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Kepler's Second Law asserts that areas swept out by a planet in equal times are equal. Kepler's Third Law is the most complicated, and it relates the period of a planet, which is the time spent for one revolution around the sun, to the average distance to the sun.
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According to Kepler's Third law,
- For all planets,the square of the orbital period (T) of a planet is proportional to the cube of the average orbital radius (R).
- T²/R³=constant=4π²/GM;where
- G=6.67×10^ -11 Nm²/kg²
- M=mass of the foci body.
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