Popular lectures on scientific subjects : $b Second series, with an autobiography of the authorHelmholtz, Hermann von
Science
Popular lectures on scientific subjects : $b Second series, with an autobiography of the author
Helmholtz, Hermann von
Science; Universities and colleges -- Germany
This would be a supposition of which we might admit the possibility,
but which could not perhaps claim any great degree of probability, if
we did not find that our predecessors, starting from quite different
considerations, had arrived at the same hypothesis.
You know that a considerable number of planets rotate around the
sun besides the eight larger ones, Mercury, Venus, the Earth, Mars,
Jupiter, Saturn, Uranus, and Neptune; in the interval between Mars
and Jupiter there circulate, as far as we know, 156 small planets or
planetoids. Moons also rotate about the larger planets--that is, about
the Earth and the four most distant ones, Jupiter, Saturn, Uranus, and
Neptune; and lastly the Sun, and at any rate the larger planets, rotate
about their own axes. Now, in the first place, it is remarkable that
all the planes of rotation of the planets and of their satellites,
as well as the equatorial planes of these planets, do not vary much
from each other, and that in these planes all the rotation is in the
same direction. The only considerable exceptions known are the moons
of Uranus, whose plane is almost at right angles to the planes of
the larger planets. It must at the same time be remarked that the
coincidence, in the direction of these planes, is on the whole greater,
the longer are the bodies and the larger the paths in question; while
in the smaller bodies, and for the smaller paths, especially for the
rotations of the planets about their own axes, considerable divergences
occur. Thus the planes of all the planets, with the exception of
Mercury and of the small ones between Mars and Jupiter, differ at most
by three degrees from the path of the Earth. The equatorial plane of
the Sun deviates by only seven and a half degrees, that of Jupiter
only half as much. The equatorial plane of the Earth deviates, it is
true, to the extent of twenty-three and a half degrees, and that of
Mars by twenty-eight and a half degrees, and the separate paths of the
small planet’s satellites differ still more. But in these paths they
all move direct, all in the same direction about the sun, and, as far
as can be ascertained, also about their own axes, like the earth--that
is, from west to east. If they had originated independently of each
other, and had come together, any direction of the planes for each
individual one would have been equally probable; a reverse direction of
the orbit would have been just as probable as a direct one; decidedly
elliptical paths would have been as probable as the almost circular
ones which we meet with in all the bodies we have named. There is, in
fact, a complete irregularity in the comets and meteoric swarms, which
we have much reason for considering to be formations which have only
accidentally come within the sphere of the sun’s attraction.
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