The Royal Observatory, Greenwich: A Glance at Its History and WorkMaunder, E. Walter (Edward Walter)
History
The Royal Observatory, Greenwich: A Glance at Its History and Work
Maunder, E. Walter (Edward Walter)
Astronomy -- History; Royal Observatory, Greenwich
Not long after his return from this tour, Halley was led to that
undertaking for which we owe him the greatest debt of gratitude, and
which must be regarded as his greatest achievement.
Some fifty years before, the great Kepler had brought out the third
of his well-known laws of planetary motion. These laws stated
that the planets move round the sun in ellipses, of which the sun
occupies one of the foci; that the straight line joining any planet
with the sun moves over equal areas of space in equal periods of
time; and, lastly, that the squares of the times in which the
several planets complete a revolution round the sun are proportional
to the cubes of their mean distances from it. These three laws were
deduced from actual examination of the movements of the planets.
Kepler did not work out any underlying cause of which these three
laws were the consequence.
But the desire to find such an underlying cause was keen amongst
astronomers, and had given rise to many researches. Amongst those
at work on the subject was Halley himself. He had seen, and been
able to prove, that if the planets moved in circles round the sun,
with the sun in the centre, then the law of the relation between the
times of revolution and the distances of the planets would show that
the attractive force of the sun varied inversely as the square of
the distance. The actual case, however, of motion in an ellipse was
too hard for him, and he could not deal with it. Halley therefore
went up to Cambridge to consult Newton, and, to his wonder and
delight, found that the latter had already completely solved the
problem, and had proved that Kepler's three laws of planetary motion
were summed up in one, namely, that the sun attracted the planets to
it with a force inversely proportional to the square of the distance.
Halley was most enthusiastic over this great discovery, and he at
once strongly urged Newton to publish it. Newton's unwillingness to
do so was great, but at length Halley overcame his reluctance; and
the Royal Society not being able at the time to afford the expense,
Halley took the charges upon himself, although his own resources had
been recently seriously damaged by the death of his father.
Public-domain text, read in full here on John Shaqi.
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