The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
The periodic times of the planets are here instructive. The materials
now forming Jupiter were situated towards the exterior of the nebula, so
that, as the nebula contracted, it tended to leave Jupiter behind. The
period in which Jupiter now revolves round the sun may give some notion
of the period of the rotation of the nebula at the time that it extended
so far as Jupiter. Subsequently to the formation, and the detachment of
Jupiter, a body which was henceforth no longer in contact with the
nebula, the latter proceeded further in its contraction. Passing over
the intermediate stages, we find the nebula contracting until it
extended no further than the line now marked by the earth’s orbit; the
speed with which the nebula was rotating must have been increasing all
the time, so that though the nebula required several years to go round
when it extended as far as Jupiter, only a fraction of that period was
necessary when it had reached the position indicated by the earth’s
track at the present time. Leaving the earth behind it, just as it had
previously left Jupiter, the nebula started on a still further
condensation. It drew in, until at last it reached a further stage by
contraction into the sun, which rotates in less than a month. Thus the
period of Jupiter namely, twelve years, the period of the earth, namely,
one year, and the period of the sun, namely, twenty-five days,
illustrate the successive accelerations of the rotation of the nebula in
the process of contraction. No doubt these statements must be received
with much qualification, but they will illustrate the nature of the
argument.
We may also here mention the satellites of Uranus, all the more so
because it has been frequently urged as an objection to the nebular
theory that the orbits of the satellites of Uranus lie in a plane which
is inclined at a very large angle; no less than 82° to the general plane
of the solar system. I shall refer in a later chapter to this subject,
and consider what explanation can be offered with regard to the great
inclination of this plane, which is one of the anomalies of our system.
For the present I merely draw attention to the fact that the movements
of all four satellites of Uranus do actually lie in the same plane,
though, as already indicated, it stands nearly at right angles to the
ecliptic.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account