The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
Let us think first of a single one of these bodies which, as is most
natural, we shall take to be the earth itself, and now let us consider
by what agency the movement of the earth around the sun is guided along
the path which so closely resembles a circle. It must, of course, be
borne in mind that there can be no direct material connection between
the two bodies; there is no physical bond uniting the earth to the sun.
It is, however, certain that some influence proceeding from the sun does
really control the motion. We may perhaps illustrate what takes place in
the following manner. Here is a globe, and here in my hand I hold a
tennis ball, which is attached to a silken thread, the other end of the
thread being attached to the ceiling. The tennis ball is to hang so that
both globe and ball are about the same height from the floor. We put the
globe directly underneath the point on the ceiling from which the silken
thread hangs. If I draw the tennis ball aside and simply release it,
then of course everybody knows what happens—it is hardly necessary to
try the experiment—the tennis ball falls at once towards the globe and
strikes it. We may, if we please, regard that tendency of the tennis
ball towards the globe as a sort of attraction which the globe exercises
upon the ball. I must, however, say that this is not a strictly accurate
version of what actually takes place. The attraction of the earth for
the tennis ball is of course largely neutralised by the support given by
the silk thread. There is thus only a slight outstanding component of
gravitation acting on the ball, and this component, which is virtually
the effective force on the ball, tends to draw the ball directly towards
the globe. For the purpose of our illustration we may neglect the direct
attraction of the earth altogether; we may omit all thought of the
tension of the silken thread. If there were indeed no attraction from
the earth, the tennis ball might remain poised in space without falling;
and if it were then attracted by the globe it would fly towards the
globe just as we actually see it do. We are therefore justified in
regarding the movement of the tennis ball as equivalent to that which
would be produced if an attractive virtue resided in the globe by which
it pulled the tennis ball. We may also imagine that the globe attracts
the tennis ball in all its positions; for whatever be the point at which
the ball is released it starts off straight towards the globe. This is
our first experiment in which, having withdrawn the ball, it is merely
released without receiving an initial impulse to one side.
[Illustration: Fig. 5.—NEBULOUS REGION AND STAR-CLUSTER
(n.g.c. 2237-9 in Monoceros).
(_Photographed by Dr. Isaac Roberts, F.R.S._)]
Public-domain text, read in full here on John Shaqi.
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