Illustrations of the Huttonian Theory of the EarthPlayfair, John
Science
Illustrations of the Huttonian Theory of the Earth
Playfair, John
Geology; Hutton, James, 1726-1797. Theory of the earth
While the parts of the sphere without the spheroid are thus continually
diminished, the loose earth and sand washed down from them, will be
deposited at the bottom of the sea, and will form strata parallel
to the surface of the superincumbent water. The actual and statical
figure are thus brought nearer one another; and, at the same time the
statical is changed, on the principle already explained, (the change in
the direction of gravity,) and is made continually to approximate to a
state, which when it has attained, no farther change can take place,
viz. an oblate elliptic spheroid, of which the surface is perpendicular
to the direction of gravity, having the equatorial diameter to the
polar axis in the ratio of 230 to 229.]
440. In the preceding reasonings, we have supposed the process of decay
and subsequent stratification to be carried on without interruption,
till the whole of the land is covered by the sea. This supposition is
useful for explaining the nature of the forces which have determined
the figure of the earth; but there is no reason to think that it has
ever been realized in its full extent, the elevation of strata from the
bottom of the sea interrupting the progress, and producing new land
in one place, as the old decays in another. The very same land also,
which is wasted at its surface, may perhaps be lifted up by the forces
that are placed under it; or it may be let down, undergoing alterations
of its level, from causes that we do not perceive, but of which the
action is undoubted, (§ 388.) But notwithstanding these interruptions,
the general tendency to produce in the earth a spheroidal figure may
remain, and more may be done by every revolution, to bring about the
attainment of that figure than to cause a deviation from it. This
figure, therefore, though never likely to be perfectly acquired, will
be the _limiting_ or _asymptotic_ figure, if it may be so called, to
which the earth will continually approach.
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