Kepler's laws of motion
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Law 1. The orbits of the planets are ellipses, with the Sun at one focus.
Law 2. The line joining a planet to the Sun sweeps out equal areas in equal times as the planet travels around the ellips.
Laws3: The square of the total time period (T) of the orbit is proportional to the cube of the average distance of the planet to the Sun (R).
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