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
This phenomenon, whose primordial antiquity can scarcely be doubted, and
which was first noticed in Europe by Childrey and Dominicus Cassini, is not
the luminous solar atmosphere itself, since this can not, in accordance with
mechanical laws, be more compressed than in the relation of 2 to 3, and
consequently can not be diffused beyond 9/20ths of Mercury's heliocentric
distance. These same laws teach us that the altitude of the extreme
boundaries of the atmosphere of a cosmical
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body above its equator, that is to say, the point at which gravity and
centrifugal force are in equilibrium, must be the same as the altitude at
which a satellite would rotate round the central body simultaneously with
the diurnal revolution of the latter.*
[footnote] *Laplace, 'Expos. du Syst. du Monde', p. 270; 'Mécanique
Céleste', t. ii., p. 169 and 171; Schubert, 'Astr.', bd. iii., § 206.
This limitation of the solar atmosphere in its present concentrated
condition is especially remarkable when we compare the central body of our
system with the nucleus of other nebulous stars. Herschel has discovered
several, in which the radius of the nebulous matter surrounding the star
appeared at an angle of 150". On the assumption that the parallax is not
fully equal to 1", we find that the outermost nebulous layer of such a star
must be 150 times further from the central body than our Earth is from the
Sun. If, therefore, the nebulous star were to occupy the place of our Sun,
its atmosphere would not only include the orbit of Uranus, but even extend
eight times beyond it.•
[footnote] *Arago, in the 'Annuaire', 1842, p. 408. Compare Sir John
Herschel's considerations on the volume and faintness of light of planetary
nebulæ, in Mary Somerville's 'Connection of the Physical Sciences', 1835,
p. 108. The opinion that the Sun is a nebulous star, whose atmosphere
presents the phenomenon of zodiacal light, did not originate with Dominicus
Cassini, but was first promulgated by Mairan in 1730 ('Traité de l'Aurore
Bor.', p. 47 and 263; Arago, in the 'Annuaire', 1842, p. 412). It is a
renewal of Kepler's views.
Considering the narrow limitation of the Sun's atmosphere, which we have
just described, we may with much probability regard the existence of a very
compressed annulus of nebulous matter,* revolving freely in space between
the orbits of Venus and Mars, as the material cause of the zodiacal light.
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