explain Kepler three laws with equation
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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.
(3) The squares of the sidereal periods (of revolution) of the planets are directly proportional to the cubes of their mean distances from the Sun.
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KEPLER'S LAWS ARE:
1) Orbit of an planet is an ellipse with the sun at one of its foci.
2) The line joining planet and the sun sweeps equal are in equal interval of time .
3) The square of its period of revolution around sun is directly proportional to the cube of the mean distance of a planet from the sun
1) Orbit of an planet is an ellipse with the sun at one of its foci.
2) The line joining planet and the sun sweeps equal are in equal interval of time .
3) The square of its period of revolution around sun is directly proportional to the cube of the mean distance of a planet from the sun
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