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
If we consider the proper, and not the perspective motions of the stars, we
shall find many that appear to be distributed in groups, having an opposite
direction; and facts hitherto observed do not, at any rate, render it a
necessary assumption that all parts of our starry stratum, or the whole of
the stellar islands filling space, should move round one large unknown
luminous or non-luminous central body. The tendency of the human mind to
investigate ultimate and highest causes certainly inclines the intellectual
activity, no less than the imagination of mankind, to adopt such an
hypothesis. Even the Stagirite proclaimed that "every thing which is moved
must be referable to a motor, and that there would be no end to
p 147
the concatenation of causes if there were not one primordial immovable
morot."*
[footnote] *Aristot., 'de Cælo', iii., 2, p. 301, Bekker: 'Phys.', viii.,
t, p. 256.
This material taken from pages 147-203
COSMOS: A Sketch of the Physical Description of the Universe, Vol. 1
by Alexander von Humboldt
Translated by E C Otte
from the 1858 Harper & Brothers edition of Cosmos, volume 1
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The manifold translatory changes of the stars, not those produced by the
parallaxes at which they are seen from the changing position of the
spectator, but the true changes constantly going on in the regions of space,
afford us incontrovertible evidence of the 'dominion of the laws of
attraction' in the remotest regions of space, beyond the limits of our solar
system. The existence of these laws is revealed to us by many phenomena,
as, for instance, by the motion of double stars, and by the amount of
retarded or accelerated motion in different parts of their elliptic orbits.
Human inquiry need no longer pursue this subject in the domain of vague
conjecture, or amid the undefined analogies of the ideal world; for even
here the progress made in the method of astronomical observations and
calculations has enabled astronomy to take up its position on a firm basis.
It is not only the discovery of the astounding numbers of double and
multiple stars revolving round a center of gravity lying 'without' their
system (2800 such systems having been discovered up to 1837), but rather the
extension of our knowledge regarding the fundamental forces of the whole
material world, and the proofs we have obtained of the universal empire of
the laws of attraction, that must be ranked among the most brilliant
discoveries of the age. The periods of revolution of colored stars present
the greatest differences; thus, in some instances, the period extends to 43
years, as in πpi of Corona, and in others to several thousands,, as in 66
of Cetus, 38 of Gemini, and 100 of Pisces. Since Herschel's measurements in
1782, the satellite of the nearest star in the triple system of [Greek
letter] of Cancer has completed more than one entire revolution. By a
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