Planetary motion

Definition and stakes

Florence M. Grimm,  Astronomical Lore in Chaucer

“ These two bodies, however, always appear to be moving directly on in their courses, each completing a revolution around the earth in a definite time, the sun in a year, the moon in 291⁄2 days. What we see in the case of the planets, on the other hand, is a complex motion compounded of the effects of the earth’s daily rotation, its yearly revolution around the sun, and the planets’ own revolutions in different periods of time in elliptical orbits around the sun. These complex planetary motions are characterized by the peculiar oscillations known as ‘direct’ and ‘retrograde’ movements. ”
Source: Gutenberg

Arthur Berry,  A Short History of Astronomy (1898)

“ Kepler's laws of planetary motion were in fact shewn to lead necessarily to the conclusions that the sun exerts on a planet an attraction inversely proportional to the square of the distance of the planet from the sun, and that such an attraction affords a sufficient explanation of the motion of the planet. ”
Source: Wikisource

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