Personal Narrative Of Travels To The Equinoctial Regions Of America During The Years 1799-1804 - Volume 1 - By Alexander Von Humboldt And Aime Bonpland.
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On the 18th of
January, and the 15th of February, 1800, the intensity of the
zodiacal light changed in a very perceptible manner, at intervals
of two or three minutes.
Sometimes it was very faint, at others it
surpassed the brilliancy of the Milky Way in Sagittarius. The
changes took place in the whole pyramid, especially toward the
interior, far from the edges. During these variations of the
zodiacal light, the hygrometer indicated considerable dryness. The
stars of the fourth and fifth magnitude appeared constantly to the
naked eye with the same degree of light. No stream of vapour was
visible: nothing seemed to alter the transparency of the
atmosphere. In other years I saw the zodiacal light augment in the
southern hemisphere half an hour before its disappearance. Cassini
admitted "that the zodiacal light was feebler in certain years, and
then returned to its former brilliancy." He thought that these slow
changes were connected with "the same emanations which render the
appearance of spots and faculae periodical on the solar disk." But
this excellent observer does not mention those changes of intensity
in the zodiacal light which I have several times remarked within
the tropics, in the space of a few minutes. Mairan asserts, that in
France it is common enough to see the zodiacal light, in the months
of February and March, mingling with a kind of Aurora Borealis,
which he calls 'undecided,' and the nebulous matter of which
spreads itself all around the horizon, or appears toward the west.
I very much doubt, whether, in the observations I have been
describing, there was any mixture of these two species of light.
The variations in intensity took place at considerable altitudes;
the light was white, and not coloured; steady, and not undulating.
Besides, the Aurora Borealis is so seldom visible within the
tropics, that during five years, though almost constantly sleeping
in the open air, and observing the heavens with unremitting
attention, I never perceived the least traces of that phenomenon.
I am rather inclined to think that the variations of the zodiacal
light are not all appearances dependent on certain modifications in
the state of our atmosphere. Sometimes, during nights equally
clear, I sought in vain for the zodiacal light, when, on the
previous night, it had appeared with the greatest brilliancy. Must
we admit that emanations which reflect white light, and seem to
have some analogy with the tails of comets, are less abundant at
certain periods? Researches on the zodiacal light have acquired a
new degree of interest since geometricians have taught us that we
are ignorant of the real causes of this phenomenon. The illustrious
author of "La Mecanique Celeste" has shown that the solar
atmosphere cannot reach even the planet Mercury; and that it could
not in any case display the lenticular form which has been
attributed to the zodiacal light. We may also entertain the same
doubts respecting the nature of this light, as with regard to that
of the tails of comets.
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