Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
His return to London and election to the Royal Society (of which he was
many years secretary) added much to his fame, and he was commissioned
by the society to visit Danzig and arbitrate an astronomical controversy
between Hooke and Hevelius, both his seniors by a generation.
On the continent he associated with other great astronomers, especially
Cassini, who had already found three Saturnian moons; and it was then he
observed the great comet of 1680, which led up to the most famous event
of Halley's life.
The seerlike Seneca may almost be said to have predicted the advent of
Halley, when he wrote ("Quaestiones Naturales," vii): "Some day there
will arise a man who will demonstrate in what region of the heavens
comets pursue their way; why they travel apart from the planets; and
what their sizes and constitution are. Then posterity will be amazed
that simple things of this sort were not explained before."
To Newton it appeared probable that cometary voyagers through space
might have orbits of their own; and he proved that the comet of 1680
never swerved from such a path. As it could nowhere approach within the
moon's orbit, clearly threats of its wrecking the earth and punishing
its inhabitants ought to frighten no more.
Halley then became intensely interested in comets, and gathered whatever
data concerning the paths of all these bodies he could find. His first
great discovery was that the comets seen in 1531 by Apian, and in 1607
by Kepler, traveled round the sun in identical paths with one he had
himself observed in 1682. A still earlier appearance of Halley's comet
(1456) seems to have given rise to a popular and long-reiterated myth of
a papal bull excommunicating "the Devil, the Turk, and the Comet."
No longer room for doubt: so certain was Halley that all three were one
and the same comet, completing the round of its orbit in about
seventy-six years, that he fearlessly predicted that it would be seen
again in 1758 or 1759. And with equal confidence he might have foretold
its return in 1835 and 1910; for all three predictions have come true to
the letter.
Halley's span of existence did not permit his living to see even the
first of these now historic verifications. But we in our day may
emphatically term the epoch of the third verified return _Annus
Halleianus_.
Says Turner, Halley's successor in the Savilian chair at Oxford to-day:
"There can be no more complete or more sensational proof of a scientific
law, than to predict events by means of it. Halley was deservedly the
first to perform this great service for Newton's Law of Gravitation, and
he would have rejoiced to think how conspicuous a part England was to
play in the subsequent prediction of the existence of Neptune."
Halley rose rapidly among the chief astronomical figures of his day. But
he had little veneration for mere authority, and the significant veering
of his religious views toward heterodoxy was for years an obstacle to
his advance.
Public-domain text, read in full here on John Shaqi.
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