Creation of the Teton Landscape: The Geologic Story of Grand Teton National Park — John Shaqi
Creation of the Teton Landscape: The Geologic Story of Grand Teton National ParkReed, John C. (John Calvin)
Science
Creation of the Teton Landscape: The Geologic Story of Grand Teton National Park
Reed, John C. (John Calvin)
Geology -- Wyoming -- Grand Teton National Park
[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._]
Public-domain text, read in full here on John Shaqi.
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