaceous Period approached,
-slightly more than 80 million years ago, the flat monotonous
-landscape (<a href="#fig41">fig. 41</a>) which had prevailed during
-most of Late Cretaceous time gave little hint that the stage
-was set for one of the most exciting and important chapters
-in the geologic history of North America.</p>
-<h3 id="c45">Birth of the Rocky Mountains</h3>
-<p>The episode of mountain building that resulted in formation
-of the ancestral Rocky Mountains has long been
-known as the <i>Laramide Revolution</i>. West and southwest of
-Wyoming, mountains had already formed, the older ones as
-far away as Nevada and as far back in time as Jurassic,
-the younger ones rising progressively farther east, like
-<span class="pb" id="Page_83">83</span>
-giant waves moving toward a coast. The first crustal movement
-in the Teton area began in latest Cretaceous time when
-a broad low northwest-trending arch developed in the approximate
-area of the present Teton Range and Gros Ventre
-Mountains. However, this uplift bore no resemblance to the
-Tetons as we know them today for the present range formed
-70 million years later.</p>
-<div class="img" id="fig41">
-<img src="images/p35a.jpg" alt="" width="600" height="512" />
-<p class="pcap">Figure 41. <i>Grand Teton National Park region slightly more than 80 million
-years ago, just before onset of Laramide Revolution. The last Cretaceous
-sea still lingered in central Wyoming.</i></p>
-</div>
-<p>One bit of evidence (there are others) of the first
-Laramide mountain building west of the Tetons is a tremendous
-deposit of quartzite boulder debris (several hundred
-cubic miles in volume) derived from the <i>Targhee uplift</i>
-(<a href="#fig42">fig. 42</a>). Nowhere is the uplift now exposed, but from the
-size, composition, and distribution of rock fragments that
-came from it, we know that it was north and west of the
-northern end of the present-day Teton Range. Powerful
-streams carried boulders, sand, and clay eastward and
-<span class="pb" id="Page_84">84</span>
-southeastward across the future site of Jackson Hole and
-deposited them in the Harebell Formation (<a href="#table4">table 4</a>). Mingled
-with this sediment were tiny flakes of gold and a small
-amount of mercury. Fine-grained debris was carried still
-farther east and southeast into two enormous depositional
-troughs in central and southern Wyoming. Most of the
-large rock fragments were derived from Precambrian and
-possibly lower Paleozoic quartzites. This means that at
-least 15,000 feet of overlying Paleozoic and Mesozoic strata
-must first have been stripped away from the Targhee uplift
-before the quartzites were exposed to erosion.</p>
-<div class="img" id="fig42">
-<img src="images/p36.jpg" alt="" width="600" height="517" />
-<p class="pcap">Figure 42. <i>Teton region at the end of Cretaceous time about 65 million years
-ago. The ancestral Teton-Gros Ventre uplift had risen and prominent southeastward
-drainage from the Targhee uplift was well established. See <a href="#fig41">figure 41</a> for State lines and location map.</i></p>
-</div>
-<div class="pb" id="Page_85">85</div>
-<p>Remains of four-legged horned ceratopsian dinosaurs,
-possibly <i>Triceratops</i> (<a href="#fig43">fig. 43</a>), reflecting the last population
-explosion of these reptiles, have been found in pebbly
-sandstone of the Harebell Formation in highway cuts on the
-Togwotee Pass road 8 miles east of the park.</p>
-<div class="img" id="fig43">
-<img src="images/p36a.jpg" alt="" width="600" height="358" />
-<p class="pcap">Figure 43. <i>Triceratops, a horned dinosaur of the type that inhabited Jackson
-Hole about 65 million years ago. Sketch by S. H. Knight.</i></p>
-</div>
-<p>Near the end of Cretaceous time, broad gentle uplifts
-also began to stir at the sites of future mountain ranges in
-many parts of Wyoming. The ancestral Teton-Gros Ventre
-arch continued to grow. Associated with and parallel to it
-was a series of sharp steepsided elongated northwest-trending
-upfolds (<i>anticlines</i>). One of these can be seen where it
-crosses the highway at the Lava Creek Campground near
-the eastern margin of Grand Teton National Park.</p>
-<p>During these episodes of mountain building, erosion,
-and deposition, the dinosaurs became extinct all over the
-world. The &ldquo;Age of Mammals&rdquo; was about to begin.</p>
-<div class="pb" id="Page_86">86</div>
-<h2 id="c46"><br /><span class="small">TERTIARY&mdash;TIME OF MAMMALS, MOUNTAINS, LAKES, AND VOLCANOES</span></h2>
-<div class="img" id="fig44">
-<img src="images/p37.jpg" alt="" width="600" height="704" />
-<p class="pcap">Figure 44. <i>The last inch of the yardstick, enlarged to show subdivisions of
-the Cenozoic Era.</i></p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th colspan="3">STRATIGRAPHIC SCALE </th><th class="lt">THE LAST INCH OF THE YARDSTICK </th><th class="l">ABSOLUTE TIME (million years ago)</th></tr>
-<tr><td class="l" colspan="3">CENOZOIC</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">QUATERNARY</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Recent and Pleistocene </td><td class="c">0 </td><td class="c">0</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">TERTIARY</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Pliocene </td><td class="c">0 </td><td class="c">0</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Miocene </td><td class="c">&#8539; </td><td class="c">12</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Oligocene </td><td class="c">&frac14; </td><td class="c">25</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Eocene </td><td class="c">&#8540; </td><td class="c">40</td></tr>
-<tr><td class="lt"> </td><td class="lt"> </td><td class="l">Paleocene </td><td class="c">&#8311;/&#8321;&#8326; </td><td class="c">55</td></tr>
-<tr><td class="l" colspan="3">MESOZOIC</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">CRETACEOUS </td><td class="l">&frac12; </td><td class="c">65</td></tr>
-</table>
-<p>The Cenozoic (<a href="#table1">table 1</a>), last and shortest of the geologic
-eras, comprises the Tertiary and Quaternary Periods.
-It began about 65 million years ago and is represented by
-only the final one-half inch of our imaginary yardstick of
-time (<a href="#fig19">fig. 19</a>). Nevertheless, it is the era during which the
-Tetons rose in their present form and the landscape was
-sculptured into the panorama of beauty that we now see. In
-order to show the many Tertiary and Quaternary events in
-the Teton region, it is necessary to enlarge greatly the last
-part of the yardstick (<a href="#fig44">fig. 44</a>). There are two reasons for
-<span class="pb" id="Page_87">87</span>
-the extraordinarily clear and complete record. First, the
-Teton region was a relatively active part of the earth&rsquo;s crust,
-characterized by many downdropped blocks. The number
-of events is great and their records are preserved in sediments
-trapped in the subsiding basins. Second, the geologically
-recent past is much easier to see than the far dimmer,
-distant past; the rocks that record later events are
-fresher, less altered, more complete, and more easily interpreted
-than are those that tell us of older events.</p>
-<div class="img" id="table5">
-<img src="images/p37a.jpg" alt="" width="700" height="598" />
-<p class="pcap">Table 5.&mdash;Cenozoic sedimentary rocks and unconsolidated deposits in the Teton region.</p>
-</div>
-<table class="center" summary="">
-<tr class="th"><th>Age </th><th class="l"> </th><th class="l">Formation </th><th class="l">Thickness (feet) </th><th class="l">Description </th><th class="l">Where exposed</th></tr>
-<tr><td class="l" colspan="3">QUATERNARY</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Recent</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Modern stream, landslide, glacial and talus deposits </td><td class="l">0-200&plusmn; </td><td class="l">Sand, gravel, and silt along present streams; jumbled broken rock in landslides and on talus slopes; debris around existing glaciers. </td><td class="l">Floor of Jackson Hole and in canyons and on mountainsides throughout the region.</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Pleistocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Glacial deposits and loess </td><td class="l">0-200&plusmn; </td><td class="l">Gravel, sand, silt, and glacial debris. </td><td class="l">Floor of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Unnamed upper lake sequence </td><td class="l">0-500 </td><td class="l">Shale, brown-gray, sandstone, and conglomerate. </td><td class="l">Gros Ventre River Valley.</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Unnamed lower lake sequence </td><td class="l">0-200 </td><td class="l">Shale, siltstone, and sandstone, gray, green, and red. </td><td class="l">National Elk Refuge.</td></tr>
-<tr><td class="lt">? </td><td class="l" colspan="3">Pleistocene or Pliocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Bivouac Formation </td><td class="l">0-1,000 </td><td class="l">Conglomerate, with purplish-gray welded tuff in upper part. </td><td class="l">Signal Mountain and West Gros Ventre Butte.</td></tr>
-<tr><td class="l" colspan="3">TERTIARY</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Pliocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Teewinot Formation </td><td class="l">0-6,000 </td><td class="l">Limestone, tuff, and claystone, white, soft. </td><td class="l">National Elk Refuge, Blacktail Butte, and eastern margin of Antelope Flat.</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Camp Davis Formation </td><td class="l">0-5,500 </td><td class="l">Conglomerate, red and gray, with white tuff, diatomite, and red and white claystone. </td><td class="l">Southernmost tip of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Miocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Colter Formation </td><td class="l">0-7,000 </td><td class="l">Volcanic conglomerate, tuff, and sandstone, white to green-brown, with locally-derived basalt and andesite rock fragments. </td><td class="l">Pilgrim and Ditch Creeks, and north end of Teton Range.</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Oligocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Wiggins Formation </td><td class="l">0-3,000 </td><td class="l">Volcanic conglomerate, gray to brown, with white tuff layers. </td><td class="l">Eastern margin of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Eocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Unnamed upper and middle Eocene sequence </td><td class="l">0-1,000 </td><td class="l">Tuff, conglomerate, sandstone, and claystone, green, underlain by variegated claystone and quartzite pebble conglomerate. </td><td class="l">Eastern margin of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Wind River and Indian Meadows Formations </td><td class="l">2,000-3,000 </td><td class="l">Claystone and sandstone, variegated, and locally-derived conglomerate; persistent coal and gray shale zone in middle. </td><td class="l">Eastern margin of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l" colspan="2">Paleocene</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Unnamed greenish-gray and brown sandstone and claystone sequence </td><td class="l">1,000-2,000 </td><td class="l">Sandstone and claystone, greenish-gray and brown, intertonguing at base with quartzite pebble conglomerate. </td><td class="l">Eastern margin of Jackson Hole.</td></tr>
-<tr><td class="lt"> </td><td class="l"> </td><td class="l">Pinyon Conglomerate </td><td class="l">500-5,000 </td><td class="l">Conglomerate, brown, chiefly of rounded quartzite; coal and claystone locally at base. </td><td class="l">Eastern part of Jackson Hole, Mt. Leidy and Pinyon Peak Highlands, and north end of Teton Range.</td></tr>
-</table>
-<div class="pb" id="Page_88">88</div>
-<div class="img" id="fig45">
-<img src="images/p38.jpg" alt="" width="600" height="409" />
-<p class="pcap">Figure 45. <i>Pinyon Conglomerate of Paleocene age, along the northwest
-margin of the Teton Range.</i></p>
-</div>
-<p>During the early part of the Tertiary Period, mountain
-building and basin subsidence were the dominant types
-of crustal movement. Seas retreated southward down the
-Mississippi Valley and never again invaded the Teton area.
-Environments on the recently uplifted land were diverse
-and favorable for the development of new forms of plants
-and animals.</p>
-<h3 id="c47">Rise and burial of mountains</h3>
-<p>The enormous section of Tertiary sedimentary rocks
-in the Jackson Hole area (<a href="#table5">table 5</a>) is one of the most impressive
-in North America. If the maximum thicknesses of
-all formations were added, they would total more than 6
-miles, but nowhere did this amount of rock accumulate in a
-single unbroken sequence. No other region in the United
-States contains a thicker or more complete nonmarine Tertiary
-record; many areas have little or none. The accumulation
-in Jackson Hole reflects active uplifts of nearby
-mountains that supplied abundant rock debris, concurrent
-<span class="pb" id="Page_89">89</span>
-sinking of nearby basins in which the sediments could be
-preserved, and proximity to the great Yellowstone-Absaroka
-volcanic area, one of the most active continental volcanic
-fields in the United States. The volume and composition
-of the Tertiary strata are, therefore, clear evidence of
-crustal and subcrustal instability.</p>
-<div class="img" id="fig46">
-<img src="images/p38a.jpg" alt="" width="600" height="522" />
-<p class="pcap">Figure 46. <i>Teton region near end of deposition of Paleocene rocks, slightly
-less than 60 million years ago. The ancestral Teton-Gros Ventre uplift
-formed a partial barrier between the Jackson Hole and Green River depositional
-basins; major drainages from the Targhee uplift spread an enormous
-sheet of gravel for 100 miles to the east. See <a href="#fig41">figure 41</a> for State lines and
-location map.</i></p>
-</div>
-<p>The many thick layers of conglomerate are evidence
-of rapid erosion of nearby highlands. The Pinyon Conglomerate
-(<a href="#fig45">fig. 45</a>), for example, contains zones as much
-as 2,500 feet thick of remarkably well-rounded pebbles,
-cobbles, and boulders, chiefly of quartzite identical with
-that in the underlying Harebell Formation and derived
-from the same source, the Targhee uplift. Like the Harebell
-the matrix contains small amounts of gold and mercury.
-<span class="pb" id="Page_90">90</span>
-Rock fragments increase in size northwestward toward
-the source area (<a href="#fig46">fig. 46</a>) and most show percussion
-scars, evidence of ferocious pounding that occurred during
-transport by powerful, swift rivers and steep gradients.</p>
-<div class="img" id="fig47">
-<img src="images/p39.jpg" alt="" width="600" height="515" />
-<p class="pcap">Figure 47. <i>Teton region at climax of Laramide Revolution, between 50 and
-55 million years ago. See <a href="#fig41">figure 41</a> for State lines and location map.</i></p>
-</div>
-<p>Conglomerates such as the Pinyon are not the only
-clue to the time of mountain building. Another type of evidence&mdash;faults&mdash;is
-demonstrated in <a href="#fig16">figure 16</a>. The youngest
-rocks cut by a fault are always older than the fault.
-Many faults and the rocks on each side are covered by still
-younger unbroken sediments. These must, therefore, have
-been deposited after fault movement ceased. By dating
-both the faulted and the overlying unbroken sediments, the
-time of fault movement can be bracketed.</p>
-<p>Observations of this type in western Wyoming indicate
-that the Laramide Revolution reached a climax during
-<span class="pb" id="Page_91">91</span>
-earliest Eocene time, 50 to 55 million years ago. Mountain-producing
-upwarps formed during this episode were
-commonly bounded on one side by either reverse or thrust
-faults (fig. <a href="#fig16B">16B</a> and <a href="#fig16C">16C</a>) and intervening blocks were downfolded
-into large, very deep basins. The amount of movement
-of the mountain blocks over the basins ranged from
-tens of miles in the Snake River, Salt River, Wyoming, and
-Hoback Ranges directly south of the Tetons to less than 5
-miles on the east margin of Jackson Hole (the west flank
-of the Washakie Range shown in <a href="#fig1">figure 1</a>). The ancestral
-Teton-Gros Ventre uplift continued to rise but remained
-one of the less conspicuous mountain ranges in the region
-(<a href="#fig47">fig. 47</a>).</p>
-<p>The Buck Mountain fault, the great reverse fault
-which lies just west of the highest Teton peaks (see <a href="#fig62">geologic map</a>
-and <a href="#pic2">cross section</a>), was formed either at this time or
-during a later episode of movement that also involved the
-southwest margin of the Gros Ventre Mountains. The Buck
-Mountain fault is of special importance because it raised a
-segment of Precambrian rocks several thousand feet. Later,
-when the entire range as we now know it was uplifted by
-movement along the Teton fault, the hard basement rocks
-in this previously upfaulted segment continued to stand
-much higher than those in adjacent parts of the range. All
-of the major peaks in the Tetons are carved from this
-doubly uplifted block.</p>
-<p>The brightly colored sandstone, mudstone, and claystone
-in the Indian Meadows and Wind River Formations
-(lower Eocene) in the eastern part of Jackson Hole were
-derived from variegated Triassic, Jurassic, and Lower Cretaceous
-rocks exposed on the adjacent mountain flanks.
-Fossils in these Eocene Formations show that it took less
-than 10 million years for the uplifts to be deeply eroded
-and partially buried in their own debris.</p>
-<p>The Laramide Revolution in the area of Grand Teton
-National Park ended during Eocene time between 45 and
-50 million years ago, and as the mountains and basins became
-stabilized a new element was added. Volcanoes broke
-through to the surface in many parts of the Yellowstone-Absaroka
-<span class="pb" id="Page_92">92</span>
-area and the constantly increasing volume of
-their eruptive debris was a major factor in the speed of
-filling of basins and burial of mountains throughout Wyoming.
-This entire process only took about 20 million years,
-and along the east margin of Jackson Hole it was largely
-completed during Oligocene time (<a href="#fig48">fig. 48</a>). However, east
-and northeast of Jackson Lake a Miocene downwarp subsequently
-formed and in it accumulated at least 7,000 feet of
-locally derived sediments of volcanic origin.</p>
-<div class="img" id="fig48">
-<img src="images/p40.jpg" alt="" width="600" height="513" />
-<p class="pcap">Figure 48. <i>Teton region near the close of Oligocene deposition, between 25
-and 30 million years ago, showing areas of major volcanoes and lava flows.
-See <a href="#fig41">figure 41</a> for State lines and location map.</i></p>
-</div>
-<h3 id="c48">The First Big Lake</h3>
-<p><i>Teewinot Lake</i> (<a href="#fig49">fig. 49</a>), the first big freshwater lake
-in Jackson Hole, was formed during Pliocene time, about
-10 million years ago, and in it the Teewinot Formation was
-deposited. These lake strata consist of more than 5,000
-feet of white limestone, thin-bedded claystone, and <i>tuff</i>
-<span class="pb" id="Page_93">93</span>
-(solidified ash made up of tiny fragments of volcanic rock
-and splinters of volcanic glass). The claystones contain fossil
-snails, clams, beaver bones and teeth, aquatic mice,
-suckers, and other fossils that indicate deposition in a shallow
-freshwater lake environment. These beds underlie
-Jackson Lake Lodge, the National Elk Refuge, part of
-Blacktail Butte, and are conspicuously exposed in white
-outcrops that look like snowbanks on the upper slopes along
-the east margin of the park across the valley from the
-Grand Teton.</p>
-<div class="img" id="fig49">
-<img src="images/p40a.jpg" alt="" width="600" height="523" />
-<p class="pcap">Figure 49. <i>Teton region near close of middle Pliocene time, about 5 million
-years ago, showing areas of major volcanoes and lava flows. See <a href="#fig41">figure 41</a> for
-State lines and location map.</i></p>
-</div>
-<p>Teewinot Lake was formed on a down-faulted block
-and was dammed behind (north of) a fault that trends east
-across the floor of Jackson Hole at the south boundary of
-the park. Lakes are among the most short-lived of earth
-features because the forces of nature soon conspire to fill
-them up or empty them. This lake existed for perhaps 5
-million years during middle Pliocene time; it was shallow,
-and remained so despite the pouring in of a mile-thick layer
-of sediment. This indicates that downdropping of the lake
-floor just about kept pace with deposition.</p>
-<div class="pb" id="Page_94">94</div>
-<div class="img" id="fig50">
-<img src="images/p41.jpg" alt="" width="600" height="768" />
-<p class="pcap">Figure 50. <i>Restoration of a middle Eocene landscape showing some of the
-more abundant types of mammals. Mural painting by Jay H. Matterness;
-photo courtesy of the Smithsonian Institution.</i></p>
-</div>
-<table class="center" summary="">
-<tr><td class="l"><i>Uintatherium</i> </td><td class="l">6-horned, saber-toothed plant eater</td></tr>
-<tr><td class="l"><i>Stylinodon</i> </td><td class="l">gnawing-toothed mammal</td></tr>
-<tr><td class="l"><i>Palaeosyops</i> </td><td class="l">early titanothere</td></tr>
-<tr><td class="l"><i>Helaletes</i> </td><td class="l">primitive tapir</td></tr>
-<tr><td class="l"><i>Sciuravus</i> </td><td class="l">squirrel-like rodent</td></tr>
-<tr><td class="l"><i>Smilodectes</i> </td><td class="l">lemurlike monkey</td></tr>
-<tr><td class="l"><i>Trogosus</i> </td><td class="l">gnawing-toothed mammal</td></tr>
-<tr><td class="l"><i>Hyrachyus</i> </td><td class="l">fleet-footed rhinoceros</td></tr>
-<tr><td class="l"><i>Ischyrotomus</i> </td><td class="l">marmotlike rodent</td></tr>
-<tr><td class="l"><i>Homacodon</i> </td><td class="l">even-toed hoofed animal</td></tr>
-<tr><td class="l"><i>Orohippus</i> </td><td class="l">ancestral horse</td></tr>
-<tr><td class="l"><i>Patriofelis</i> </td><td class="l">large flesh eater</td></tr>
-<tr><td class="l"><i>Mesonyx</i> </td><td class="l">hyenalike mammal</td></tr>
-<tr><td class="l"><i>Helohyus</i> </td><td class="l">even-toed hoofed mammal</td></tr>
-<tr><td class="l"><i>Metacheiromys</i> </td><td class="l">armadillolike edentate</td></tr>
-<tr><td class="l"><i>Machaeroides</i> </td><td class="l">saber-toothed mammal</td></tr>
-<tr><td class="l"><i>Hyopsodus</i> </td><td class="l">clawed, plant-eating mammal</td></tr>
-<tr><td class="l"><i>Saniwa</i> </td><td class="l">monitorlike lizard</td></tr>
-<tr><td class="l"><i>Crocodilus</i> </td><td class="l">crocodile</td></tr>
-<tr><td class="l"><i>Echmatemys</i> </td><td class="l">turtle</td></tr>
-</table>
-<div class="pb" id="Page_95">95</div>
-<p>Other lakes formed in response to similar crustal
-movements in nearby places. One such lake, <i>Grand Valley
-Lake</i> (<a href="#fig49">fig. 49</a>), formed about 25 miles southwest of Teewinot
-Lake; both contained sediments with nearly the same
-thickness, composition, appearance, age, and fossils. Although
-these two lakes are on opposite sides of the Snake
-River Range, the ancestral Snake River apparently flowed
-through a canyon previously cut across the range and provided
-a direct connection between them.</p>
-<h3 id="c49">Development of mammals</h3>
-<p>The Cenozoic Era is known as the &ldquo;Age of Mammals.&rdquo;
-Small mammals had already existed, though quite inconspicuously,
-in Wyoming for about 90 million years before
-Paleocene time. Then about 65 million years ago their proliferation
-began as a result of the extinction of dinosaurs,
-obliteration of seaways that were barriers to distribution,
-and the development of new and varied types of environment.
-These new environments included savannah plains,
-low hills and high mountains, freshwater lakes and swamps,
-and extensive river systems. The mammals increased in
-size and, for the first time, became abundant in numbers of
-both species and individuals. The development and widespread
-distribution of grasses and other forage on which
-many of the animals depended were highly significant.
-Successful adaptation of <i>herbivores</i> (vegetation-eating animals)
-led, in turn, to increased varieties and numbers of
-predatory <i>carnivores</i> (meat-eating animals).</p>
-<p>During early Eocene time, coal swamps formed in
-eastern Jackson Hole and persisted for thousands of years,
-as is shown by 60 feet of coal in a single bed at one locality.
-Continuing on into middle Eocene time, the climate was
-subtropical and humid, and the terrain was near sea level.
-Tropical breadfruits, figs, and magnolias flourished along
-with a more temperate flora of redwood, hickory, maple,
-and oak. Horses the size of a dog and many other small
-mammals were abundant. Primates, thriving in an ideal
-forest habitat, were numerous. Streams contained gar fish
-and crocodiles (<a href="#fig50">fig. 50</a>).</p>
-<div class="pb" id="Page_96">96</div>
-<div class="img" id="fig51">
-<img src="images/p42.jpg" alt="" width="600" height="699" />
-<p class="pcap">Figure 51. <i>A typical Oligocene landscape showing some of the more abundant
-types of mammals. Mural painting by Jay H. Matterness; photo courtesy
-of Smithsonian Institution.</i></p>
-</div>
-<table class="center" summary="">
-<tr><td class="l"><i>Trigonias</i> </td><td class="l">early rhinoceros</td></tr>
-<tr><td class="l"><i>Perchoerus</i> </td><td class="l">early peccary</td></tr>
-<tr><td class="l"><i>Mesohippus</i> </td><td class="l">3-toed horse</td></tr>
-<tr><td class="l"><i>Aepinacodon</i> </td><td class="l">remote relative of hippopotamus</td></tr>
-<tr><td class="l"><i>Archaeotherium</i> </td><td class="l">giant piglike mammal</td></tr>
-<tr><td class="l"><i>Protoceras</i> </td><td class="l">bizarre horned ruminant</td></tr>
-<tr><td class="l"><i>Hesperocyon</i> </td><td class="l">ancestral dog</td></tr>
-<tr><td class="l"><i>Hyracodon</i> </td><td class="l">small fleet-footed rhinoceros</td></tr>
-<tr><td class="l"><i>Po&euml;brotherium</i> </td><td class="l">ancestral camel</td></tr>
-<tr><td class="l"><i>Hypisodus</i> </td><td class="l">very small chevrotainlike ruminant</td></tr>
-<tr><td class="l"><i>Ictops</i> </td><td class="l">small insect-eating mammal</td></tr>
-<tr><td class="l"><i>Brontotherium</i> </td><td class="l">titanothere</td></tr>
-<tr><td class="l"><i>Protapirus</i> </td><td class="l">ancestral tapir</td></tr>
-<tr><td class="l"><i>Glyptosaurus</i> </td><td class="l">extinct lizard</td></tr>
-<tr><td class="l"><i>Hoplophoneus</i> </td><td class="l">saber-toothed cat</td></tr>
-<tr><td class="l"><i>Subhyracodon</i> </td><td class="l">early rhinoceros</td></tr>
-<tr><td class="l"><i>Merycoidodon</i> </td><td class="l">sheeplike grazing mammal</td></tr>
-<tr><td class="l"><i>Hyaenodon</i> </td><td class="l">archaic hyenalike mammal</td></tr>
-<tr><td class="l"><i>Hypertragulus</i> </td><td class="l">chevrotainlike ruminant</td></tr>
-</table>
-<div class="pb" id="Page_97">97</div>
-<p>Early in the Oligocene Epoch, between 30 and 35 million
-years ago, the climate in Jackson Hole became cooler
-and drier, and the subtropical plants gave way to the warm
-temperate flora of oak, beech, maple, alder, and ash. The
-general land surface rose higher above sea level, perhaps
-by accumulation of several thousand feet of Oligocene volcanic
-rocks (<a href="#fig52">fig. 52</a>) rather than by continental uplift.
-<i>Titanotheres</i> (large four-legged mammals with the general
-size and shape of a rhinoceros) flourished in great numbers
-for a few million years and then abruptly vanished. Horses
-by now were about the size of a very small modern colt.
-Rabbits, rodents, carnivores, tiny camels, and other mammals
-were abundant in Jackson Hole, and the fauna, surprisingly,
-was essentially the same as that 500 miles to the
-east, at a much lower elevation, on the plains of Nebraska
-and South Dakota (<a href="#fig51">fig. 51</a>).</p>
-<p>The Miocene Epoch (15 to 25 million years ago) was
-the time of such intense volcanic activity in the Teton region
-that animals must have found survival very difficult. A
-few skeletons and fragmentary parts of camels about the
-size of a small horse and other piglike animals called
-<i>oreodonts</i> comprise our only record of mammals; nothing
-is known of the plants. Farther east the climate fluctuated
-from subtropical to warm temperate, gradually becoming
-cooler toward the end of the epoch.</p>
-<p>Fossils in the Pliocene lake deposits (8 to 10 million
-years old; see description of Teewinot Formation) include
-shallow-water types of snails, clams, diatoms, and ostracodes,
-as well as beavers, mice, suckers, and frogs. Pollen
-in these beds show that adjacent upland areas supported
-fir, spruce, pine, juniper, sage, and other trees and shrubs
-common to the area today. Therefore, the climate must
-have been much cooler than in Miocene time. No large
-mammals of Pliocene age have been found in Jackson Hole.
-The record of life during Quaternary time is discussed
-later.</p>
-<div class="pb" id="Page_98">98</div>
-<div class="img" id="fig52">
-<img src="images/p43.jpg" alt="" width="600" height="419" />
-<p class="pcap">Figure 52. <i>Layers of volcanic conglomerate separated by thin white tuff beds
-in Wiggins Formation. These cliffs, on the north side of Togwotee Pass, are
-about 1,100 feet high and represent a cross section of part of the enormous
-blanket of waterlaid debris that spread south and east from the Yellowstone-Absaroka
-volcanic area. These and younger deposits from the same general
-source filled the basins and almost completely buried the mountains in this
-part of Wyoming.</i></p>
-</div>
-<h3 id="c50">Volcanoes</h3>
-<p>Volcanoes are one of the most interesting parts of the
-geologic story of the Teton region. Although ash from distant
-volcanoes had settled in northwestern Wyoming at least
-as far back in time as Jurassic, the first nearby active volcanoes
-(since the Precambrian) erupted in the Yellowstone-Absaroka
-region during the early Eocene, about 50 million
-years ago. From then on, the volcanic area grew in size and
-the violence of eruptions and volume of debris increased
-until Pliocene time. This debris had a profound influence
-on the color and composition of the sediments and on the
-environment and types of plants and animals.</p>
-<p>The color of the volcanic rocks and the sediments
-derived from them varies significantly from one epoch to
-<span class="pb" id="Page_99">99</span>
-another. For example, the middle Eocene rocks are white
-to light-green, red, and purple, upper Eocene are dark-green,
-Oligocene are light-gray, white, and brown, Miocene
-are dark-green, brown, and gray, and Pliocene are white to
-red-brown.</p>
-<div class="img" id="fig53">
-<img src="images/p43a.jpg" alt="" width="600" height="434" />
-<p class="pcap">Figure 53. <i>Air oblique view south, showing the north end of the Teton
-Range disappearing beneath Pleistocene lava flows. Light-colored bare area
-at lower left is vertical Paleozoic limestone surrounded on three sides by
-nearly horizontal rhyolite lava flows. Bare slope at lower right is west-dipping
-Pinyon Conglomerate, also overlapped by lava. Grand Teton is on
-right skyline and Mt. Moran is rounded summit on middle skyline.</i></p>
-</div>
-<p>As mentioned earlier, it is probable that the vast outpouring
-of volcanic rocks during late Tertiary time in the
-Teton region and to the north and northeast is directly related
-to the subsidence of Jackson Hole and the rise of the
-Tetons.</p>
-<p>The spectacular banded cliffs of the Wiggins Formation
-on both sides of Togwotee Pass (<a href="#fig52">fig. 52</a>) and farther
-north in the Absaroka Range are remnants of Oligocene volcanic
-conglomerate and tuff that once spread as a blanket
-<span class="pb" id="Page_100">100</span>
-several thousand feet thick across eastern Jackson Hole and
-partially or completely buried the nearby older folded
-mountain ranges.</p>
-<div class="img" id="fig54">
-<img src="images/p44.jpg" alt="" width="600" height="350" />
-<p class="pcap">Figure 54. <i>Obsidian, a volcanic glass less than 10 million years old, especially
-prized by Indians who used it for spear and arrow points and for tools.</i></p>
-</div>
-<p>About 25 million years ago, with the start of the
-Miocene Epoch, volcanic vents opened up within, and along
-the borders of, Grand Teton National Park. Major centers
-of eruption were at the north end of the Teton Range, east
-of Jackson Lake, and south of Spread Creek. They emitted
-a prodigious amount of volcanic ash and fragments of congealed
-lava. For example, adjacent to one vent a mile in
-diameter, about 4 miles north-northeast of Jackson Lake
-Lodge, is a continuous section, 7,000 feet thick, of waterlaid
-strata derived in large part from this volcanic source.
-These sedimentary rocks comprise the Colter Formation
-which is darker colored and contains more iron and magnesium
-than the Wiggins Formation. The site of deposition
-at this locality was a north-trending trough that represented
-an early stage in the downwarping of Jackson Hole.</p>
-<p>Pliocene volcanoes erupted in southern and central
-Yellowstone Park. The volcanoes emitted viscous,
-frothy, pinkish-gray and brown lava called <i>rhyolite</i>. This
-is an extrusive igneous rock that has the same composition
-<span class="pb" id="Page_101">101</span>
-as granite, but is much finer grained. In several places,
-lava apparently flowed into the north end of Teewinot
-Lake, chilled suddenly, and solidified into a black volcanic
-glass called <i>obsidian</i>. Because it chips easily into
-thin flakes having a smooth surface, obsidian was prized
-by the Indians, who used it for spear and arrow points
-(<a href="#fig54">fig. 54</a>). Some of this obsidian has a potassium-argon
-date of 9 million years.</p>
-<div class="img" id="fig55">
-<img src="images/p44a.jpg" alt="" width="600" height="267" />
-<p class="pcap">Figure 55. <i>East face of Signal Mountain showing Bivouac Formation (upper
-Pliocene or Pleistocene). Tilted ledge is rhyolitic welded tuff 2.5 million
-years old, and slopes above and below it are conglomerate. National Park
-Service photo by W. E. Dilley.</i></p>
-</div>
-<p>After Teewinot Lake was filled with sediment, the
-floor of Jackson Hole became a flat boulder-covered surface.
-Nearby vents erupted heavy fiery clouds of gaseous
-molten rock that rolled across this plain and then congealed
-into hard layers with the general appearance of lava flows.
-Under a microscope, however, the rock is seen to be made
-up of compressed fragments of glass that matted down and
-solidified when the clouds stopped moving. This kind of
-rock is called a <i>welded tuff</i>. One of these forms the conspicuous
-ledge in the Bivouac Formation on the north and
-east sides of Signal Mountain (<a href="#fig55">fig. 55</a>), and is especially
-important because it has a potassium-argon date of 2.5
-million years. More of this <i>welded tuff</i> flowed southward
-from Yellowstone National Park, engulfed the north end
-of the Teton Range (<a href="#fig53">fig. 53</a>), and continued southward
-along the west side of the mountains for 35 miles and along
-the east side for 25 miles.</p>
-<div class="pb" id="Page_102">102</div>
-<div class="img" id="fig56">
-<img src="images/p45.jpg" alt="" width="600" height="733" />
-<p class="pcap">Figure 56. <i>The final 3 million years on our yardstick of time, enlarged to
-show approximate dates of major events.</i></p>
-</div>
-<table class="center" summary="">
-<tr><td class="c">THE LAST HUNDREDTHS OF AN INCH OF THE YARDSTICK </td><td class="c">ABSOLUTE TIME (Years ago) </td><td class="l">IMPORTANT EVENTS</td></tr>
-<tr><td class="c">0 </td><td class="c">0 </td><td class="l">Last glaciation followed by faulting</td></tr>
-<tr><td class="c">&sup1;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">50000 </td><td class="l">Second glaciation</td></tr>
-<tr><td class="c">&sup2;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">100000 </td><td class="l">?&mdash;First glaciation</td></tr>
-<tr><td class="c">&#8310;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">700000 </td><td class="l">?&mdash;Second Quaternary lake</td></tr>
-<tr><td class="c">&#8312;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">1 million </td><td class="l">?&mdash;Tilting and faulting of southern part of Jackson Hole</td></tr>
-<tr><td class="c">&sup1;&sup1;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">1.3 million </td><td class="l">?&mdash;First Quaternary lake</td></tr>
-<tr><td class="c">&sup1;&sup2;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">1.5 million </td><td class="l">} Complex series of volcanic eruptions in southern Jackson Hole</td></tr>
-<tr><td class="c">&sup1;&#8309;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">1.9 million </td><td class="l">}</td></tr>
-<tr><td class="c">&sup1;&#8310;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">2 million </td><td class="l">?&mdash;Development of Hoback normal fault</td></tr>
-<tr><td class="c">&sup2;/&#8321;&#8320;&#8320; </td><td class="c">2.5 million </td><td class="l">Eruption of welded tuff in Bivouac Formation</td></tr>
-<tr><td class="c">&sup2;&#8308;/&#8321;&#8320;&#8320;&#8320; </td><td class="c">3 million</td></tr>
-</table>
-<h2 id="c51"><br /><span class="small">QUATERNARY&mdash;TIME OF ICE, MORE LAKES, AND CONTINUED CRUSTAL DISTURBANCE</span></h2>
-<p>The Quaternary Period is represented by less than 15-thousandths
-of the last inch on our yardstick of time (<a href="#fig56">fig. 56</a>)
-and the entire Ice Age takes up less than 2-thousandths
-of an inch (less than the thickness of this page). Nevertheless,
-the spectacular effects of various forces of nature on
-the Teton landscape during this short interval of time are of
-such significance that they warrant a separate discussion.
-<span class="pb" id="Page_103">103</span>
-The role of glaciers in carving the rugged Teton peaks and
-shaping the adjacent valleys was mentioned in the first part
-of this booklet, but is discussed in more detail here. The
-magnitude and complexity of crustal movements increased
-during the final 2 million years of time&mdash;so much so that
-the beginning of Quaternary time has not yet been identified
-with any single event. <a href="#fig56">Figure 56</a> shows the major
-events described below.</p>
-<h3 id="c52">Hoback normal fault</h3>
-<p>The <i>Hoback normal fault</i>, 30 miles long, with a mile
-or more displacement, developed in the southernmost part
-of Jackson Hole about 2 million years ago. This fault is on
-the east side of the valley. Thus, the valley block was downdropped
-between this fault and the Teton fault that borders
-the west side.</p>
-<h3 id="c53">Volcanic activity</h3>
-<p>During or shortly after major movement on the Hoback
-fault, and perhaps related to it, there was a complex
-series of volcanic eruptions west and north of the town of
-Jackson, along the south boundary of the park. In rapid
-succession, lavas of many types, with a combined thickness
-of more than 1,000 feet, were extruded and volcanic plugs
-intruded into the near-surface sedimentary rocks. These
-volcanic rocks can be seen on the East and West Gros
-Ventre Buttes.</p>
-<p>There are no active volcanoes in the Teton region today
-and no postglacial lava flows or cinder cones. Five miles
-north of Grand Teton National Park are boiling springs
-(Flagg Ranch hot springs) that are associated with the
-youngest (late Quaternary) lavas in southern Yellowstone
-Park. Elsewhere in Jackson Hole are a number of lukewarm
-springs but their relation to volcanic rocks has not
-been determined.</p>
-<p>What happened to the vast thicknesses of volcanic debris?
-We know they existed because sections of them have
-been measured on the eroded edges of uptilted folds and
-fault blocks. Many cubic miles of these rocks are now
-buried beneath the floor of Jackson Hole, but a much greater
-volume was carried completely out of the region by water,
-<span class="pb" id="Page_104">104</span>
-ice, and wind during the final chapter of geologic
-history.</p>
-<h3 id="c54">Preglacial lakes</h3>
-<p>Remnants of two sets of lake deposits in Jackson Hole
-record preglacial events in Quaternary time. Downdropping
-of southern Jackson Hole along the Hoback and Teton
-faults blocked the southwestward drainage of the Snake
-River, and a new lake formed overlapping and extending
-south of the site of the long-vanished Teewinot Lake. Incorporated
-in the lake sediments are fragments of lava like
-that in nearby Quaternary flows. From this we know that
-the lake formed after at least some of the lava was emplaced.
-Apparently subsidence was more rapid than filling,
-for a time, at least, because this new lake was deep.
-Fossil snails preserved in olive-drab to gray fine-grained
-claystone overlying lava flows at the north end of East Gros
-Ventre Butte are the kind now living at depths of 120 to 300
-feet in Lake Tahoe, California-Nevada. Near the margins
-of the lake, pink and green claystone and soft sandstone
-were deposited. The duration of this lake is not known but
-it lasted long enough for 200 feet of beds to accumulate.
-Subsequent faulting and warping destroyed the lake, left
-tilted remnants of the beds perched 1,000 feet up on the
-east side of Jackson Hole, and permitted the Snake River to
-reestablish its course across the mountains to the southwest.</p>
-<p>Later downdropping of Jackson Hole impounded a
-second preglacial lake. Little is known about its extent because
-nearly everywhere the soft brown and gray shale,
-claystone, and sandstone deposited in it were scooped out
-and washed away during subsequent glaciations. A few
-remnants of the lake deposits are preserved in protected
-places, however; two are within the Gros Ventre River Valley&mdash;one
-downstream from Lower Slide Lake about a mile
-east of the park and the other 4 miles farther east. The latter
-remnant is nearly 500 feet thick and the upper half is
-largely very fine grained shale and claystone. This fine
-texture suggests that the lake existed for a good many thousand
-years, for such deposits commonly accumulate more
-slowly than coarser grained debris.</p>
-<div class="pb" id="Page_105">105</div>
-<div class="img" id="fig57">
-<img src="images/p46.jpg" alt="" width="600" height="513" />
-<p class="pcap">Figure 57. <i>Map showing extent and direction of movement of first and
-largest ice sheet. See <a href="#fig41">figure 41</a> for State lines and location map.</i></p>
-</div>
-<h3 id="c55">The Ice Age</h3>
-<p>With the uplift of the Teton Range and the formation
-of Jackson Hole late in Cenozoic time the landscape gradually
-began to assume the general outlines that we see today.
-Rain, wind, snow, and frost shaped the first crude
-approximations of the present ridges and peaks. Streams
-cut into the rising Teton fault block, eroding the ancestral
-canyons deeper and deeper as the uplift continued. The
-most recent great chapter in the story of the Teton landscape,
-however, remained to be written by the glaciers of
-the <i>Ice Age</i>.</p>
-<p>The reasons for the climatic changes that caused the
-Ice Age are still a matter of much scientific debate. Various
-theories have been advanced that attribute them to changes
-in solar radiation, changes in the earth&rsquo;s orbit and inclination
-<span class="pb" id="Page_106">106</span>
-to the sun, variations in the amount of carbon dioxide
-in the atmosphere, shifts in the positions of the continents
-or the poles, and to many other factors, but none has met
-with universal acceptance. No doubt the explanation lies in
-some unusual combination of circumstances, for widespread
-glaciation occurred only twice before in the earth&rsquo;s
-history&mdash;once in the late Precambrian and once during the
-Permian. It is quite clear, however, that the glaciers did
-not form in response to any local cause such as the uplift of
-the Teton Range, for concurrent climatic changes and ice
-advance took place throughout many parts of the world.</p>
-<p>At least three times in the last 250,000 years glaciers
-from the surrounding highlands invaded Jackson Hole. The
-oldest and most widespread glaciation probably took place
-about 200,000 years ago; it was called the <i>Buffalo Glaciation</i>
-by Prof. Eliot Blackwelder in 1915 (see selected
-references). The age estimate is based on measurements
-of the thickness of the decomposed layer on the surface of
-obsidian pebbles in the glacial debris. Major sources of ice
-were the Beartooth Mountains (<a href="#fig1">fig. 1</a>), the Absaroka
-Range, and the Wind River Range. The Gros Ventre Mountains
-and Teton Range furnished lesser amounts of ice.</p>
-<p>The ice from the Beartooth and Absaroka centers of
-ice accumulation converged in the northeastern part of
-Grand Teton National Park and flowed south along the face
-of the Teton Range in a giant stream that in many places
-was 2,000 feet thick (<a href="#fig57">fig. 57</a>). All but the highest parts
-of the Pinyon Peak and Mount Leidy Highlands were
-buried and scoured. Signal Mountain, Blacktail Butte, and
-the Gros Ventres Buttes were overridden and shaped by ice
-at this time. Another glacier, this one from the Wind River
-Range, flowed northwest along the Continental Divide, then
-down the Gros Ventre River Valley, and merged with the
-southward-moving main ice stream west of Lower Slide
-Lake. Where Jackson Hole narrows southward, the glacier
-became more and more confined, but nevertheless flowed
-all the way through the Snake River Canyon and on into
-Idaho.</p>
-<div class="pb" id="Page_107">107</div>
-<div class="img" id="fig58">
-<img src="images/p47.jpg" alt="" width="600" height="535" />
-<p class="pcap">Figure 58. <i>Glacial deposits, outwash, and loess exposed along Boyle Ditch in
-Jackson Hole National Elk Refuge. Indicated are middle Pliocene Teewinot
-formation (A), oldest till (B), Bull Lake outwash gravel (C), and post-Bull
-Lake loess (D), which here contains snail shells dated by Carbon-14 as 15,000
-years old. Height of cliff is about 30 feet.</i></p>
-</div>
-<p>The volume of this great ice mass was probably considerably
-more than 1,000 cubic miles. When it melted,
-nearly all the previously accumulated soil in Jackson Hole
-was washed away and a pavement of quartzite boulders
-mantled much of the glaciated surface. In areas not subsequently
-glaciated, the lack of soil and abundance of quartzite
-boulders drastically influenced the topography, later
-drainage, distribution of all types of vegetation, especially
-conifers and grass, and the pattern of human settlement and
-industry.</p>
-<div class="pb" id="Page_108">108</div>
-<div class="img" id="fig59">
-<img src="images/p48.jpg" alt="" width="600" height="411" />
-<p class="pcap">Figure 59. <i>View west from the Snake River overlook showing at upper right
-the Burned Ridge moraine (with trees) merging southward with the highest
-(oldest) Pinedale outwash plain. The next lower surface is composed of
-outwash from the Jackson Lake moraine which lies to the right, out of the
-picture. At the bottom is Deadman&rsquo;s Bar, a gravel deposit at the present
-river level. Photo by H. D. Pownall.</i></p>
-</div>
-<p>The second glaciation, named <i>Bull Lake</i>, was less
-than half as extensive as the first. A large tongue of ice
-from the Absaroka center of accumulation flowed down the
-Buffalo River Valley and joined ice from the Tetons on the
-floor of Jackson Hole. An enormous outwash fan of quartzite
-boulders extended from near Blacktail Butte southward
-throughout most of southern Jackson Hole. Glaciers in the
-Gros Ventre Mountains did not advance beyond the east
-margin of the valley floor. Carbon-14 ages and data from
-weathered obsidian pebbles suggest that this glaciation took
-place between 35,000 and 80,000 years ago.</p>
-<p>Bull Lake moraines and outwash deposits are overlain
-directly in the southern part of Jackson Hole by fine
-silt, rather than by deposits of the third glaciation (<a href="#fig58">fig. 58</a>).
-This silt, of windblown origin, is called <i>loess</i> and contains
-<span class="pb" id="Page_109">109</span>
-fossil shells dated by Carbon-14 as between 13,000 and
-19,000 years old. Wherever the loess occurs, it is marked
-by abundant modern coyote dens and badger burrows.</p>
-<div class="img" id="fig60">
-<img src="images/p48a.jpg" alt="" width="800" height="464" />
-<p class="pcap">Figure 60. <i>Air oblique view west toward the Teton Range, showing effects
-of Pinedale Glaciation on the landscape. Mt. Moran is at top left; the
-mountain front is broken by U-shaped valleys from which ice emerged into
-the area now occupied by Jackson Lake. The timbered area bordering
-Jackson Lake is the Jackson Lake moraine. One of the braided outlet
-channels breaching the Jackson Lake moraine can be seen crossing the outwash
-plain at the left center. Lakes at lower right occupy &ldquo;potholes&rdquo; near
-where the 9,000-year-old snail shells occur. Snake River is in foreground.
-Photo by R. L. Casebeer.</i></p>
-</div>
-<p>The third and last glaciation, named the <i>Pinedale</i>,
-was even less extensive than the others. Nevertheless it was
-of great importance for it added the final touches to the
-present landscape. The jagged intricately ice-carved peaks
-(<a href="#fig4">fig. 4</a>) and the glittering lakes and broad gravelly plains
-are vivid reminders of this recent chapter in geologic
-history.</p>
-<p>Pinedale glaciers advanced down Cascade, Garnet,
-Avalanche, and Death Canyons and spilled out onto the
-floor of Jackson Hole, where they built the outermost loops
-of the conspicuous terminal moraines that now encircle
-Jenny, Bradley, Taggart, and Phelps Lakes (<a href="#fig13">fig. 13</a>). Ice
-streams from Glacier Gulch and Open Canyon also left
-prominent moraines on the valley floor, but these do not
-contain lakes. Ice from Leigh Canyon and all of the eastward-draining
-valleys to the north combined to form a
-large glacier in roughly the present position of Jackson
-Lake. This ice entirely surrounded Signal Mountain, leaving
-only the upper few hundred feet projecting as an island
-or <i>nunatak</i>.</p>
-<div class="pb" id="Page_110">110</div>
-<div class="img" id="fig61">
-<img src="images/p49.jpg" alt="" width="600" height="923" />
-<p class="pcap">Figure 61. <i>The Pinedale Glaciers in the central part of Jackson Hole as they
-might have appeared at the time the Jackson Lake moraine was built. Solid
-color areas are lakes; dark irregular pattern shows areas of moraine deposited
-during the maximum advance of the Pinedale Glaciers. Pattern of
-open circles shows older Pinedale outwash plains; pattern of fine dots shows
-outwash plains built at the time the glaciers were in the positions shown in
-the drawing. Coarser dots near the margins of the glaciers represent concentrations
-of rock debris in the ice.</i></p>
-</div>
-<div class="pb" id="Page_111">111</div>
-<p>The southernmost major advance of Pinedale ice from
-Jackson Lake is marked by a series of densely timbered
-moraines that cross the Snake River Valley. This series is
-collectively named the <i>Burned Ridge moraine</i> (<a href="#fig61">fig. 61</a>).
-Extending southward for 10 miles from this moraine is a
-remarkably flat surfaced gravelly outwash deposit. It was
-spread by streams that poured from the glacier at the time
-the moraine was being built (<a href="#fig59">fig. 59</a>). East of the Snake
-River, the main highway from a point just north of Blacktail
-Butte to the Snake River overlook is built on this flat
-untimbered surface. We assume that the outwash is younger
-than 15,000 years because it apparently overlies loess of
-that age.</p>
-<p>The glacier withdrew rapidly northward from the
-Burned Ridge moraine, leaving behind many large irregular
-masses of stagnant, debris-covered ice. The sites of
-these became kettles, locally known as &ldquo;The Potholes&rdquo; (<a href="#fig12">fig. 12</a>).
-The main glacier retreated to a position marked by
-the loop of moraines just south of Jackson Lake (<a href="#fig60">fig. 60</a>).
-<a href="#fig61">Figure 61</a> is a sketch map showing how the glaciers in this
-part of Jackson Hole might have appeared at the time the
-Jackson Lake moraine was built.</p>
-<p>Abundant snail shells have been found in lake sediments
-in the bottoms of the kettles north of the Burned
-Ridge moraine (<a href="#fig60">fig. 60</a>) as well as on low ridges between
-them. Carbon-14 age determinations indicate that the snails
-lived about 9,000 years ago, either in a lake already present
-before the Pinedale ice advanced and formed the
-Burned Ridge moraine or in ponds that filled kettles left as
-the ice melted behind this moraine.</p>
-<p>In either case, the shells indicate that the Pinedale
-glaciers probably existed on the floor of Jackson Hole as
-<span class="pb" id="Page_112">112</span>
-recently as 9,000 years ago, at a time when Indians were
-already living in the area. We can easily imagine the fascination
-with which these primitive peoples may have
-watched as year after year the glaciers wasted away, slowly
-retreating back into the canyons, then withdrawing into the
-sheltered recesses of the high mountains, eventually to
-dwindle and disappear.</p>
-<p>Many bits of evidence, both from North America and
-Europe, indicate that there was a period called the <i>climatic
-optimum</i> about 6,000 years ago when the climate was
-significantly warmer and drier than at present. We suspect,
-though there is as yet no direct proof, that the Pinedale
-glaciers wasted away entirely during this interval.</p>
-<p>The modern pattern of vegetation in Jackson Hole is
-strongly influenced by the distribution of Pinedale glacial
-moraines and outwash deposits. Almost without exception
-the moraines are heavily forested, whereas the nearby outwash
-deposits are covered only by a sparse growth of sagebrush.
-This is probably because the moraines contain large
-amounts of clay and silt produced by the grinding action
-of the glaciers. Material of this type retains water much
-better and, because of the greater variety of chemical elements,
-is more fertile than the porous quartzite gravel and
-sand on the outwash plains.</p>
-<h3 id="c56">Modern glaciers</h3>
-<p>About a dozen small rapidly dwindling glaciers exist
-today in shaded reentrants high in the Teton Range. They
-are probably vestiges of ice masses built up since the climatic
-optimum, during the so-called &ldquo;<i>Little Ice Age</i>.&rdquo;
-These glaciers, while insignificant compared to those still
-present in many other mountain ranges, are fascinating
-working models of the great ice streams that shaped the
-Tetons during Pleistocene time.</p>
-<p>The Teton Glacier (<a href="#fig6">fig. 6</a>) is one of the best known.
-It is an ice body about 3,500 feet long and 1,100 feet wide
-that lies at the head of Glacier Gulch, shaded by the encircling
-ridges of the Grand Teton, Mount Owen, and
-Mount Teewinot. Ice in the central part is moving at a rate
-of more than 30 feet a year.</p>
-<div class="pb" id="Page_113">113</div>
-<h2 id="c57"><br /><span class="small">THE PRESENT AND THE FUTURE</span></h2>
-<p>The geologic story of the Teton country from the time
-the earth was new to the present day has been summarized.
-What can we learn from it? We become aware that events
-recorded in the rocks are not a chaotic jumble of random
-accidents but came in an orderly, logical succession. We
-see the majestic parade of life evolving from simple to complex
-types, overcoming all natural disasters, and adapting
-to ever-changing environments. We can only speculate as
-to the motivating force that launched this fascinating geologic
-and biologic venture and what the ultimate goal may
-be. New facts and new ideas are added to the story each
-year, but many unknown chapters remain to be studied;
-these offer an irresistible, continuing challenge to inquisitive
-minds, strong bodies, and restless, adventurous spirits.</p>
-<p>Most geologic processes that developed the Teton
-landscape have been beneficial to man; a few have interfered
-with his activities, cost him money, time, effort, and
-on occasion, his life. Postglacial faulting and tilting
-along the southern margin of Grand Teton National Park
-diverted drainage systems (such as Flat Creek, southwest
-of the Flat Creek fault on the south edge of the <a href="#fig62">geologic map</a>),
-raised hills, dropped valleys, and made steep slopes
-unstable. Flood-control engineers wage a never-ending
-struggle to keep the Snake River from shifting to the west
-side of Jackson Hole as the valley tilts westward in response
-to movement along the Teton fault. Each highway
-into Jackson Hole has been blocked by a landslide at one
-time or another and maintenance of roads across slide areas
-requires much ingenuity. We see one slide (the Gros Ventre)
-that blocked a river; larger slides have occurred in the
-past, and more can be expected. Abundant fresh fault
-scarps are a constant reminder that public buildings, campgrounds,
-dams, and roads need to be designed to withstand
-the effects of earthquakes. Some of these problems have
-geologic solutions; others can be avoided or minimized as
-further study increases our understanding of this region.</p>
-<div class="pb" id="Page_114">114</div>
-<p>Man appeared during the last one-fiftieth of an inch
-on our yardstick of time gone by. In this short span he has
-had more impact on the earth and its inhabitants than any
-other form of life. Will he use wisely the lessons of the
-past as a guide while he writes his record on the yardstick
-of the future?</p>
-<div class="pb" id="Page_115">115</div>
-<h2 id="c58"><br /><span class="small">APPENDIX</span></h2>
-<h3 id="c59">Acknowledgements</h3>
-<p>This booklet could not have been prepared without the
-cooperation and assistance of many individuals and organizations.
-We are indebted to the National Park Service for
-the use of facilities, equipment, and photographs, and for
-the enthusiasm and interest of all of the park staff. We
-especially appreciate the cooperation, advice, and assistance
-rendered by the late Fred C. Fagergren, former superintendent
-of Grand Teton National Park; Willard E.
-Dilley, former chief park naturalist; and R. Alan Mebane,
-former assistant chief park naturalist.</p>
-<p>Profs. Charles C. Bradley and John Montagne of
-Montana State University and Bruno J. Giletti of Brown
-University generously provided us with unpublished data.
-Cooperators during the years of background research were
-the late Dr. H. D. Thomas, State Geologist of Wyoming,
-and Dr. D. L. Blackstone, Jr., Chairman, Department of
-Geology, University of Wyoming.</p>
-<p>Helpful suggestions were made by many of our colleagues
-with the U.&nbsp;S. Geological Survey; S. S. Oriel, in
-particular, gave unstintingly of his time and talents in the
-review and revision of an early version of the manuscript.
-A later version had the further benefit of critical review by
-three other people, all experienced in presenting various
-types of scientific data to public groups: John M. Good,
-former chief park naturalist of Yellowstone National Park;
-Bryan Harry, former assistant chief park naturalist of
-Grand Teton National Park; and Richard Klinck, &ldquo;1965
-National Teacher of the Year.&rdquo;</p>
-<p>We are indebted to Ann C. Christiansen, Geologic
-Map Editor, for advice and guidance on the illustrations
-and to R. C. Fuhrmann and his staff for preparation of
-many of the line drawings. Block diagrams and photo
-artwork were prepared by J. R. Stacy and R. A. Reilly.
-All photographs without specific credit lines are by the
-authors. From the beginning of the Teton field study to
-editing and proofing of the final manuscript, our wives,
-Jane M. Love and Linda H. Reed, have been enthusiastic
-and indispensable participants.</p>
-<div class="pb" id="Page_116">116</div>
-<h3 id="c60">Selected references&mdash;if you wish to read further</h3>
-<dl class="undent"><dt>Blackwelder, Eliot, 1915, Post-Cretaceous history of the mountains of central western Wyoming: Jour. Geology, v. 23, p. 97-117, 193-217, 307-340.</dt>
-<dt>Bradley, F. H., 1873, Report on the geology of the Snake River district: U.S. Geol. Survey Terr. 6th Ann. Rept. (Hayden), p. 190-271.</dt>
-<dt>Edmund, R. W., 1951, Structural geology and physiography of the northern end of the Teton Range, Wyoming: Augustana Library Pub. 23, 82 p.</dt>
-<dt>Fryxell, F. M., 1930, Glacial features of Jackson Hole, Wyoming: Augustana Library Pub. 13, 129 p.</dt>
-<dt>&mdash;&mdash;, 1938, The Tetons, interpretations of a mountain landscape: Univ. California Press, Berkeley, Calif., 77 p.</dt>
-<dt>Hague, Arnold, 1904, Atlas to accompany U.S. Geol. Survey Monograph 32 on the geology of Yellowstone National Park.</dt>
-<dt>&mdash;&mdash;, Iddings, J. P., Weed, W. H., and others, 1899, Geology of the Yellowstone National Park: U.S. Geol. Survey Monograph 32, Pt. 2, 893 p.</dt>
-<dt>Harry, Bryan, 1963, Teton trails, a guide to the trails of Grand Teton National Park: Grand Teton Natural History Association, Moose, Wyo., 56 p.</dt>
-<dt>Horberg, Leland, 1938, The structural geology and physiography of the Teton Pass area, Wyoming: Augustana Library Pub. 16, 86 p.</dt>
-<dt>Hurley, P. M., 1959, How old is the earth?: Anchor Books, Garden City, N. Y., 160 p.</dt>
-<dt>Ortenburger, Leigh, 1965, A climber&rsquo;s guide to the Teton Range: Sierra Club, San Francisco, 336 p.</dt>
-<dt>St. John, O. H., 1883, Report on the geology of the Wind River district: U.S. Geol. Geog. Survey Terr. 12th Ann. Rept. (Hayden), Pt. 1, p. 173-270.</dt>
-<dt>Wyoming Geological Association, 1956, Guidebook, 11th annual field conf., Jackson Hole, Wyoming, 1956, Casper, Wyo., 256 p., incl. sketch maps, diagrams, tables, and illus., also geol. map, sections, and charts. Composed of a series of individual papers by various authors.</dt></dl>
-<div class="pb" id="Page_117">117</div>
-<h3 id="c61">About the authors</h3>
-<p>J. D. Love, a native of Wyoming, received his bachelor
-and master of arts degrees from the University of Wyoming
-and his doctor of philosophy degree from Yale University.
-His first field season in the Teton country, in 1933, was
-financed by the Geological Survey of Wyoming. After 12
-years of geologic work ranging from New England to Utah
-and Michigan to Mississippi, he returned to the Teton region.
-Beginning in 1945, he spent parts or all of 20 field
-seasons in and near the Tetons. He compiled the first geologic
-map of Teton County. He is the senior author of the
-geologic map of Wyoming, and author or co-author of more
-than 70 other published maps and papers on the geology of
-Wyoming. In 1961, the University of Wyoming awarded
-him an honorary doctor of laws degree for his work on
-uranium deposits that &ldquo;led to the development of the uranium
-industry in Wyoming.&rdquo; The Wyoming Geological Association
-made him an honorary life member and gave him a
-special award for his geologic studies of the Teton area. He
-is a Fellow of the Geological Society of America and is
-active in various other geological organizations, as well as
-having been president of the Wyoming Chapters of Sigma
-Xi (scientific honorary) and Phi Beta Kappa (scholastic
-honorary) societies.</p>
-<p>John C. Reed, Jr., joined the U.S. Geological Survey in
-1953 after receiving his doctor of philosophy degree from
-the John Hopkins University. His principal geologic work
-before coming to the Teton region was in Alaska and in the
-southern Appalachians. Beginning in 1961, he spent five
-field seasons studying and mapping the Precambrian
-rocks in Grand Teton National Park, including all the high
-peaks in the Teton Range. He is a noted mountaineer, a Fellow
-of the Geological Society of America, a member of the
-Arctic Institute of North America, and the American Alpine
-Club. His numerous publications, in addition to those on
-the Tetons, describe the geology of mountainous areas in
-Alaska, the Appalachians, and Utah.</p>
-<div class="pb" id="Page_118">118</div>
-<h2 id="c62"><br /><span class="small"><span class="center">Index of selected terms and features</span></span></h2>
-<p class="center"><a href="#index_A" class="ab">A</a> <a href="#index_B" class="ab">B</a> <a href="#index_C" class="ab">C</a> <a href="#index_D" class="ab">D</a> <a href="#index_E" class="ab">E</a> <a href="#index_F" class="ab">F</a> <a href="#index_G" class="ab">G</a> <a href="#index_H" class="ab">H</a> <a href="#index_I" class="ab">I</a> <a href="#index_J" class="ab">J</a> <a href="#index_K" class="ab">K</a> <a href="#index_L" class="ab">L</a> <a href="#index_M" class="ab">M</a> <a href="#index_N" class="ab">N</a> <a href="#index_O" class="ab">O</a> <a href="#index_P" class="ab">P</a> <a href="#index_Q" class="ab">Q</a> <a href="#index_R" class="ab">R</a> <a href="#index_S" class="ab">S</a> <a href="#index_T" class="ab">T</a> <span class="ab">U</span> <span class="ab">V</span> <a href="#index_W" class="ab">W</a> <span class="ab">X</span> <span class="ab">Y</span> <span class="ab">Z</span></p>
-<dl class="index">
-<dt><i><b>Term</b></i><span class="jr"> <i><b>Defined or described on page</b></i></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_A"><b>A</b></dt>
-<dt>amphibolite<span class="jr"> <a href="#Page_51">51</a></span></dt>
-<dt>anticlines<span class="jr"> <a href="#Page_85">85</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_B"><b>B</b></dt>
-<dt>badlands<span class="jr"> <a href="#Page_14">14</a></span></dt>
-<dt>bentonite<span class="jr"> <a href="#Page_81">81</a></span></dt>
-<dt>biotite<span class="jr"> <a href="#Page_51">51</a></span></dt>
-<dt>brachiopods<span class="jr"> <a href="#Page_70">70</a></span></dt>
-<dt>Buffalo Glaciation<span class="jr"> <a href="#Page_106">106</a></span></dt>
-<dt>Bull Lake Glaciation<span class="jr"> <a href="#Page_108">108</a></span></dt>
-<dt>Burned Ridge moraine<span class="jr"> <a href="#Page_111">111</a></span></dt>
-<dt>buttes<span class="jr"> <a href="#Page_18">18</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_C"><b>C</b></dt>
-<dt>Carbon-14<span class="jr"> <a href="#Page_48">48</a></span></dt>
-<dt>carnivores<span class="jr"> <a href="#Page_95">95</a></span></dt>
-<dt>chlorite<span class="jr"> <a href="#Page_56">56</a></span></dt>
-<dt>cirque<span class="jr"> <a href="#Page_30">30</a></span></dt>
-<dt>climatic optimum<span class="jr"> <a href="#Page_112">112</a></span></dt>
-<dt>Cordilleran trough<span class="jr"> <a href="#Page_69">69</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_D"><b>D</b></dt>
-<dt>diabase<span class="jr"> <a href="#Page_59">59</a></span></dt>
-<dt>dikes<span class="jr"> <a href="#Page_56">56</a></span></dt>
-<dt>dipping<span class="jr"> <a href="#Page_39">39</a></span></dt>
-<dt>dolomite<span class="jr"> <a href="#Page_75">75</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_E"><b>E</b></dt>
-<dt>&ldquo;edgewise&rdquo; conglomerate<span class="jr"> <a href="#Page_73">73</a></span></dt>
-<dt>epochs<span class="jr"> <a href="#Page_46">46</a></span></dt>
-<dt>eras<span class="jr"> <a href="#Page_46">46</a></span></dt>
-<dt>erosion<span class="jr"> <a href="#Page_27">27</a></span></dt>
-<dt>erratics<span class="jr"> <a href="#Page_31">31</a></span></dt>
-<dt>extrusive igneous rocks<span class="jr"> <a href="#Page_46">46</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_F"><b>F</b></dt>
-<dt>fault<span class="jr"> <a href="#Page_9">9</a></span></dt>
-<dt>fault block mountain range<span class="jr"> <a href="#Page_37">37</a></span></dt>
-<dt>fault scarps<span class="jr"> <a href="#Page_37">37</a></span></dt>
-<dt>formations<span class="jr"> <a href="#Page_66">66</a></span></dt>
-<dt>frost wedging<span class="jr"> <a href="#Page_25">25</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_G"><b>G</b></dt>
-<dt>geologic<span class="jr"> <a href="#Page_10">10</a></span></dt>
-<dt>glacial striae<span class="jr"> <a href="#Page_30">30</a></span></dt>
-<dt>gradients<span class="jr"> <a href="#Page_28">28</a></span></dt>
-<dt>Grand Valley Lake<span class="jr"> <a href="#Page_95">95</a></span></dt>
-<dt>granite<span class="jr"> <a href="#Page_55">55</a></span></dt>
-<dt>granite gneiss<span class="jr"> <a href="#Page_54">54</a></span></dt>
-<dt>groups<span class="jr"> <a href="#Page_47">47</a></span></dt>
-<dt>gypsum<span class="jr"> <a href="#Page_79">79</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_H"><b>H</b></dt>
-<dt>herbivores<span class="jr"> <a href="#Page_95">95</a></span></dt>
-<dt>Hoback normal fault<span class="jr"> <a href="#Page_103">103</a></span></dt>
-<dt>hole<span class="jr"> <a href="#Page_8">8</a></span></dt>
-<dt>hornblende<span class="jr"> <a href="#Page_51">51</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_I"><b>I</b></dt>
-<dt>Ice Age<span class="jr"> <a href="#Page_105">105</a></span></dt>
-<dt>igneous rocks<span class="jr"> <a href="#Page_46">46</a></span></dt>
-<dt>intrusive igneous rocks<span class="jr"> <a href="#Page_46">46</a></span></dt>
-</dl>
-<div class="pb" id="Page_119">119</div>
-<dl class="index">
-<dt class="center" id="index_J"><b>J</b></dt>
-<dt>Jackson Hole<span class="jr"> <a href="#Page_8">8</a></span></dt>
-<dt>jade<span class="jr"> <a href="#Page_55">55</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_K"><b>K</b></dt>
-<dt>kettle<span class="jr"> <a href="#Page_31">31</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_L"><b>L</b></dt>
-<dt>Laramide Revolution<span class="jr"> <a href="#Page_82">82</a></span></dt>
-<dt>lateral moraine<span class="jr"> <a href="#Page_30">30</a></span></dt>
-<dt>layered gneisses<span class="jr"> <a href="#Page_51">51</a></span></dt>
-<dt>Little Ice Age<span class="jr"> <a href="#Page_112">112</a></span></dt>
-<dt>loess<span class="jr"> <a href="#Page_108">108</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_M"><b>M</b></dt>
-<dt>magma<span class="jr"> <a href="#Page_60">60</a></span></dt>
-<dt>magnetite<span class="jr"> <a href="#Page_52">52</a></span></dt>
-<dt>marine sedimentary rocks<span class="jr"> <a href="#Page_21">21</a></span></dt>
-<dt>metamorphic rocks<span class="jr"> <a href="#Page_53">53</a></span></dt>
-<dt>muscovite<span class="jr"> <a href="#Page_55">55</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_N"><b>N</b></dt>
-<dt>normal fault<span class="jr"> <a href="#Page_39">39</a></span></dt>
-<dt>nunatak<span class="jr"> <a href="#Page_111">111</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_O"><b>O</b></dt>
-<dt>obsidian<span class="jr"> <a href="#Page_101">101</a></span></dt>
-<dt>oreodonts<span class="jr"> <a href="#Page_97">97</a></span></dt>
-<dt>outwash<span class="jr"> <a href="#Page_31">31</a></span></dt>
-<dt>outwash plain<span class="jr"> <a href="#Page_31">31</a></span></dt>
-<dt>outwash terraces<span class="jr"> <a href="#Page_34">34</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_P"><b>P</b></dt>
-<dt>pegmatite<span class="jr"> <a href="#Page_56">56</a></span></dt>
-<dt>period<span class="jr"> <a href="#Page_46">46</a></span></dt>
-<dt>Pinedale Glaciation<span class="jr"> <a href="#Page_109">109</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_Q"><b>Q</b></dt>
-<dt>quartzite<span class="jr"> <a href="#Page_63">63</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_R"><b>R</b></dt>
-<dt>reverse fault<span class="jr"> <a href="#Page_39">39</a></span></dt>
-<dt>rhyolite<span class="jr"> <a href="#Page_100">100</a></span></dt>
-<dt>rock glaciers<span class="jr"> <a href="#Page_26">26</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_S"><b>S</b></dt>
-<dt>schist<span class="jr"> <a href="#Page_51">51</a></span></dt>
-<dt>sedimentary rocks<span class="jr"> <a href="#Page_45">45</a></span></dt>
-<dt>series<span class="jr"> <a href="#Page_47">47</a></span></dt>
-<dt>serpentine<span class="jr"> <a href="#Page_55">55</a></span></dt>
-<dt>&ldquo;soapstone&rdquo;<span class="jr"> <a href="#Page_55">55</a></span></dt>
-<dt>Sundance Sea<span class="jr"> <a href="#Page_79">79</a></span></dt>
-<dt>systems<span class="jr"> <a href="#Page_46">46</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_T"><b>T</b></dt>
-<dt>talus<span class="jr"> <a href="#Page_24">24</a></span></dt>
-<dt>Targhee uplift<span class="jr"> <a href="#Page_83">83</a></span></dt>
-<dt>Teewinot Lake<span class="jr"> <a href="#Page_92">92</a></span></dt>
-<dt>terminal moraine<span class="jr"> <a href="#Page_30">30</a></span></dt>
-<dt>Tetons<span class="jr"> <a href="#Page_8">8</a></span></dt>
-<dt>Teton fault<span class="jr"> <a href="#Page_37">37</a></span></dt>
-<dt>thrust fault<span class="jr"> <a href="#Page_39">39</a></span></dt>
-<dt>timberline<span class="jr"> <a href="#Page_15">15</a></span></dt>
-<dt>titanothere<span class="jr"> <a href="#Page_97">97</a></span></dt>
-<dt>treeline<span class="jr"> <a href="#Page_15">15</a></span></dt>
-<dt>Triceratops<span class="jr"> <a href="#Page_85">85</a></span></dt>
-<dt>trilobites<span class="jr"> <a href="#Page_70">70</a></span></dt>
-<dt>tuff<span class="jr"> <a href="#Page_92">92</a></span></dt>
-</dl>
-<dl class="index">
-<dt class="center" id="index_W"><b>W</b></dt>
-<dt>welded tuff<span class="jr"> <a href="#Page_101">101</a></span></dt>
-</dl>
-<div class="pb" id="Page_120">120</div>
-<h2 id="c63"><br /><span class="small">The GRAND TETON NATURAL HISTORY ASSOCIATION</span></h2>
-<p>The Grand Teton Natural History Association
-assists the National Park Service in
-the development of a broad public understanding
-of the geology, plant and animal
-life, history, and related subjects pertaining
-to Grand Teton National Park. It aids
-in the development of museums and wayside
-exhibits, offers for sale publications on
-natural and human history, and cooperates
-with the Government in the interest of
-Grand Teton National Park.</p>
-<p><i>Mail orders</i>: For a publication list, write
-the Grand Teton Natural History Association,
-Moose, Wyoming 83012.</p>
-<table class="center" summary="">
-<tr><td class="r"><i>Creative Director</i>: </td><td class="l">Century III Advertising. Inc.</td></tr>
-<tr><td class="r"><i>Designer</i>: </td><td class="l">Les Hays Studios, Inc.</td></tr>
-<tr><td class="r"><i>Color Separations</i>&mdash;<i>Assembly</i>&mdash;<i>Plates</i>: </td><td class="l">Orent Graphic Arts, Inc.</td></tr>
-<tr><td class="r"><i>Type</i>: </td><td class="l">Bodoni and Gothic</td></tr>
-<tr><td class="r"><i>Printer</i>: </td><td class="l">Omaha Printing Co.</td></tr>
-<tr><td class="r"><i>Printing</i>: </td><td class="l">Offset Lithography.</td></tr>
-<tr><td class="r"> </td><td class="l">Six Colors on Covers</td></tr>
-<tr><td class="r"> </td><td class="l">Two Colors on Body</td></tr>
-</table>
-<div class="pb" id="Page_121">121</div>
-<div class="img" id="fig62">
-<img src="images/map2_lr.jpg" alt="" width="600" height="808" />
-<p class="pcap">GEOLOGIC MAP OF GRAND TETON NATIONAL PARK<br /><span class="center"><a class="abl" href="images/map2_hr.jpg">High-resolution Map</a></span></p>
-</div>
-<div class="img" id="pic2">
-<img src="images/p50a.jpg" alt="" width="600" height="679" />
-<p class="pcap">EXPLANATION</p>
-</div>
-<dl class="undent"><dt>CENOZOIC</dt>
-<dd>QUATERNARY</dd>
-<dd class="t">Sand, gravel, and talus</dd>
-<dd class="t2"><i>Includes glacial outwash and materials deposited by present streams</i></dd>
-<dd class="t">Landslide deposits</dd>
-<dd class="t">Moraine deposits of Pinedale glaciers</dd>
-<dd class="t">Moraine deposits of Bull Lake and older glaciers</dd>
-<dd>TERTIARY</dd>
-<dd class="t">Volcanic rocks</dd>
-<dd class="t2"><i>Lava flows and volcanic ash</i></dd>
-<dd class="t">Conglomerate, sandstone, shale, claystone, marl, and pumice</dd>
-<dd class="t2"><i>Deposited on land or in shallow lakes</i></dd>
-<dt>MESOZOIC</dt>
-<dd>Conglomerate, sandstone, shale, and coal</dd>
-<dd class="t"><i>Deposited on land</i></dd>
-<dd>Shale, sandstone, and limestone</dd>
-<dd class="t"><i>Mostly deposited in shallow seas</i></dd>
-<dt>PALEOZOIC</dt>
-<dd>Limestone, shale, and sandstone</dd>
-<dd class="t"><i>Deposited in shallow seas</i></dd>
-<dt>PRECAMBRIAN</dt>
-<dd>Diabase dikes</dd>
-<dd>Granite, gneiss, and schist</dd>
-<dt>Fault</dt>
-<dd><i>Dashed where approximately located; dotted where concealed beneath unfaulted younger deposits. U is on the side that moved up; D, on the side that moved down</i></dd>
-<dt>Geologic contact</dt></dl>
-<div class="img" id="pic3">
-<img src="images/p59.jpg" alt="" width="1000" height="598" />
-<p class="pcap">View southwest from Lake Solitude toward the
-Grand Teton (right), Mt. Owen, and Mt. Teewinot.
-<b><i>Wyoming Travel Commission photo
-by J. R. Simon.</i></b></p>
-</div>
-<div class="img" id="pic4">
-<img src="images/p61.jpg" alt="" width="643" height="1001" />
-<p class="pcap">Grand Teton, Mt. Owen, and Mt. Teewinot from
-Jenny Lake Flat. <b><i>National Park Service photo
-by W. E. Dilley.</i></b></p>
-</div>
-<h2>Transcriber&rsquo;s Notes</h2>
-<ul><li>Retained publication information from the printed edition: this eBook is public-domain in the country of publication.</li>
-<li>Corrected a few palpable typos.</li>
-<li>Re-arranged text in captions closer to the corresponding image.</li>
-<li>Expanded ambiguous references to illustrations, <i>e.g.</i> &ldquo;Figure D&rdquo; to  &ldquo;Figure 16D&rdquo;</li>
-<li>Added one section heading, &ldquo;The First Big Lake&rdquo; to match the table of contents.</li>
-<li>Included a transcription of the text within some images, with estimated scale readings from charts.</li>
-<li>In the text versions only, text in italics is delimited by _underscores_.</li></ul>
-
-
-
-
-
-
-
-<pre>
-
-
-
-
-
-End of the Project Gutenberg EBook of Creation of the Teton Landscape, by 
-J. D. Love and John C. Reed
-
-*** END OF THIS PROJECT GUTENBERG EBOOK CREATION OF THE TETON LANDSCAPE ***
-
-***** This file should be named 52838-h.htm or 52838-h.zip *****
-This and all associated files of various formats will be found in:
-        http://www.gutenberg.org/5/2/8/3/52838/
-
-Produced by Stephen Hutcheson, Dave Morgan and the Online
-Distributed Proofreading Team at http://www.pgdp.net
-
-Updated editions will replace the previous one--the old editions will
-be renamed.
-
-Creating the works from print editions not protected by U.S. copyright
-law means that no one owns a United States copyright in these works,
-so the Foundation (and you!) can copy and distribute it in the United
-States without permission and without paying copyright
-royalties. Special rules, set forth in the General Terms of Use part
-of this license, apply to copying and distributing Project
-Gutenberg-tm electronic works to protect the PROJECT GUTENBERG-tm
-concept and trademark. Project Gutenberg is a registered trademark,
-and may not be used if you charge for the eBooks, unless you receive
-specific permission. If you do not charge anything for copies of this
-eBook, complying with the rules is very easy. You may use this eBook
-for nearly any purpose such as creation of derivative works, reports,
-performances and research. They may be modified and printed and given
-away--you may do practically ANYTHING in the United States with eBooks
-not protected by U.S. copyright law. Redistribution is subject to the
-trademark license, especially commercial redistribution.
-
-START: FULL LICENSE
-
-THE FULL PROJECT GUTENBERG LICENSE
-PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK
-
-To protect the Project Gutenberg-tm mission of promoting the free
-distribution of electronic works, by using or distributing this work
-(or any other work associated in any way with the phrase "Project
-Gutenberg"), you agree to comply with all the terms of the Full
-Project Gutenberg-tm License available with this file or online at
-www.gutenberg.org/license.
-
-Section 1. General Terms of Use and Redistributing Project
-Gutenberg-tm electronic works
-
-1.A. By reading or using any part of this Project Gutenberg-tm
-electronic work, you indicate that you have read, understand, agree to
-and accept all the terms of this license and intellectual property
-(trademark/copyright) agreement. If you do not agree to abide by all
-the terms of this agreement, you must cease using and return or
-destroy all copies of Project Gutenberg-tm electronic works in your
-possession. If you paid a fee for obtaining a copy of or access to a
-Project Gutenberg-tm electronic work and you do not agree to be bound
-by the terms of this agreement, you may obtain a refund from the
-person or entity to whom you paid the fee as set forth in paragraph
-1.E.8.
-
-1.B. "Project Gutenberg" is a registered trademark. It may only be
-used on or associated in any way with an electronic work by people who
-agree to be bound by the terms of this agreement. There are a few
-things that you can do with most Project Gutenberg-tm electronic works
-even without complying with the full terms of this agreement. See
-paragraph 1.C below. There are a lot of things you can do with Project
-Gutenberg-tm electronic works if you follow the terms of this
-agreement and help preserve free future access to Project Gutenberg-tm
-electronic works. See paragraph 1.E below.
-
-1.C. The Project Gutenberg Literary Archive Foundation ("the
-Foundation" or PGLAF), owns a compilation copyright in the collection
-of Project Gutenberg-tm electronic works. Nearly all the individual
-works in the collection are in the public domain in the United
-States. If an individual work is unprotected by copyright law in the
-United States and you are located in the United States, we do not
-claim a right to prevent you from copying, distributing, performing,
-displaying or creating derivative works based on the work as long as
-all references to Project Gutenberg are removed. Of course, we hope
-that you will support the Project Gutenberg-tm mission of promoting
-free access to electronic works by freely sharing Project Gutenberg-tm
-works in compliance with the terms of this agreement for keeping the
-Project Gutenberg-tm name associated with the work. You can easily
-comply with the terms of this agreement by keeping this work in the
-same format with its attached full Project Gutenberg-tm License when
-you share it without charge with others.
-
-1.D. The copyright laws of the place where you are located also govern
-what you can do with this work. Copyright laws in most countries are
-in a constant state of change. If you are outside the United States,
-check the laws of your country in addition to the terms of this
-agreement before downloading, copying, displaying, performing,
-distributing or creating derivative works based on this work or any
-other Project Gutenberg-tm work. The Foundation makes no
-representations concerning the copyright status of any work in any
-country outside the United States.
-
-1.E. Unless you have removed all references to Project Gutenberg:
-
-1.E.1. The following sentence, with active links to, or other
-immediate access to, the full Project Gutenberg-tm License must appear
-prominently whenever any copy of a Project Gutenberg-tm work (any work
-on which the phrase "Project Gutenberg" appears, or with which the
-phrase "Project Gutenberg" is associated) is accessed, displayed,
-performed, viewed, copied or distributed:
-
-  This eBook is for the use of anyone anywhere in the United States and
-  most other parts of the world at no cost and with almost no
-  restrictions whatsoever. You may copy it, give it away or re-use it
-  under the terms of the Project Gutenberg License included with this
-  eBook or online at www.gutenberg.org. If you are not located in the
-  United States, you'll have to check the laws of the country where you
-  are located before using this ebook.
-
-1.E.2. If an individual Project Gutenberg-tm electronic work is
-derived from texts not protected by U.S. copyright law (does not
-contain a notice indicating that it is posted with permission of the
-copyright holder), the work can be copied and distributed to anyone in
-the United States without paying any fees or charges. If you are
-redistributing or providing access to a work with the phrase "Project
-Gutenberg" associated with or appearing on the work, you must comply
-either with the requirements of paragraphs 1.E.1 through 1.E.7 or
-obtain permission for the use of the work and the Project Gutenberg-tm
-trademark as set forth in paragraphs 1.E.8 or 1.E.9.
-
-1.E.3. If an individual Project Gutenberg-tm electronic work is posted
-with the permission of the copyright holder, your use and distribution
-must comply with both paragraphs 1.E.1 through 1.E.7 and any
-additional terms imposed by the copyright holder. Additional terms
-will be linked to the Project Gutenberg-tm License for all works
-posted with the permission of the copyright holder found at the
-beginning of this work.
-
-1.E.4. Do not unlink or detach or remove the full Project Gutenberg-tm
-License terms from this work, or any files containing a part of this
-work or any other work associated with Project Gutenberg-tm.
-
-1.E.5. Do not copy, display, perform, distribute or redistribute this
-electronic work, or any part of this electronic work, without
-prominently displaying the sentence set forth in paragraph 1.E.1 with
-active links or immediate access to the full terms of the Project
-Gutenberg-tm License.
-
-1.E.6. You may convert to and distribute this work in any binary,
-compressed, marked up, nonproprietary or proprietary form, including
-any word processing or hypertext form. However, if you provide access
-to or distribute copies of a Project Gutenberg-tm work in a format
-other than "Plain Vanilla ASCII" or other format used in the official
-version posted on the official Project Gutenberg-tm web site
-(www.gutenberg.org), you must, at no additional cost, fee or expense
-to the user, provide a copy, a means of exporting a copy, or a means
-of obtaining a copy upon request, of the work in its original "Plain
-Vanilla ASCII" or other form. Any alternate format must include the
-full Project Gutenberg-tm License as specified in paragraph 1.E.1.
-
-1.E.7. Do not charge a fee for access to, viewing, displaying,
-performing, copying or distributing any Project Gutenberg-tm works
-unless you comply with paragraph 1.E.8 or 1.E.9.
-
-1.E.8. You may charge a reasonable fee for copies of or providing
-access to or distributing Project Gutenberg-tm electronic works
-provided that
-
-* You pay a royalty fee of 20% of the gross profits you derive from
-  the use of Project Gutenberg-tm works calculated using the method
-  you already use to calculate your applicable taxes. The fee is owed
-  to the owner of the Project Gutenberg-tm trademark, but he has
-  agreed to donate royalties under this paragraph to the Project
-  Gutenberg Literary Archive Foundation. Royalty payments must be paid
-  within 60 days following each date on which you prepare (or are
-  legally required to prepare) your periodic tax returns. Royalty
-  payments should be clearly marked as such and sent to the Project
-  Gutenberg Literary Archive Foundation at the address specified in
-  Section 4, "Information about donations to the Project Gutenberg
-  Literary Archive Foundation."
-
-* You provide a full refund of any money paid by a user who notifies
-  you in writing (or by e-mail) within 30 days of receipt that s/he
-  does not agree to the terms of the full Project Gutenberg-tm
-  License. You must require such a user to return or destroy all
-  copies of the works possessed in a physical medium and discontinue
-  all use of and all access to other copies of Project Gutenberg-tm
-  works.
-
-* You provide, in accordance with paragraph 1.F.3, a full refund of
-  any money paid for a work or a replacement copy, if a defect in the
-  electronic work is discovered and reported to you within 90 days of
-  receipt of the work.
-
-* You comply with all other terms of this agreement for free
-  distribution of Project Gutenberg-tm works.
-
-1.E.9. If you wish to charge a fee or distribute a Project
-Gutenberg-tm electronic work or group of works on different terms than
-are set forth in this agreement, you must obtain permission in writing
-from both the Project Gutenberg Literary Archive Foundation and The
-Project Gutenberg Trademark LLC, the owner of the Project Gutenberg-tm
-trademark. Contact the Foundation as set forth in Section 3 below.
-
-1.F.
-
-1.F.1. Project Gutenberg volunteers and employees expend considerable
-effort to identify, do copyright research on, transcribe and proofread
-works not protected by U.S. copyright law in creating the Project
-Gutenberg-tm collection. Despite these efforts, Project Gutenberg-tm
-electronic works, and the medium on which they may be stored, may
-contain "Defects," such as, but not limited to, incomplete, inaccurate
-or corrupt data, transcription errors, a copyright or other
-intellectual property infringement, a defective or damaged disk or
-other medium, a computer virus, or computer codes that damage or
-cannot be read by your equipment.
-
-1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES - Except for the "Right
-of Replacement or Refund" described in paragraph 1.F.3, the Project
-Gutenberg Literary Archive Foundation, the owner of the Project
-Gutenberg-tm trademark, and any other party distributing a Project
-Gutenberg-tm electronic work under this agreement, disclaim all
-liability to you for damages, costs and expenses, including legal
-fees. YOU AGREE THAT YOU HAVE NO REMEDIES FOR NEGLIGENCE, STRICT
-LIABILITY, BREACH OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE
-PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE FOUNDATION, THE
-TRADEMARK OWNER, AND ANY DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE
-LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT, CONSEQUENTIAL, PUNITIVE OR
-INCIDENTAL DAMAGES EVEN IF YOU GIVE NOTICE OF THE POSSIBILITY OF SUCH
-DAMAGE.
-
-1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you discover a
-defect in this electronic work within 90 days of receiving it, you can
-receive a refund of the money (if any) you paid for it by sending a
-written explanation to the person you received the work from. If you
-received the work on a physical medium, you must return the medium
-with your written explanation. The person or entity that provided you
-with the defective work may elect to provide a replacement copy in
-lieu of a refund. If you received the work electronically, the person
-or entity providing it to you may choose to give you a second
-opportunity to receive the work electronically in lieu of a refund. If
-the second copy is also defective, you may demand a refund in writing
-without further opportunities to fix the problem.
-
-1.F.4. Except for the limited right of replacement or refund set forth
-in paragraph 1.F.3, this work is provided to you 'AS-IS', WITH NO
-OTHER WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED, INCLUDING BUT NOT
-LIMITED TO WARRANTIES OF MERCHANTABILITY OR FITNESS FOR ANY PURPOSE.
-
-1.F.5. Some states do not allow disclaimers of certain implied
-warranties or the exclusion or limitation of certain types of
-damages. If any disclaimer or limitation set forth in this agreement
-violates the law of the state applicable to this agreement, the
-agreement shall be interpreted to make the maximum disclaimer or
-limitation permitted by the applicable state law. The invalidity or
-unenforceability of any provision of this agreement shall not void the
-remaining provisions.
-
-1.F.6. INDEMNITY - You agree to indemnify and hold the Foundation, the
-trademark owner, any agent or employee of the Foundation, anyone
-providing copies of Project Gutenberg-tm electronic works in
-accordance with this agreement, and any volunteers associated with the
-production, promotion and distribution of Project Gutenberg-tm
-electronic works, harmless from all liability, costs and expenses,
-including legal fees, that arise directly or indirectly from any of
-the following which you do or cause to occur: (a) distribution of this
-or any Project Gutenberg-tm work, (b) alteration, modification, or
-additions or deletions to any Project Gutenberg-tm work, and (c) any
-Defect you cause.
-
-Section 2. Information about the Mission of Project Gutenberg-tm
-
-Project Gutenberg-tm is synonymous with the free distribution of
-electronic works in formats readable by the widest variety of
-computers including obsolete, old, middle-aged and new computers. It
-exists because of the efforts of hundreds of volunteers and donations
-from people in all walks of life.
-
-Volunteers and financial support to provide volunteers with the
-assistance they need are critical to reaching Project Gutenberg-tm's
-goals and ensuring that the Project Gutenberg-tm collection will
-remain freely available for generations to come. In 2001, the Project
-Gutenberg Literary Archive Foundation was created to provide a secure
-and permanent future for Project Gutenberg-tm and future
-generations. To learn more about the Project Gutenberg Literary
-Archive Foundation and how your efforts and donations can help, see
-Sections 3 and 4 and the Foundation information page at
-www.gutenberg.org
-
-
-
-Section 3. Information about the Project Gutenberg Literary Archive Foundation
-
-The Project Gutenberg Literary Archive Foundation is a non profit
-501(c)(3) educational corporation organized under the laws of the
-state of Mississippi and granted tax exempt status by the Internal
-Revenue Service. The Foundation's EIN or federal tax identification
-number is 64-6221541. Contributions to the Project Gutenberg Literary
-Archive Foundation are tax deductible to the full extent permitted by
-U.S. federal laws and your state's laws.
-
-The Foundation's principal office is in Fairbanks, Alaska, with the
-mailing address: PO Box 750175, Fairbanks, AK 99775, but its
-volunteers and employees are scattered throughout numerous
-locations. Its business office is located at 809 North 1500 West, Salt
-Lake City, UT 84116, (801) 596-1887. Email contact links and up to
-date contact information can be found at the Foundation's web site and
-official page at www.gutenberg.org/contact
-
-For additional contact information:
-
-    Dr. Gregory B. Newby
-    Chief Executive and Director
-    gbnewby@pglaf.org
-
-Section 4. Information about Donations to the Project Gutenberg
-Literary Archive Foundation
-
-Project Gutenberg-tm depends upon and cannot survive without wide
-spread public support and donations to carry out its mission of
-increasing the number of public domain and licensed works that can be
-freely distributed in machine readable form accessible by the widest
-array of equipment including outdated equipment. Many small donations
-($1 to $5,000) are particularly important to maintaining tax exempt
-status with the IRS.
-
-The Foundation is committed to complying with the laws regulating
-charities and charitable donations in all 50 states of the United
-States. Compliance requirements are not uniform and it takes a
-considerable effort, much paperwork and many fees to meet and keep up
-with these requirements. We do not solicit donations in locations
-where we have not received written confirmation of compliance. To SEND
-DONATIONS or determine the status of compliance for any particular
-state visit www.gutenberg.org/donate
-
-While we cannot and do not solicit contributions from states where we
-have not met the solicitation requirements, we know of no prohibition
-against accepting unsolicited donations from donors in such states who
-approach us with offers to donate.
-
-International donations are gratefully accepted, but we cannot make
-any statements concerning tax treatment of donations received from
-outside the United States. U.S. laws alone swamp our small staff.
-
-Please check the Project Gutenberg Web pages for current donation
-methods and addresses. Donations are accepted in a number of other
-ways including checks, online payments and credit card donations. To
-donate, please visit: www.gutenberg.org/donate
-
-Section 5. General Information About Project Gutenberg-tm electronic works.
-
-Professor Michael S. Hart was the originator of the Project
-Gutenberg-tm concept of a library of electronic works that could be
-freely shared with anyone. For forty years, he produced and
-distributed Project Gutenberg-tm eBooks with only a loose network of
-volunteer support.
-
-Project Gutenberg-tm eBooks are often created from several printed
-editions, all of which are confirmed as not protected by copyright in
-the U.S. unless a copyright notice is included. Thus, we do not
-necessarily keep eBooks in compliance with any particular paper
-edition.
-
-Most people start at our Web site which has the main PG search
-facility: www.gutenberg.org
-
-This Web site includes information about Project Gutenberg-tm,
-including how to make donations to the Project Gutenberg Literary
-Archive Foundation, how to help produce our new eBooks, and how to
-subscribe to our email newsletter to hear about new eBooks.
-
-
-
-</pre>
-
-</body>
-</html>
diff --git a/old/52838-h/images/cover.jpg b/old/52838-h/images/cover.jpg
deleted file mode 100644
index 6734f89..0000000
--- a/old/52838-h/images/cover.jpg
+++ /dev/null
diff --git a/old/52838-h/images/map1_hr.jpg b/old/52838-h/images/map1_hr.jpg
deleted file mode 100644
index fdae32c..0000000
--- a/old/52838-h/images/map1_hr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/map1_lr.jpg b/old/52838-h/images/map1_lr.jpg
deleted file mode 100644
index f4fa704..0000000
--- a/old/52838-h/images/map1_lr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/map2_hr.jpg b/old/52838-h/images/map2_hr.jpg
deleted file mode 100644
index 6c2d619..0000000
--- a/old/52838-h/images/map2_hr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/map2_lr.jpg b/old/52838-h/images/map2_lr.jpg
deleted file mode 100644
index 3af6774..0000000
--- a/old/52838-h/images/map2_lr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p03.jpg b/old/52838-h/images/p03.jpg
deleted file mode 100644
index 2b54eab..0000000
--- a/old/52838-h/images/p03.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p05.jpg b/old/52838-h/images/p05.jpg
deleted file mode 100644
index f825a85..0000000
--- a/old/52838-h/images/p05.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p07.jpg b/old/52838-h/images/p07.jpg
deleted file mode 100644
index 586460a..0000000
--- a/old/52838-h/images/p07.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p09.jpg b/old/52838-h/images/p09.jpg
deleted file mode 100644
index eebc9d1..0000000
--- a/old/52838-h/images/p09.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p10.jpg b/old/52838-h/images/p10.jpg
deleted file mode 100644
index 4558ddf..0000000
--- a/old/52838-h/images/p10.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p11.jpg b/old/52838-h/images/p11.jpg
deleted file mode 100644
index c76e069..0000000
--- a/old/52838-h/images/p11.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p12.jpg b/old/52838-h/images/p12.jpg
deleted file mode 100644
index 14fc83d..0000000
--- a/old/52838-h/images/p12.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p13.jpg b/old/52838-h/images/p13.jpg
deleted file mode 100644
index e9b5c59..0000000
--- a/old/52838-h/images/p13.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p13a.jpg b/old/52838-h/images/p13a.jpg
deleted file mode 100644
index c08b845..0000000
--- a/old/52838-h/images/p13a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p13b.jpg b/old/52838-h/images/p13b.jpg
deleted file mode 100644
index 758e47d..0000000
--- a/old/52838-h/images/p13b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p14.jpg b/old/52838-h/images/p14.jpg
deleted file mode 100644
index ea18a66..0000000
--- a/old/52838-h/images/p14.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p14a.jpg b/old/52838-h/images/p14a.jpg
deleted file mode 100644
index c3ced18..0000000
--- a/old/52838-h/images/p14a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p15.jpg b/old/52838-h/images/p15.jpg
deleted file mode 100644
index 9ac1100..0000000
--- a/old/52838-h/images/p15.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p16.jpg b/old/52838-h/images/p16.jpg
deleted file mode 100644
index 23a5229..0000000
--- a/old/52838-h/images/p16.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p16a.jpg b/old/52838-h/images/p16a.jpg
deleted file mode 100644
index baa98c7..0000000
--- a/old/52838-h/images/p16a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p17.jpg b/old/52838-h/images/p17.jpg
deleted file mode 100644
index 64ec59f..0000000
--- a/old/52838-h/images/p17.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p17a.jpg b/old/52838-h/images/p17a.jpg
deleted file mode 100644
index bf99ca2..0000000
--- a/old/52838-h/images/p17a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p17b.jpg b/old/52838-h/images/p17b.jpg
deleted file mode 100644
index 1e2b25c..0000000
--- a/old/52838-h/images/p17b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p18.jpg b/old/52838-h/images/p18.jpg
deleted file mode 100644
index 71ab099..0000000
--- a/old/52838-h/images/p18.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p19.jpg b/old/52838-h/images/p19.jpg
deleted file mode 100644
index 6d89cb4..0000000
--- a/old/52838-h/images/p19.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p19a.jpg b/old/52838-h/images/p19a.jpg
deleted file mode 100644
index 71b25a2..0000000
--- a/old/52838-h/images/p19a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p20.jpg b/old/52838-h/images/p20.jpg
deleted file mode 100644
index 0a0ce9d..0000000
--- a/old/52838-h/images/p20.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p21.jpg b/old/52838-h/images/p21.jpg
deleted file mode 100644
index 1da6ae0..0000000
--- a/old/52838-h/images/p21.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p22.jpg b/old/52838-h/images/p22.jpg
deleted file mode 100644
index 4822cbb..0000000
--- a/old/52838-h/images/p22.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p22a.jpg b/old/52838-h/images/p22a.jpg
deleted file mode 100644
index 6c6c7c2..0000000
--- a/old/52838-h/images/p22a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p23.jpg b/old/52838-h/images/p23.jpg
deleted file mode 100644
index 13cede8..0000000
--- a/old/52838-h/images/p23.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p23a.jpg b/old/52838-h/images/p23a.jpg
deleted file mode 100644
index 7edf7dc..0000000
--- a/old/52838-h/images/p23a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p23b.jpg b/old/52838-h/images/p23b.jpg
deleted file mode 100644
index 33d1d6f..0000000
--- a/old/52838-h/images/p23b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p24.jpg b/old/52838-h/images/p24.jpg
deleted file mode 100644
index 114a002..0000000
--- a/old/52838-h/images/p24.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p24a.jpg b/old/52838-h/images/p24a.jpg
deleted file mode 100644
index 4055a16..0000000
--- a/old/52838-h/images/p24a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p25.jpg b/old/52838-h/images/p25.jpg
deleted file mode 100644
index f346ec4..0000000
--- a/old/52838-h/images/p25.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p25a.jpg b/old/52838-h/images/p25a.jpg
deleted file mode 100644
index 542c333..0000000
--- a/old/52838-h/images/p25a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p26.jpg b/old/52838-h/images/p26.jpg
deleted file mode 100644
index df10a85..0000000
--- a/old/52838-h/images/p26.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p26a.jpg b/old/52838-h/images/p26a.jpg
deleted file mode 100644
index ae862f6..0000000
--- a/old/52838-h/images/p26a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p27.jpg b/old/52838-h/images/p27.jpg
deleted file mode 100644
index c9ddce5..0000000
--- a/old/52838-h/images/p27.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p28.jpg b/old/52838-h/images/p28.jpg
deleted file mode 100644
index 215beb1..0000000
--- a/old/52838-h/images/p28.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p29.jpg b/old/52838-h/images/p29.jpg
deleted file mode 100644
index 1f7a79f..0000000
--- a/old/52838-h/images/p29.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p29a.jpg b/old/52838-h/images/p29a.jpg
deleted file mode 100644
index bc90842..0000000
--- a/old/52838-h/images/p29a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p30.jpg b/old/52838-h/images/p30.jpg
deleted file mode 100644
index a3b8843..0000000
--- a/old/52838-h/images/p30.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p30a.jpg b/old/52838-h/images/p30a.jpg
deleted file mode 100644
index cd7f793..0000000
--- a/old/52838-h/images/p30a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p30b.jpg b/old/52838-h/images/p30b.jpg
deleted file mode 100644
index 349a921..0000000
--- a/old/52838-h/images/p30b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p31.jpg b/old/52838-h/images/p31.jpg
deleted file mode 100644
index 52e2b40..0000000
--- a/old/52838-h/images/p31.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p31b.jpg b/old/52838-h/images/p31b.jpg
deleted file mode 100644
index 3c0e1a3..0000000
--- a/old/52838-h/images/p31b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p31c.jpg b/old/52838-h/images/p31c.jpg
deleted file mode 100644
index e3801c8..0000000
--- a/old/52838-h/images/p31c.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p31f.jpg b/old/52838-h/images/p31f.jpg
deleted file mode 100644
index 3ed677e..0000000
--- a/old/52838-h/images/p31f.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32a.jpg b/old/52838-h/images/p32a.jpg
deleted file mode 100644
index 57c33ca..0000000
--- a/old/52838-h/images/p32a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32b.jpg b/old/52838-h/images/p32b.jpg
deleted file mode 100644
index 4bff0b2..0000000
--- a/old/52838-h/images/p32b.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32c.jpg b/old/52838-h/images/p32c.jpg
deleted file mode 100644
index a605c2a..0000000
--- a/old/52838-h/images/p32c.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32d.jpg b/old/52838-h/images/p32d.jpg
deleted file mode 100644
index fd2dea9..0000000
--- a/old/52838-h/images/p32d.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32g.jpg b/old/52838-h/images/p32g.jpg
deleted file mode 100644
index 2d5a7c9..0000000
--- a/old/52838-h/images/p32g.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p32h.jpg b/old/52838-h/images/p32h.jpg
deleted file mode 100644
index af06aaa..0000000
--- a/old/52838-h/images/p32h.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p33.jpg b/old/52838-h/images/p33.jpg
deleted file mode 100644
index 291e338..0000000
--- a/old/52838-h/images/p33.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p33a.jpg b/old/52838-h/images/p33a.jpg
deleted file mode 100644
index b91b5b0..0000000
--- a/old/52838-h/images/p33a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p34.jpg b/old/52838-h/images/p34.jpg
deleted file mode 100644
index 5d380b8..0000000
--- a/old/52838-h/images/p34.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p35.jpg b/old/52838-h/images/p35.jpg
deleted file mode 100644
index 1003656..0000000
--- a/old/52838-h/images/p35.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p35a.jpg b/old/52838-h/images/p35a.jpg
deleted file mode 100644
index 5d35bd6..0000000
--- a/old/52838-h/images/p35a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p36.jpg b/old/52838-h/images/p36.jpg
deleted file mode 100644
index e072b40..0000000
--- a/old/52838-h/images/p36.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p36a.jpg b/old/52838-h/images/p36a.jpg
deleted file mode 100644
index 255c80f..0000000
--- a/old/52838-h/images/p36a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p37.jpg b/old/52838-h/images/p37.jpg
deleted file mode 100644
index 5f9187d..0000000
--- a/old/52838-h/images/p37.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p37a.jpg b/old/52838-h/images/p37a.jpg
deleted file mode 100644
index af13e0f..0000000
--- a/old/52838-h/images/p37a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p38.jpg b/old/52838-h/images/p38.jpg
deleted file mode 100644
index 54afea0..0000000
--- a/old/52838-h/images/p38.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p38a.jpg b/old/52838-h/images/p38a.jpg
deleted file mode 100644
index 339c02d..0000000
--- a/old/52838-h/images/p38a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p39.jpg b/old/52838-h/images/p39.jpg
deleted file mode 100644
index 5336ed5..0000000
--- a/old/52838-h/images/p39.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p40.jpg b/old/52838-h/images/p40.jpg
deleted file mode 100644
index ecf5a1b..0000000
--- a/old/52838-h/images/p40.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p40a.jpg b/old/52838-h/images/p40a.jpg
deleted file mode 100644
index 43c893a..0000000
--- a/old/52838-h/images/p40a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p41.jpg b/old/52838-h/images/p41.jpg
deleted file mode 100644
index 6a2d9c5..0000000
--- a/old/52838-h/images/p41.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p42.jpg b/old/52838-h/images/p42.jpg
deleted file mode 100644
index c658512..0000000
--- a/old/52838-h/images/p42.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p43.jpg b/old/52838-h/images/p43.jpg
deleted file mode 100644
index eedd5f8..0000000
--- a/old/52838-h/images/p43.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p43a.jpg b/old/52838-h/images/p43a.jpg
deleted file mode 100644
index 1f5f5b6..0000000
--- a/old/52838-h/images/p43a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p44.jpg b/old/52838-h/images/p44.jpg
deleted file mode 100644
index 854248d..0000000
--- a/old/52838-h/images/p44.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p44a.jpg b/old/52838-h/images/p44a.jpg
deleted file mode 100644
index 2b58997..0000000
--- a/old/52838-h/images/p44a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p45.jpg b/old/52838-h/images/p45.jpg
deleted file mode 100644
index 0d7758d..0000000
--- a/old/52838-h/images/p45.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p46.jpg b/old/52838-h/images/p46.jpg
deleted file mode 100644
index fbed40f..0000000
--- a/old/52838-h/images/p46.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p47.jpg b/old/52838-h/images/p47.jpg
deleted file mode 100644
index 4753832..0000000
--- a/old/52838-h/images/p47.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p48.jpg b/old/52838-h/images/p48.jpg
deleted file mode 100644
index c794a64..0000000
--- a/old/52838-h/images/p48.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p48a.jpg b/old/52838-h/images/p48a.jpg
deleted file mode 100644
index 8e203ee..0000000
--- a/old/52838-h/images/p48a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p49.jpg b/old/52838-h/images/p49.jpg
deleted file mode 100644
index b87d28b..0000000
--- a/old/52838-h/images/p49.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p50a.jpg b/old/52838-h/images/p50a.jpg
deleted file mode 100644
index e37ac0e..0000000
--- a/old/52838-h/images/p50a.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p59.jpg b/old/52838-h/images/p59.jpg
deleted file mode 100644
index dece56a..0000000
--- a/old/52838-h/images/p59.jpg
+++ /dev/null
diff --git a/old/52838-h/images/p61.jpg b/old/52838-h/images/p61.jpg
deleted file mode 100644
index a64c6ad..0000000
--- a/old/52838-h/images/p61.jpg
+++ /dev/null
diff --git a/old/52838-h/images/v1_hr.jpg b/old/52838-h/images/v1_hr.jpg
deleted file mode 100644
index 759de08..0000000
--- a/old/52838-h/images/v1_hr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/v1_lr.jpg b/old/52838-h/images/v1_lr.jpg
deleted file mode 100644
index fe96f92..0000000
--- a/old/52838-h/images/v1_lr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/v2_hr.jpg b/old/52838-h/images/v2_hr.jpg
deleted file mode 100644
index 9a811d0..0000000
--- a/old/52838-h/images/v2_hr.jpg
+++ /dev/null
diff --git a/old/52838-h/images/v2_lr.jpg b/old/52838-h/images/v2_lr.jpg
deleted file mode 100644
index 21d334a..0000000
--- a/old/52838-h/images/v2_lr.jpg
+++ /dev/null