Illustrations of Universal Progress: A Series of Discussions — John Shaqi
Illustrations of Universal Progress: A Series of DiscussionsSpencer, Herbert
Philosophy
Illustrations of Universal Progress: A Series of Discussions
Spencer, Herbert
Philosophy; Political science; Science
It follows as a corollary from the Nebular Hypothesis, that the Earth must
at first have been incandescent; and whether the Nebular Hypothesis be true
or not, this original incandescence of the Earth is now inductively
established--or, if not established, at least rendered so highly probable
that it is a generally admitted geological doctrine. Let us look first at
the astronomical attributes of this once molten globe. From its rotation
there result the oblateness of its form, the alternations of day and night,
and (under the influence of the moon) the tides, aqueous and atmospheric.
From the inclination of its axis, there result the precession of the
equinoxes and the many differences of the seasons, both simultaneous and
successive, that pervade its surface. Thus the multiplication of effects is
obvious. Several of the differentiations due to the gradual cooling of the
Earth have been already noticed--as the formation of a crust, the
solidification of sublimed elements, the precipitation of water, &c.,--and
we here again refer to them merely to point out that they are simultaneous
effects of the one cause, diminishing heat.
Let us now, however, observe the multiplied changes afterwards arising from
the continuance of this one cause. The cooling of the Earth involves its
contraction. Hence the solid crust first formed is presently too large for
the shrinking nucleus; and as it cannot support itself, inevitably follows
the nucleus. But a spheroidal envelope cannot sink down into contact with a
smaller internal spheroid, without disruption; it must run into wrinkles as
the rind of an apple does when the bulk of its interior decreases from
evaporation. As the cooling progresses and the envelope thickens, the
ridges consequent on these contractions must become greater, rising
ultimately into hills and mountains; and the later systems of mountains
thus produced must not only be higher, as we find them to be, but they must
be longer, as we also find them to be. Thus, leaving out of view other
modifying forces, we see what immense heterogeneity of surface has arisen
from the one cause, loss of heat--a heterogeneity which the telescope shows
us to be paralleled on the face of the moon, where aqueous and atmospheric
agencies have been absent.
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