Kepler's third law states that the square of the period of revolution (T) of a planet around the sun is proportional to the third power of the average distance (r) between the sun and the planet, i.e., T² = Kr³, where K is a constant. If the masses of the sun and planet are M and m respectively, then as per Newton's law of gravitation, the force of attraction between them is F = GMm/r², where G is the gravitational constant. The relation between G and K is described as:<p></p>

Kepler's third law states that the square of the period of revolution (T) of a planet around the sun is proportional to the third power of the average distance (r) between the sun and the planet, i.e., T² = Kr³, where K is a constant. If the masses of the sun and planet are M and m respectively, then as per Newton's law of gravitation, the force of attraction between them is F = GMm/r², where G is the gravitational constant. The relation between G and K is described as:

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