Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.Spencer, Herbert
Philosophy
Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.
Spencer, Herbert
Philosophy; Political science; Science
evidently, in a large spheroid, a depth below the surface at which the
pressure will be great enough, if the temperature is sufficiently low.
Hence it is inferable that somewhere between centre and surface in the
supposed larger spheroid, there will arise that state described by Prof.
Andrews, in which "flickering striæ" of liquid float in gaseous matter
of equal density. And it may be inferred that gradually, as the process
goes on, these striæ will become more abundant while the gaseous
interspaces diminish; until, eventually, the liquid becomes continuous.
Thus there will result a molten shell containing a gaseous nucleus
equally dense with itself at their surface of contact and more dense at
the centre--a molten shell which will slowly thicken by additions to
both exterior and interior.
That a solid crust will eventually form on this molten shell may be
reasonably concluded. To the demurrer that solidification cannot
commence at the surface, because the solids formed would sink, there are
two replies. The first is that various metals expand while solidifying,
and therefore would float. The second is that since the envelope of the
supposed spheroid would consist of the gases and non-metallic elements,
compounds of these with the metals and with one another would
continually accumulate on the molten shell; and the crust, consisting of
oxides, chlorides, sulphurets, and the rest, having much less specific
gravity than the molten shell, would be readily supported by it.
Clearly a planet thus constituted would be in an unstable state. Always
it would remain liable to a catastrophe resulting from change in its
gaseous nucleus. If, under some condition of pressure and temperature
eventually reached, the components of this suddenly entered into one of
those proto-chemical combinations forming a new element, there might
result an explosion capable of shattering the entire planet, and
propelling its fragments in all directions with high velocities. If the
hypothetical planet between Jupiter and Mars was intermediate in size as
in position, it would apparently fulfil the conditions under which such
a catastrophe might occur.
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