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Download : Fundamentals of Astrodynamics
In
1665 Newton was a student at the University of Cambridge when an
outbreak of the plague forced the university to close down for 2
years. Those 2 years were to be the most creative period in
Newton's life. The 23-year-old genius conceived the law of
gravitation, the laws of motion and developed the fundamental
concepts of the differential calculus during the long vacation of
1666, but owing to some small discrepancies in his explanation of the
moon's motion he tossed his papers aside. The world was not to learn
of his momentous discoveries until some 20 years later!
To
Edmund Halley, discoverer of Halley's comet, is due the credit for
bringing Newton's discoveries before the world. One day in 1685
Halley and two of his contemporaries, Christopher Wren and Robert
Hooke, were discussing the theory of Descartes which explained the
motion of the planets by means of whirlpools and eddies which swept
the planets around the sun. Dissatisfied with this explanation, they
speculated whether a force. "similar to magnetism " and
falling off inversely with the square of distance might not require
the planets to move in precisely elliptical paths. Hooke thought that
this should be easy to prove whereupon Wren offered Hooke 40
shillings if he could produce
the proof with in 2 weeks. The 2 weeks passed and nothing more was
heard from Hooke.
Several
months later Halley was visiting Newton at Cambridge and, without
mentioning the bet, casually posed the question, "If the sun
pulled the planets with a force inversely proportional to the square
of their distances, in what paths ought they to go? " To
Halley's utter and complete astonishment Newton replied without
hesitation, "Why, in ellipses, of course. I have already calculated it and have the proof among my papers somewhere. Give me a few
days and I shall find it for you." Newton was referring to the
work he had done some 20 years earlier and only in this casual way
was his greatest discovery made known to the world!
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