CM111A – Calculus I Compact Lecture Notes
Kepler’s First Law (1605): the orbit of each planet is an ellipse, with the sun at one of the two foci Kepler’s Second Law (1602): a line joining the sun to an orbiting planet sweeps out equal areas in equal times Kepler’s Third Law (1618): the square of a planet’s orbit period is proportional to cube of its distance to the sun
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