Appletons' Popular Science Monthly, February 1900: Vol. 56, November, 1899 to April, 1900Various
Science
Appletons' Popular Science Monthly, February 1900: Vol. 56, November, 1899 to April, 1900
Various
Science -- Periodicals; Technology -- Periodicals
Although the most important of all crust movements in determining the
whole history of the earth, and especially of the organic kingdom, we
shall dwell no further on them, because no progress has yet been made
in their explanation. This, too, must be left to the workers of the
twentieth century.
_The Principle of Isostasy._--The principle of static equilibrium as
applied to earth forms was first brought forward (as so many other
valuable suggestions and anticipations in many departments of science)
by the wonderfully fertile mind of Sir John Herschel, and used by him
in the explanation of the sinking of river deltas under the increasing
weight of accumulating sediments.[C] It was afterward applied to
continental masses by Archbishop Pratt[D] and by the Royal Astronomer
Professor Airy.[E] But for its wide application as a principle in
geology, its clear definition, and its embodiment in an appropriate
name, we are indebted to Major Dutton, United States Army.[F]
[C] Philosophical Magazine, vol. ii, p. 212, 1837; Quarterly
Journal of Geological Society, vol. ii, p. 548, 1837.
[D] Philosophical Magazine, vol. ix, p. 231, and vol. x, p.
240, 1855.
[E] Philosophical Trans., 1855, p. 101.
[F] Philosophical Society of Washington, 1892.
The principle may be briefly stated as follows: A globe so large as the
earth, under the influence of its own gravity, must behave like a very
stiffly viscous body--that is, the general form of the earth and its
greatest inequalities must be in substantial static equilibrium. For
example, the general form of the earth is oblate spheroid, because that
is the only form of equilibrium of a rotating body. Rotation determines
a distribution of gravity with latitude which brings about this form.
With any other form the earth would be in a state of strain to which
it must slowly yield, and finally relieve itself by becoming oblate.
If the rotation stopped, the earth would accommodate itself to the new
distribution of gravity and become spherical.
The same is true of the large inequalities of surface. Oceanic
basins and continental arches must be in static equilibrium or they
could not sustain themselves. In order to be in equilibrium the
sub-oceanic material must be as much more dense than the continental
and sub-continental material as the ocean bottoms are lower than
the continental surfaces. Such static equilibrium, by difference of
density, is completely explained by the mode of formation of oceanic
basins already given.
So also plateaus and great mountain ranges are at least partly
sustained by gravitative equilibrium, but partly also by earth
rigidity. It is only the smaller inequalities, such as ridges, peaks,
valleys, etc., that are sustained by earth rigidity alone.
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