state laws of kepler
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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,
(2)having the Sun as one of the foci.
(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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There are actually three, Kepler's laws that is, of planetary motion:
- every planet's orbit is an ellipse with the Sun at a focus;
- a line joining the Sun and a planet sweeps out equal areas in equal times; and
- the square of a planet's orbital period is proportional to the cube of the semi-major axis
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