Kepler's law of planetary motion 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 Law➫ A law state that the orbit of each planet is an ellipse with the sun at one focus of the ellipse.
▸ This law is also known as - Kepler's Law 0f Planetary Motion.
➧The Kepler's Laws are:-▃▃▃▃▃▃▃▃▃▃▃▃▃▃▃▃▃▃▃⤵
❶❫ Laws 0f 0rbit:-▬▬▬▬▬▬▬▬▬▬☟
Every planets revolves around the sun in an Elliptical 0rbit with the Sun situated at one of the foci of the ellipse.
❷❫ Laws 0f Area:-▬▬▬▬▬▬▬▬▬▬☟
Each planets moves in a such a way that an imaginary line drawn from the sun to the planets sweeps out equal area in equal intervals of time.
❸❫ Laws 0f Time Period:-▬▬▬▬▬▬▬▬▬▬▬☟
The square of the orbital period of a planet is proportional to the cube of the semi-major axis of its 0rbit.
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