History of Physical Astronomy, From the Earliest Ages to the Middle of the 19th Century. Comprehending a Detailed Account of the Establishment of the Theory of Gravitation By Newton, And Its Development By His Successors; With An Exposition of the Progres

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This remark applies * Phil. Trans., 1798, p. 78. f Ibid., 1815, p. 356.
t Ibid., 1798, p. 76; ibid., 1815, p. 355.
§ Opera Varia, torn, ii., p. 524.
II Anc. Mem. Acad, des Sciences, tome x., p. 586.
^ Phil. Trans., 1790, Part I., p. 7 ; also 1798, p. 74.
** It results from the invisibility of the satellites of Uranus near conjunction, that the eclipses of these bodies (which, on account of the great inclination of their orbits can only take place on the occasion of the passage of the planet thr
...ough either of the nodes) will necessarily be invisible also, HISTORY OF PHYSICAL ASTRONOMY. O35 not merely to the four satellites alluded to by Herscliel at a later period of liis researches, the existence of which might be regarded as proble- matical, but also to the two satellites originally discovered by him in 1787, the theory of whose motions he had brought to a state of consider- able perfection. It does not appear that any astronomer obtained even a sight of these faint objects until the year 1828, when Sir John Herschel detected them with a 20-feet reflector.

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