state and establish keplars law of planetry 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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- Keplers1st law:
Every planet move around the sun in elliptical orbits with sun situated at one of the focii
2nd law:
The line that joins any planet to the sun sweeps equal areas in equal intervals of time.
3rd law:
The square of the time period of a planet around the sun is directly proportional to. The square of semi major axis.
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