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-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
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