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
Soc.', and 'The Planet Neptune', 1848, by J. P. Nicholl.) -- Tr.
We may, with no incondsiderable degree of probability, include within the
domain of our Sun, in the immediate sphere of its central force, a rotating
ring of vaporous matter, lying probably between the orbits of Venus and
Mars, but certainly beyond that of the Earth,* which appears to us in
p 92
a pyramidal form, and is known as the 'Zodiacal Light'; and a host of very
small asteroids, whose orbits either intersect, or very nearly approach,
that of our earth, and which present us with the phenomena of aerolites and
falling or shooting stars.
[footnote] * "If there should be molecules in the zones diffused by the
atmosphere of the Sun of too volatile a nature either to combine with one
another or with the planets, we must suppose that they would, in circling
round that luminary, present all the appearances of zodiacal light, without
opposing any appreciable resistance to the different bodies composing the
planetary system, either owing to their extreme rarity, or to the similarity
existing between their motion and that of the planets with which they come
in contact." -- Laplace, 'Expos. du Syst. du Monde' (ed. 5), p. 415.
When we consider the complication of variously-formed bodies which revolve
round the Sun in orbits of such dissimilar eccentricity--although we may not
be disposed, with the immortal author of the 'Mecanique Celeste', to regard
the largr number of comets as nebulous stars, passing from one central
system to another,* we yet can not fail to acknowledge that the planetary
system, especially so called (that is, the group of heavenly bodies which,
together with their satellites, revolve with but slightly eccentric orbits
round the Sun), constitutes but a small portion of the whole system with
respect to individual numbers, if not to mass.
[footnote] *Laplace, 'Exp. du Syst. du Monde', p. 396, 414.
It has been proposed to consider the telescopic planets, Vesta, Juno, Ceres,
and Pallas, with their more closely intersecting, inclined, and eccentric
orbits, as a zone of separation, or as a middle group in space; and if this
view be adopted, we shall discover that the interior planetary group
(consisting of Mercury, Venus, the Earth, and Mars) presents several very
striking contrasts* when compared with the exterior group, comprising
Jupiter, Saturn, and Uranus.
[footnote] *Littrow, 'Astronomie', 1825, bd.xi., 107. Mädler, 'Astron.',
1841, § 212. Laplace, 'Exp. du Syst. du Monde', p. 210.
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