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
Among Jupiter's satellites, which severally display these same
synchronous movements, there also exists a still more remarkable
relation. "If the mean angular velocity of the first satellite be added
to twice that of the third, the sum will be equal to three times that of
the second;" and "from this it results that the situations of any two of
them being given, that of the third can be found." Now here, as before,
no conceivable advantage results. Neither in this case can the connexion
have been accidental: the probabilities are infinity to one to the
contrary. But again, according to Laplace, the Nebular Hypothesis
supplies a solution. Are not these significant facts?
Most significant fact of all, however, is that presented by the rings of
Saturn. As Laplace remarks, they are, as it were, still extant witnesses
of the genetic process he propounded. Here we have, continuing
permanently, forms of aggregation like those through which each planet
and satellite once passed; and their movements are just what, in
conformity with the hypothesis, they should be. "La durée de la rotation
d'une planète doit donc être, d'après cette hypothèse, plus petite que
la durée de la révolution du corps le plus voisin qui circule autour
d'elle," says Laplace. And he then points out that the time of Saturn's
rotation is to that of his rings as 427 to 438--an amount of difference
such as was to be expected.[19]
Respecting Saturn's rings it may be further remarked that the place of
their occurrence is not without significance.
Rings detached early in the process of concentration, consisting of
gaseous matter having extremely little power of cohesion, can have
little ability to resist the disruptive forces due to imperfect balance;
and, therefore, collapse into satellites. A ring of a denser kind,
whether solid, liquid, or composed of small discrete masses (as Saturn's
rings are now concluded to be), we can expect will be formed only near
the body of a planet when it has reached so late a stage of
concentration that its equatorial portions contain matters capable of
easy precipitation into liquid and, finally, solid forms. Even then it
can be produced only under special conditions. Gaining a
rapidly-increasing preponderance as the gravitative force does during
the closing stages of concentration, the centrifugal force cannot, in
ordinary cases, cause the leaving behind of rings when the mass has
become dense. Only where the centrifugal force has all along been very
great, and remains powerful to the last, as in Saturn, can we expect
dense rings to be formed.
We find, then, that besides those most conspicuous peculiarities of the
Solar System which first suggested the theory of its evolution, there
are many minor ones pointing in the same direction. Were there no other
evidence, these mechanical arrangements would, considered in their
totality, go far to establish the Nebular Hypothesis.
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