Illustrations of Universal Progress: A Series of DiscussionsSpencer, Herbert
Philosophy
Illustrations of Universal Progress: A Series of Discussions
Spencer, Herbert
Philosophy; Political science; Science
Before proceeding to consider what the Nebular Hypothesis indicates
respecting the internal structures of the Sun and planets, we may state
that our reasonings, though of a kind not admitting of direct verification,
are nothing more than deductions from the established principles of
physics. We have submitted them to an authority not inferior to any that
can be named; and while unprepared to commit himself to them, he yet sees
nothing to object.
Starting, then, with a rotating spheroid of aeriform matter, in the later
stages of its concentration, but before it has begun to take a liquid or
solid form, let us inquire what must be the actions going on in it. Mutual
gravitation continually aggregates its atoms into a smaller and denser
mass; and the aggregating force goes on increasing, as the common centre of
gravity is approached. An obstacle to concentration, however, exists in the
centrifugal force, which at this stage bears a far higher ratio to gravity
than afterwards, and in a gaseous spheroid must produce a very oblate form.
At the same time, the approximation of the atoms is resisted by a force
which, in being overcome, is evolved as heat. This heat must be greatest
where the atoms are subject to the highest pressure--namely, about the
central parts. And as fast as it escapes into space, further approximation
and further generation of heat must take place. But in a gaseous spheroid,
having internal parts hotter than its external parts, there must be some
circulation. The currents must set from the hottest region to the coolest
by some particular route; and from the coolest to the hottest by some other
route. In a very oblate spheroid, the coolest region must be that about the
equator: the surface there bearing so large a ratio to the mass. Hence
there will be currents from the centre to the equator, and others from the
equator to the centre. What will be the special courses of these currents?
Supposing an original state of rest, about to pass into motion in obedience
to the disturbing forces, the currents commencing at the centre will follow
the lines of most rapidly-decreasing density; seeing that the inertia will
be least in those lines. That is to say, there will be a current from the
centre towards each pole, along the axis of rotation; and the space thus
continually left vacant will be filled by the collapse of matter coming in
at right angles to the axis. The process cannot end here, however. If there
are constant currents from the centre towards the poles, there must be a
constant accumulation at the poles; the spheroid will be ever becoming more
protuberant about the poles than the conditions of mechanical equilibrium
permit. If, however, the mass at the poles is thus ever in excess, it must,
by the forces acting on it, be constantly moved over the outer surface of
the spheroid from the poles towards the equator: thus only can that form
which rotation necessitates be maintained. And a further result of this
Public-domain text, read in full here on John Shaqi.
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