Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1Humboldt, Alexander von
History
Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1
Humboldt, Alexander von
Astronomy; Cosmography; Physical geography; Science -- History
Mädler and Wilhelm Beer, be expressed as 2.47 semi-diameters of that
planet, or as 80,088 miles. Its distance from the surface of the main
planet is therefore 47,480 miles, and from the outer-most edge of the ring
only 4916 miles. The traveler may form to himself an estimate of the
smallness of this amount by remembering the statement of an enterprising
navigator, Captain Beechey, that he had in three years passed over 72,800
miles. If, instead of absolute distances, we take the semi-diameters of the
principal planets, we shall find that even the first or nearest of the moons
of Jupiter (which is 26,000 miles further removed from the center of that
planet than our moon is from that of the Earth) is only six semi-diameters
of Jupiter from its center, while our moon is removed from us fully 60 1/3d
semi-diameters of the Earth.
In the subordinate systems of satellites, we find that the same laws of
gravitation which regulate the revolutions of the principal planets round
the Sun likewise govern the mutual relations existing between these planets
among one another and with reference to their attendant satellites. The
twelve moons of Saturn, Jupiter, and the Earth all most like the primary
planets from west to east, and in elliptic orbits, deviating
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but little from circles. It is only in the case of one moon, and perhaps in
that of the first and innermost of the satellites of Saturn (0.068), that we
discover an eccentricity greater than that of Jupiter; according to the very
exact observations of Bessel, the eccentricity of the sixth of Saturn's
satellites (0.029) exceeds that of the Earth. On the extremest limits of
the planetary system, where, at a distance nineteen times greater than that
of our Earth, the centripetal force of the Sun is greatly diminished, the
satellites of Uranus (which most striking contrasts from the facts observed
with regard to other secondary planets. Instead, as in all other
satellites, of having their orbits but slightly inclined toward the ecliptic
and (not excepting even Saturn's ring, which may be regarded as a fusion of
agglomerated satellites) moving from west to east, the satellites of Uranus
are almost perpendicular to the ecliptic, and move retrogressively from east
to west, as Sir John Herschel has proved by observations continued during
many years. If the primary and secondary planets have been formed by the
condensation of rotating rings of solar and planetary atmospheric vapor,
there must have existed singular causes of retardation or impediment in the
vaporous rings revolving round Uranus, by which, under the relations with
which we are unacquainted, the revolution of the second and fourth of its
satellites was made to assume a direction opposite to that of the rotation
of the central planet.
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