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
We have now to recount an event unique in scientific history. The
discovery of Neptune has been characterised as the result of a "movement
of the age,"[214] and with some justice. It had become necessary to the
integrity of planetary theory. Until it was accomplished, the phantom of
an unexplained anomaly in the orderly movements of the solar system must
have continued to haunt astronomical consciousness. Moreover, it was
prepared by many, suggested as possible by not a few, and actually
achieved, simultaneously, independently, and completely, by two
investigators.
The position of the planet Uranus was recorded as that of a fixed star
no less than twenty times between 1690 and the epoch of its final
detection by Herschel. But these early observations, far from affording
the expected facilities for the calculation of its orbit, proved a
source of grievous perplexity. The utmost ingenuity of geometers failed
to combine them satisfactorily with the later Uranian places, and it
became evident, either that they were widely erroneous, or that the
revolving body was wandering from its ancient track. The simplest course
was to reject them altogether, and this was done in the new Tables
published in 1821 by Alexis Bouvard, the indefatigable computating
partner of Laplace. But the trouble was not thus to be got rid of. After
a few years fresh irregularities began to appear, and continued to
increase until absolutely "intolerable." It may be stated as
illustrative of the perfection to which astronomy had been brought, that
divergencies regarded as menacing the very foundation of its theories
never entered the range of unaided vision. In other words, if the
theoretical and the real Uranus had been placed side by side in the sky,
they would have seemed, to the sharpest eye, to form a single body.[215]
The idea that these enigmatical disturbances were due to the attraction
of an unknown exterior body was a tolerably obvious one; and we
accordingly find it suggested in many different quarters. Bouvard
himself was perhaps the first to conceive it. He kept the possibility
continually in view, and bequeathed to his nephew's diligence the
inquiry into its reality when he felt that his own span was drawing to a
close; but before any progress had been made with it, he had already
(June 7, 1843) "ceased to breathe and to calculate." The Rev. T. J.
Hussey actually entertained in 1834 the notion, but found his powers
inadequate to the task, of assigning an approximate place to the
disturbing body; and Bessel, in 1840, laid his plans for an assault in
form upon the Uranian difficulty, the triumphant exit from which fatal
illness frustrated his hopes of effecting or even witnessing.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account