A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
The recognition of the second followed as the immediate consequence of
the detection of the first. Olbers had made himself so familiar with the
positions of the small stars along the track of the long-missing body,
that he was at once struck (March 28, 1802) with the presence of an
intruder near the spot where he had recently identified Ceres. He at
first believed the new-comer to be a variable star usually
inconspicuous, but just then at its maximum of brightness; but within
two hours he had convinced himself that it was no _fixed_ star, but a
rapidly moving object. The aid of Gauss was again invoked, and his
prompt calculations showed that this fresh celestial acquaintance (named
"Pallas" by Olbers), revolved round the sun at nearly the same mean
distance as Ceres, and was beyond question of a strictly analogous
character.
This result was perplexing in the extreme. The symmetry and simplicity
of the planetary scheme appeared fatally compromised by the admission of
many, where room could, according to old-fashioned rules, only be found
for one. A daring hypothesis of Olbers's invention provided an exit from
the difficulty. He supposed that both Ceres and Pallas were fragments of
a primitive trans-Martian planet, blown to pieces in the remote past,
either by the action of internal forces or by the impact of a comet; and
predicted that many more such fragments would be found to circulate in
the same region. He, moreover, pointed out that these numerous orbits,
however much they might differ in other respects, must all have a common
line of intersection,[206] and that the bodies moving in them must
consequently pass, at each revolution, through two opposite points of
the heavens, one situated in the Whale, the other in the constellation
of the Virgin, where already Pallas had been found and Ceres recaptured.
The intimation that fresh discoveries might be expected in those
particular regions was singularly justified by the detection of two
bodies now known respectively as Juno and Vesta. The first was found
near the predicted spot in Cetus by Harding, Schröter's assistant at
Lilienthal, September 2, 1804; the second by Olbers himself in Virgo,
after three years of persistent scrutiny, March 29, 1807.
Public-domain text, read in full here on John Shaqi.
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