The Uses of Astronomy - An Oration Delivered at Albany on the 28th of July, 1856 by Edward Everett
page 59 of 72 (81%)
page 59 of 72 (81%)
![]() | ![]() |
|
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.] But if some of the adventurous speculations built by Sir William Herschell on the bewildering revelations of his telescope have been since questioned, the vast progress which has been made in sidereal astronomy, to which, as I understand, the Dudley Observatory will be particularly devoted, the discovery of the parallax of the fixed stars, the investigation of the interior relations of binary and triple systems of stars, the theories for the explanation of the extraordinary, not to say fantastic, shapes discerned in some of the nebulous systems--whirls and spirals radiating through spaces as vast as the orbit of Neptune;[A] |
|