The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
The idea of diffused matter distributed here and there in space, and
gradually condensing into stars, is by no means new. As early as 1572,
Tycho Brahé proposed such an hypothesis, to explain the sudden
apparition of a new star in Cassiopeia, which he considered as formed by
the recent agglomeration of the "celestial matter" diffused in space.
Kepler adopted the same idea to explain the new star which appeared in
Ophiuchus, in 1604. Halley, Lacaille, Mairan and others, entertained the
same opinion. The hypothesis of a self-luminous, nebulous matter
diffused in space, and forming here and there immense masses, has been
proposed from the origin of the telescope, and was adopted by Sir
William Herschel, who in his grand speculations on the universe
considered the nebulæ as immense masses of phosphorescent vapors,
gradually condensing around one or several centres into stars or
clusters of stars. The evidence afforded by the spectroscope seems to be
in favor of such an hypothesis, and shows us that gaseous agglomerations
exist in space.
According to our modern conception, the visible universe is but an
infinitely small portion of the infinite universe perceived by our mind.
The great blazing centre around which our little, non-luminous globe
pursues its endless journey, is only an humble member of a cluster
comprising four hundred equally powerful suns, as they are believed to
be, although they appear to us as little twinkling stars. The nearest of
these stars is 221,000 times as far from the Sun as the Sun is from the
Earth, and yet this entire cluster is only one among the several hundred
Star-clusters composing the great galactic nebula in which we are
involved, comprising thirty or fifty millions of such suns. Among the
4,000 irresolvable nebulæ in the sky, perhaps over one-half are
supposed to be galaxies, like our own galaxy, composed of star-clusters,
and millions of stars. Besides these remote galaxies, vast
agglomerations of yet uncondensed, nebulous matter exist in space, and
form the nebulæ proper, in which the genesis of suns is slowly
elaborated. Although the visible universe is limited by the penetrating
power of our instruments, yet we see in imagination the infinite
universe stretching farther and farther; but we know not whether this
invisible universe is totally devoid of matter, or whether it also is
filled with millions and millions of suns and galaxies.
APPENDIX
KEY TO THE PLATES
PLATE I.--GROUP OF SUN-SPOTS AND VEILED SPOTS.
_Observed June_ 17, 1875, _at 7h. 30m. A. M._
Public-domain text, read in full here on John Shaqi.
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