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 theory of an exploded planet now seemed to have everything in its
favour. It required that the mean or average distances of the
newly-discovered bodies should be nearly the same, but admitted a wide
range of variety in the shapes and positions of their orbits, provided
always that they preserved common points of intersection. These
conditions were fulfilled with a striking approach to exactness. Three
of the four "asteroids" (a designation introduced by Sir. W.
Herschel[207]) conformed with very approximate precision to "Bode's law"
of distances; they all traversed, in their circuits round the sun,
nearly the same parts of Cetus and Virgo; while the eccentricities and
inclinations of their paths departed widely from the planetary
type--that of Pallas, to take an extreme instance, making with the
ecliptic an angle of nearly 35°. The minuteness of these bodies appeared
further to strengthen the imputation of a fragmentary character.
Herschel estimated the diameter of Ceres at 162, that of Pallas at 147
miles.[208] But these values are now known to be considerably too small.
A suspected variability of brightness in some of the asteroids, somewhat
hazardously explained as due to the irregularities of figure to be
expected in cosmical _potsherds_ (so to speak), was added to the
confirmatory evidence.[209] The strong point of the theory, however, lay
not in what it explained, but in what it had predicted. It had been
twice confirmed by actual exploration of the skies, and had produced, in
the recognition of Vesta, the first recorded instance of the
_premeditated_ discovery of a heavenly body.
The view not only commended itself to the facile imagination of the
unlearned, but received the sanction of the highest scientific
authority. The great Lagrange bestowed upon it his analytical
_imprimatur_, showing that the explosive forces required to produce the
supposed catastrophe came well within the bounds of possibility; since a
velocity of less than twenty times that of a cannon-ball leaving the
gun's mouth would have sufficed, according to his calculation, to launch
the asteroidal fragments on their respective paths. Indeed, he was
disposed to regard the hypothesis of disruption as more generally
available than its author had designed it to be, and proposed to
supplement with it, as explanatory of the eccentric orbits of comets,
the nebular theory of Laplace, thereby obtaining, as he said, "a
complete view of the origin of the planetary system more conformable to
Nature and mechanical laws than any yet proposed."[210]
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