Graham's Magazine, Vol. XLI, No. 2, August 1852Various
General
Graham's Magazine, Vol. XLI, No. 2, August 1852
Various
Literature -- Periodicals; Literature, Modern -- 19th century -- Periodicals
morality?” The discovery of the great nebula in Orion was accidentally
made by Huygens in the year 1656. Cassini, nurtured in France, soon
afterward added four more satellites to the system of Saturn, those now
called the first, second, third, and fifth, and he detected the black
list, or dark, elliptical line bisecting the surface of the ring, and
dividing it into two. Astronomy is under immense obligations to a
measure adopted by the courts of France and England at nearly the same
period, for the patronage of scientific associations, and the founding
of national observatories. The Royal Society of London was incorporated
by charter in the year 1662, and numbered among its early members Boyle,
Hooke, Wallis, Ward, Newton, and Flamstead. The Royal Academy of
Sciences at Paris, was founded in the year 1666, and enrolled among its
first members Auzout, Picard, Roberval, and Richer. Upon the invitation
of Louis XIV. Huygens left Holland to become a royal academician, but
being a Protestant, the revocation of the edict of Nantes ultimately
compelled him to return to his native soil. The edict did not affect
Cassini, a Catholic foreigner similarly invited; and to him, with his
son and grandson, the French academy owes much of its early distinction.
Besides his before named discoveries, he determined the periods of
rotation of the principal planets, and observed the elliptical form of
Jupiter’s disc, owing to compression at the poles.
Roëmer, the inventor of the transit instrument with which he made
observations from the window of his house, rendered no unimportant
service by showing that the instruments need not be fixed on high
towers: he also discovered, in the year 1675, the interesting and
hitherto unsuspected fact, of the progressive transmission of light
through space, and the appreciable velocity with which it travels. This
was attained by a series of careful observations of the eclipses of
Jupiter’s satellites. It was found, by comparing the times of immersion
of the satellites in the planet’s shadow and emersion from it, with the
times calculated from the laws of their movements, that there was an
acceleration or retardation of the phenomena by a few minutes, plainly
dependent upon the variations of the earth’s distance from Jupiter; for
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