The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
The energy of the earth-moon system is on the decline: the lost energy
might conceivably be drawn from the rotation of the earth, or it might
be drawn from the revolution of the moon, or it might be drawn from both
If it were drawn from the revolution of the moon, that would imply that
the moon would lose some of its speed or some of its distance, or in any
case that the moon would get nearer to the earth and revolve more
slowly, the speed of the earth being on this supposition unaltered. In
this case, the moment of momentum of the earth would remain the same as
before, while the moment of momentum of the moon would be lessened; the
total moment of momentum would therefore have decreased, but this we
have seen to be impossible. It therefore follows that the energy
withdrawn from the earth-moon system is not to be obtained at the
expense of the revolution of the moon.
The energy must therefore be obtained at the expense of the rotation of
the earth on its axis. But if this be the case, the speed with which the
earth rotates must be diminished; that is to say, the length of the day
must be increased. And if the speed of the earth’s rotation be reduced,
that means that the amount of moment of momentum contributed by the
earth is lessened. But the total quantity of moment of momentum must be
sustained, and this can only be done by making the moon go further away
and describe a larger orbit. We thus see that in consequence of the
tides the length of the day must be increasing, and the moon must be
gradually retreating. Thus we find that at earlier periods the moon’s
distance from the earth must have been less than it is at present, and
the further we look back through remote periods the less do we find the
distance between the earth and the moon. Thus we see that there must
have been a time when the moon or the materials of the moon were in
actual contact with the materials of the earth. In fact, it seems quite
possible that the moon may have been a portion of the earth, broken off
at some very early period, while the earth was still in a liquid state,
if indeed it had condensed to even that extent. Thus the revolution of
the moon round the earth is hardly to be used as an argument in favour
of the nebular hypothesis. The moon is indeed a consequence of the
earth’s rotation.
The satellites of Mars offer conditions of a very different kind, though
here, again, tidal influences have been so important, that it is perhaps
questions relating to tides that are illustrated by these satellites
rather than the nebular theory.
Public-domain text, read in full here on John Shaqi.
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