Pleasant Ways in ScienceProctor, Richard A. (Richard Anthony)
Science
Pleasant Ways in Science
Proctor, Richard A. (Richard Anthony)
Science
The view which I have long entertained respecting the growth of the
solar system—viz., that it had its origin, not in contraction only or
chiefly, but in combined processes of contraction and accretion—seems
to me to be very strongly confirmed by Dr. Draper’s discovery. This
would not be the place for a full discussion of the reasons on which
this opinion is based. But I may remark that I believe no one who
applies the laws of physics, _as at present known_, to the theory of
the simple contraction of a great nebulous mass formerly extending
far beyond the orbit of Neptune, till, when planet after planet had
been thrown off, the sun was left in his present form and condition
in the centre, will fail to perceive enormous difficulties in the
hypothesis, or to recognize in Dr. Draper’s discovery a difficulty
added to those affecting the hypothesis _so presented_. Has it ever
occurred, I often wonder, to those who glibly quote the nebular theory
as originally propounded, to inquire how far some of the processes
suggested by Laplace are in accordance with the now known laws of
physics? To begin with, the original nebulous mass extending to a
distance exceeding the earth’s distance from the sun more than thirty
times (this being only the distance of Neptune), if we assign to it a
degree of compression making its axial diameter half its equatorial
diameter, would have had a volume exceeding the sun’s (roughly) about
120,000,000,000 times, and in this degree its mean density would have
been less than the sun’s. This would correspond to a density equal
(roughly) to about one-400,000th part of the density of hydrogen gas at
atmospheric pressure. To suppose that a great mass of matter, having
this exceedingly small mean density, and extending to a distance of
three or four thousand millions of miles from its centre, could under
any circumstances rotate as a whole, or behave in other respects after
the fashion attributed to the gaseous embryon of the solar system
in ordinary descriptions of the nebular hypothesis, is altogether
inconsistent with correct ideas of physical and dynamical laws. It is
absolutely a necessity of any nebular hypothesis of the solar system,
that from the very beginning a central nucleus and subordinate nuclei
should form in it, and grow according to the results of the motions (at
first to all intents and purposes independent) of its various parts.
Granting this state of things, we arrive, by considering the combined
effects of accretion and contraction, at a process of development
according fully as well as that ordinarily described with the general
relations described by Laplace, and accounting also (in a general way)
for certain peculiarities which are in no degree explained by the
ordinary theory. Amongst these may specially be noted the arrangement
and distribution of the masses within the solar system, and the fact
that so far as spectroscopic evidence enables us to judge, a general
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