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] *Arago, in the 'Annuaire', 1832, p. 246. Several physical facts
appear to indicate that, in a mechanical separation of matter into its
smallest particles, if the mass be very small in relation to the surface,
the electrical tension may increase sufficiently for the production of light
and heat. Experiments with a large concave mirror have not hitherto given
any positive evidence of the presence of radiant heat in the zodiacal light.
(Lettre de M. Matthiessen à M. Arago, in the 'Comptes Rendus', t. xvi.,
1843, Avril, p. 687.)
Must we suppose that changes are actually in progress in the nebulous ring?
or is it not more probable that, although I could not, by my meteorological
instruments, detect any change of heat or moisture near the ground, and
small stars of the fifth and sixth magnitudes appeared to shine with equally
undiminished intensity of light, processes of condensation may be going on
in the uppermost strata of the air, by means of which the transparency, or
rather, the reflection of light, may be modified in some peculiar and
unknown manner?
p 143
An assumption of the existence of such meteorological causes on the confines
of our atmosphere is strengthened by the "sudden flash and pulsation of
light," which, according to the acute observations of Olbers, vibrated for
several seconds through the tail of a comet, which appeared during the
continuance of the pulsations of light to be lengthened by several degrees,
and then again contracted.*
[footnote] *"What you tell me of the changes of light in the zodiacal
light, and of the causes to which you ascribe such changes within the
tropics, is of the greatr interest to me, since I have been for a long time
past particularly attentive, every spring, to this phenomenon in our
northern latitudes. I, too, have always believed that the zodiacal light
rotated; but I assumed (contrary to Poisson's opinion, which you have
communicated to me) that it completely extended to the Sun, with
considerably augmenting brightness. The light circle which, in total solar
eclipses, is seen surrounding the darkened Sun, I have regarded as the
brightest portion of the zodiacal light. I have convinced my self that this
light is very different in different years, often for several successive
years being very bright and diffused, while in othr years it is scarcely
perceptible. I tyhink that I find the first trace of an allusion to the
zodiacal light in a letter from Rothmann to Tycho, in which he mentions that
in the spring he has observed the twilight did not close until the sun was
24ºdegrees below the horizon. Rothmann must certainly have confounded the
disappearance of the setting zodiacal light in the vapors of the western
horizon with the actual cessation of twilight. I have failed to observe the
pulsations of the light, probably on account of the faintness with which it
appears in these countries. You are, however, certainly right in ascribing
Public-domain text, read in full here on John Shaqi.
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