what is Keplers law of planetary motion
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Kepler's three laws of planetary motion can be stated as follows: (1) All planets move about the Sun in elliptical orbits, having the Sun as one of the foci. (2) A radius vector joining any planet to the Sun sweeps out equal areas in equal lengths of time.
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Kepler's first law: The orbit of a planet is an ellipse with sun at one of the focii.
Kepler's second law: The line joining the planet and sun sweeps equal areas in equal interval of time .
Kepler's third law: The square of the period of revolution of a planet around the sun is directly proportional to the cube of the mean distance of the planet from the sun.
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