The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
IN the present chapter, and in the two chapters which are to follow, I
propose to give an outline of those arguments in favour of the nebular
theory which are presented by certain remarkable coincidences observed
in the movements of the bodies of our solar system. There are, indeed,
certain features in the movements of the planets which would seem so
inexplicable if the arrangement of the system had taken place by chance,
that it is impossible not to seek for some physical explanation. We have
already had occasion to refer in previous chapters to the movements of
the bodies of our system. It will be our object at present to show that
it is hardly conceivable that the movements could have acquired the
peculiar characteristics they possess unless the solar system has itself
had an origin such as that which the nebular theory assigns.
The argument on which we are to enter is, it must be confessed, somewhat
subtle, but its cogency is irresistible. For this argument we are
indebted to one of the great founders of the nebular theory. It was
given by Kant himself in his famous essay.
We will commence with a preliminary point which relates to elementary
mechanics. It may, however, help to clear up a difficult point in our
argument if I now state some well-known principles in a manner specially
adapted for our present purpose.
Let us think of two bodies, A and S, and, for the sake of clearness, we
may suppose that each of these bodies is a perfect sphere. We might
think of them as billiard balls, or balls of stone, or balls of iron. We
shall, however, suppose them to be formed of material which is perfectly
rigid. They may be of any size whatever, large or small, equal or
unequal. One of them may be no greater than a grain of mustard-seed, and
the other may be as large as the moon or the earth or the sun. Let us
further suppose that there is no other body in the universe by which the
mutual attraction of the two bodies we are considering can be interfered
with. If these two bodies are abandoned to their mutual attraction, let
us now see what the laws of mechanics assure us must necessarily happen.
[Illustration: Fig. 45.—A SPIRAL PRESENTED EDGEWISE (n.g.c. 4631; in
Coma Berenices).
(_Photographed by Dr. Isaac Roberts, F.R.S._)]
Public-domain text, read in full here on John Shaqi.
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