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] *Fries, 'Vorlesungen uber die Sternkunde', 1833, s. 262-267
(Lectures on the Science of Astronomy). An infelicitously chosen instance
of the good omen of a comet may be found in Seneca, 'Nat. Quest.', vii., 17
and 21. The philosopher thus writes of the comet: "Quem nos Neronis
principatu latissimo vidimus et qui cometis detraxit infamiam."
The strange form of a large comet, its faint nebulous light, and its sudden
appearance in the vault of heaven, have in all regions been almost
invariably regarded by the people at large as some new and formidable agent
inimical to the existing state of things. The sudden occurrence and short
duration of the phenomenon lead to the belief of some equally rapid
reflection of its agency in terrestrial matters, whose varied nature renders
it easy to find events that may be regarded as the fulfillment of the evil
foretold by the appearance of these mysterious cosmical bodies. In our own
day, however, the public mind has taken another and more cheerful, although
singular, turn with regard to comets; and in the German vineyards in the
beautiful valleys of the Rhine and Moselle, a belief has arisen, ascribing
to these once ill-omened bodies a beneficial influence on the ripening of
the vine. The evidence yielded by experience, of which there is no lack in
these days, when comets may so frequently be observed, has not been able to
shake the common belief in the meteorological myth of the existence of
wandering stars capable of radiating heat.
This material taken from pages 111- 147
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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From comets I would pass to the consideration of a far more enigmatical
class of agglomerated matter -- the smallest of all asteroids, to which we
apply the name 'aërolites', or 'meteoric stones',* when they reach our
atmosphere in a fragmentary condition.
[footnote] * (Much valuable information may be obtained regarding the
origin and composition of aërolites or meteoric stones in Memoirs on the
subject, by Baumbeer and other writers, in the numbers of Poggendorf's
'Annalen', from 1845 to the present time.) -- Tr.
Public-domain text, read in full here on John Shaqi.
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