A Century's Progress in AstronomyMacpherson, Hector
History
A Century's Progress in Astronomy
Macpherson, Hector
Astronomy -- History
The fact that the Earth and Moon were almost in contact suggests that
they were probably in contact. In other words, the Moon originally
formed part of the Earth, which, in consequence of its short-rotation
period, and probably also owing to the interference of the solar tide,
split into two portions, and the smaller of these now forms the Moon. It
is likely that the matter now forming the Moon was detached from the
Earth in separate particles. Just as the tides raised by the Moon tend
to retard the motion of the Earth, so the Earth tides raised in the Moon
have already done their work. The Moon now rotates on its axis in the
same time as it revolves round the Earth. Part of the evolution of the
Earth-Moon system is completed. Schiaparelli’s discovery that the
rotation periods of both Venus and Mercury coincide with their times of
revolution is distinctly confirmatory of Darwin’s theory.
In his chapter on the “Evolution of Celestial Systems” in his book on
‘The Tides,’ Darwin discusses the distribution of the satellites of the
Solar System. He says of the evolution of a planet: “We have seen that
rings should be shed from the central nucleus when the contraction of
the nebula has induced a certain degree of augmentation of rotation.
Now, if the rotation were retarded by some external cause, the genesis
of a ring might be retarded or entirely prevented.” He then remarks that
probably the formation of the Moon was retarded, and in the case of
Mercury and Venus, solar tidal friction prevented satellite formation.
This explains why Mercury and Venus have no satellites, the Earth only
one, Mars two, while the exterior planets have each several satellites.
The theory of tidal friction was extended in 1892 to the explanation of
the double stars by the American astronomer, See. See showed by
mathematical calculation the effects of tidal friction in shaping the
eccentric orbits of the binary stars, the course of evolution being
traced from double stars, revolving almost in contact, which the
spectroscope reveals, to the telescopic doubles. See’s researches have
done much to supplement those of Darwin, who considers that there are
two types of cosmical evolution,—the Laplacian, and the “second” or
lunar type.
Lowell, in his work on ‘The Solar System’ (1903), adds six congruities
to those remarked by Laplace and his successors. These are, “All the
satellites turn the same face to their primaries (so far as we can
judge); Mercury, and probably Venus, do the same to the Sun; one law
governs position and size in the Solar System and in all the satellite
systems; orbital inclinations in the satellite systems increase with
distance from the primary; the outer planets show a greater tilt of axis
to orbit-plane with increased distance from the Sun (so far as
detectable); the inner planets show a similar relation.”
Public-domain text, read in full here on John Shaqi.
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