Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
One of the most remarkable phenomena of the solar system is the
rigorous equality which is observed to subsist between the angular
motions of rotation and revolution of each satellite. It is infinity to
unity that this is not the effect of hazard. The theory of universal
gravitation makes infinity to disappear from this improbability, by
shewing that it is sufficient for the existence of this phenomenon,
that at the commencement these motions did not differ much. Then,
the attraction of the planet would establish between them a perfect
equality; but at the same time it has given rise to a periodic
oscillation in the axis of the satellite directed to the planet, of
which oscillation the extent depends on the primitive difference
between these motions. As the observations of Mayer on the libration
of the Moon, and those which Bouvard and Nicollet made for the
same purpose, at my request, did not enable us to recognize this
oscillation; the difference on which it depends must be extremely
small, which indicates with every appearance of probability the
existence of a particular cause, which has confined this difference
within very narrow limits, in which the attraction of the planet might
establish between the mean motions of rotation and revolution a rigid
equality, which at length terminated by annihilating the oscillation
which arose from this equality. Both these effects result from our
hypothesis; for we may conceive that the Moon, in a state of vapour,
assumed in consequence of the powerful attraction of the earth the
form of an elongated spheroid, of which the greater axis would be
constantly directed towards this planet, from the facility with which
the vapours yield to the slightest force impressed upon them. The
terrestrial attraction continuing to act in the same manner, while
the Moon is in a state of fluidity, ought at length, by making the
two motions of this satellite to approach each other, to cause their
difference to fall within the limits, at which their rigorous equality
commences to establish itself. Then this attraction should annihilate,
by little and little, the oscillation which this equality produced on
the greater axis of the spheroid directed towards the earth. It is in
this manner that the fluids which cover this planet, have destroyed by
their friction and resistance the primitive oscillations of its axis
of rotation, which is only now subject to the nutation resulting from
the actions of the Sun and Moon. It is easy to be assured that the
equality of the motions of rotation and revolution of the satellites
ought to oppose the formation of rings and secondary satellites, by the
atmospheres of these bodies. Consequently observation has not hitherto
indicated the existence of any such. The motions of the three first
satellites of Jupiter present a phenomenon still more extraordinary
than the preceding; which consists in this, that the mean longitude of
the first, minus three times that of the second, plus twice that of
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