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
[footnote] *Sir John Herschel, in a letter from Feldhuysen, dated Jan.
13th, 1836. Nicholl, 'Architecture of the Heavens', 1838, p. 22. (See,
also, some separate notices by Sir William Herschel on the starless space
which separates us by a great distance from the Milky Way, in the 'Philos.
Transact.' for 1817, Part ii., p. 328.)
A cubic inch of the polishing slate of Bilin contains, according to
Ehrenberg, 40,000 millions of the silicious shells of Galionellae.
The stellar Milky Way, in the region of which, according to Argelander's
admirable observations, the brightest stars of the firmament appear to be
congregated, is almost at right angles
p 151
with another Milky Way, composed of nebulae. The former constitutes,
according to Sir John Herschel's views, an annulus, that is to say, an
independent zone, somewhat remote from our lenticular-shaped starry stratum,
and similar to Saturn's ring. Our planetary system lies in an eccentric
direction, nearer to the region of the Cross than to the diametrically
opposite point, Cassiopeia.*
[footnote] *Sir John Herschel, 'Astronom.', 624; likewise in his
'Observations on Nebulae and Clusters of Stars' ('Phil. Transact.', 1833,
Part ii., p. 479, fig. 25): "We have here a brother system, bearing a real
physical resemblance and strong analogy of structure to our own."
An imperfectly seen nebulous spot, discovered by Messier in 1774, appeared
to present a remarkable similarity to the form of our starry stratum and the
divided ring of our Milky Way.*
[footnote] *Sir William Herschel, in the 'Phil. Trans.' for 1785, Part i.,
p. 257. Sir John Herschel, 'Astron.', 616. ("The 'nebulous' region of the
heavens forms 'a nebulous Milky Way', composed of distinct nebulae, as the
other of stars." The same observation was made in a letter he addressed to
me in March, 1829.)
The Milky Way composed of nebulae does not belong to our starry stratum, but
surrounds it at a great distance without being physically connected with it,
passing almost in the form of a large cross through the dense nebulae of
Virgo, especially in the northern wing, through Comae Berenicis, Ursa Major,
Andromeda's girdle, and Pisces Boreales. It probably intersects the stellar
Milky Way in Cassiopeia, and connects its dreary poles (rendered starless
from the attractive forces by which stellar bodies are made to agglomerate
into groups) in the least dense portion of the starry stratum.
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