The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
In addition to the revolutions of the planets around the sun, there are
other motions which can be accounted for as consequences of the
contraction of the nebula. We now refer to that central portion which is
to form the sun, and consider, in the first instance, only one of the
subordinate portions which is to form a planet. As these two bodies form
part of the same nebulous mass they will to a certain extent rotate
together as one piece. If any body is rotating as a whole, every part of
that body is also in actual rotation. We shall refer to this again later
on; but for the present it is sufficient to observe that as the planet
was originally continuous with the sun, it had a motion of rotation
besides its motion of revolution, and it revolved round its own axis in
a period equal to that of its revolution round the sun. In the beginning
the rotation of the planet was therefore an exceedingly slow movement.
But it became subsequently accelerated. For we have already explained
that each planet is by itself subjected to the law of the conservation
of moment of momentum. As each planet assumes a separate existence, it
draws to itself its share of the moment of momentum, and that must be
strictly preserved. But the planet, or rather the materials which are to
form the future planet, are all the time shrinking; they are drawing
more closely together. If, therefore, the area which each particle of
the planet describes when multiplied by the mass of that particle and
added to the similar products arising from all the other particles, is
to remain constant, it becomes necessary that just as the orbits of
these particles diminish in size, so must the speed at which they
revolve increase. We thus find that there is a tendency in the planet to
accelerate its rotation. And thus we see that a time will come when the
planet, having assumed an independent existence, will be found rotating
round its axis with a velocity which must be considered high in
comparison with the angular velocity which the planet had while it still
formed part of the original nebula.
Public-domain text, read in full here on John Shaqi.
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