Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
Tidal friction has also been operant in producing sun-raised tides upon
the early plastic substances which composed the planets: more powerfully
in the case of planets nearer the sun; less rapidly if the planet's mass
is large; also less completely if the planet has solidified earlier on
account of its small dimensions. So Darwin would account for the
present rotation periods of all the planets: both Mercury and Venus
powerfully acted on by the sun on account of their nearness to him, and
their rotational energy completely exhausted, so that they now and for
all time turn a constant face toward him, as the moon does to the earth;
earth and possibly Mars even yet undergoing a very slight lengthening of
their day; Jupiter and Saturn, also Uranus and probably Neptune, still
exhibiting relatively swift axial rotation, because of their great mass
and great original moment of momentum, and also by reason of their vast
distances from the central tide-raising body, the sun.
By applying to stellar systems the principles developed by Darwin, See
accounted for the fact, to which he was the first to direct attention,
that the great eccentricity of the binary orbits is a necessary result
of the secular action of tidal friction. The double stars, then, were
double nebulæ, originally single, but separated by a process allied to
that known as "fission" in protozoans. Indeed, Poincaré proved
mathematically that a swiftly revolving nebula, in consequence of
contraction, first undergoes distortion into a pear-shaped or hour-glass
figure, the two masses ultimately separating entirely; and the
observations of the Herschels, Lord Rosse and others, with the recent
photographic plates at the Lick and Mount Wilson observatories, afford
immediate confirmation in a multitude of double nebulæ, widely scattered
throughout the nebular regions of the heavens.
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