The uses of astronomy : $b An oration delivered at Albany on the 28th of July, 1856Everett, Edward
Science
The uses of astronomy : $b An oration delivered at Albany on the 28th of July, 1856
Everett, Edward
Astronomy; Dudley Observatory
With Bradley, in 1741, a new period commenced in instrumental astronomy,
not so much of discovery as of measurement. The superior accuracy and
minuteness with which the motions and distances of the heavenly bodies
were now observed, resulted in the accumulation of a mass of new
materials, both for tabular comparison and theoretical speculation.
These materials formed the enlarged basis of astronomical science
between Newton and Sir William Herschell. His gigantic reflectors
introduced the astronomer to regions of space before unvisited--extended
beyond all previous conception the range of the observed phenomena, and
with it proportionably enlarged the range of constructive theory. The
discovery of a new primary planet and its attendant satellites was
but the first step of his progress into the labyrinth of the heavens.
Cotemporaneously with his observations, the French astronomers, and
especially La Place, with a geometrical skill scarcely, if at all,
inferior to that of its great author, resumed the whole system of
Newton, and brought every phenomenon observed since his time within his
laws. Difficulties of fact, with which he struggled in vain, gave way to
more accurate observations; and problems that defied the power of his
analysis, yielded to the modern improvements of the calculus.
HERSCHELL'S NEBULAR THEORY.
But there is no _Ultima Thule_ in the progress of science. With the
recent augmentations of telescopic power, the details of the nebular
theory, proposed by Sir W. Herschell with such courage and ingenuity,
have been drawn in question. Many--most--of those milky patches in which
he beheld what he regarded as cosmical matter, as yet in an unformed
state,--the rudimental material of worlds not yet condensed,--have been
resolved into stars, as bright and distinct as any in the firmament.
I well recall the glow of satisfaction with which, on the 22d of
September, 1847, being then connected with the University at Cambridge,
I received a letter from the venerable director of the Observatory
there, beginning with these memorable words:--"You will rejoice with
me that the great nebula in Orion has yielded to the powers of our
incomparable telescope! * * * It should be borne in mind that this
nebula, and that of Andromeda [which has been also resolved at
Cambridge], are the last strongholds of the nebular theory."[A]
[Footnote A: _Annals of the Observatory of Harvard College_, p. 121.]
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