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Humboldt, Alexander von, 1769-1859

"COSMOS: A Sketch of the Physical Description of the Universe, Vol. 1"

', 1837, s. 280. I was informed in Cumana that
shortly before the fearful earthquake of 1766, and consequently thirty-three
years (the same interval) before the great fall of stars on the 11th and
12th of November, 1799, a similar fiery manifestation had been observed in
the heavens. But it was on the 21st of October, 1766, and not in the
beginning of November, that the earthquake occurred. Possibly some traveler
in Quito may yet be able to ascertain the day on which the volcano of
Cayambe, which is situated there, was for the space of an hour enveloped in
falling stars, so that the inhabitants endeavored to appease heaven by
religious processions. ('Relat. Hist.', t. i., chap. iv., p 307; chap. x.,
p. 520 and 527.)

The different meteoric streams, each of which is composed of myriads of
small cosmical bodies, probably intersect our Earth's orbit in the same
manner as Biela's comet. According to this hypothesis, we may represent to
ourselves these asteroid-meteors as composing a closed ring or zone, within
which they all pursue one common orbit. The s aller planets between Mars
and Jupiter present us if we except Pallas with an analogous relation in
their constantly intersecting orbits. As yet, however, we have no certain
knowledge as to whether changes in the periods at which the stream becomes
visible, or the 'retardations' of the phenomena of which I have already
spoken, indicate a regular precession of oscillation of the nodes -- that is
to say, of the points of intersection of the Earth's orbit and of that of
the ring; or whether this ring or zone attains so considerable a degree of
breadth from the irregular grouping and distances apart of the small bodies,
that it requires several days for the Earth to traverse it.


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