Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.Spencer, Herbert
Philosophy
Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.
Spencer, Herbert
Philosophy; Political science; Science
The calculations ending with these figures were made while the Sun's
distance was still estimated at 95 millions of miles. Of course the
reduction afterwards established in the estimated distance, entailing,
as it did, changes in the factors which entered into the calculations,
affected the results; and, though it was unlikely that the relations
stated would be materially changed, it was needful to have the
calculations made afresh. Mr. Lynn has been good enough to undertake
this task, and the figures given in the text are his. In the case of
Mars a large error in my calculation had arisen from accepting Arago's
statement of his density (0·95), which proves to be something like
double what it should be. Here a curious incident may be named. When, in
1877, it was discovered that Mars has two satellites, though, according
to my hypothesis, it seemed that he should have none, my faith in it
received a shock; and since that time I have occasionally considered
whether the fact is in any way reconcilable with the hypothesis. But now
the proof afforded by Mr. Lynn that my calculation contained a wrong
factor, disposes of the difficulty--nay, changes the objection to a
verification. It turns out that, according to the hypothesis, Mars
_ought_ to have satellites; and, further, that he ought to have a number
intermediate between 1 and 4.]
[Footnote 19: Since this paragraph was first published, the discovery
that Mars has two satellites revolving round him in periods shorter than
that of his rotation, has shown that the implication on which Laplace
here insists is general only, and not absolute. Were it a necessary
assumption that all parts of a concentrating nebulous spheroid revolve
with the same angular velocities, the exception would appear an
inexplicable one; but if, as suggested in a preceding section, it is
inferable from the process of formation of a nebulous spheroid, that its
outer strata will move round the general axis with higher angular
velocities than the inner ones, there follows a possible interpretation.
Though, during the earlier stages of concentration, while the nebulous
matter, and especially its peripheral portions, are very rare, the
effects of fluid-friction will be too small to change greatly such
differences of angular velocities as exist; yet, when concentration has
reached its last stages, and the matter is passing from the gaseous into
the liquid and solid states, and when also the convection-currents have
become common to the whole mass (which they probably at first are not),
the angular velocity of the peripheral portion will gradually be
assimilated to that of the interior; and it becomes comprehensible that
in the case of Mars the peripheral portion, more and more dragged back
by the internal mass, lost part of its velocity during the interval
between the formation of the innermost satellite and the arrival at the
final form.]
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