Kepler’s third law states that square of period of revolution (T) of

1.	Kepler’s third law states that square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance r between sun and planet i.e. T2=Kr3 where K is constant.If the masses of sun and planet are M and m respectively then as per Newton’s law of gravitation force of attraction between them is F=GMmr2 , here G is gravitational constant The relation between G and K is described as:
Answer» Kepler’s third law states that square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance r between sun and planet i.e. $T^{2} = K r^{3}$ where K is constant.If the masses of sun and planet are M and m respectively then as per Newton’s law of gravitation force of attraction between them is $F = \frac{G M m}{r^{2}}$ , here G is gravitational constant The relation between G and K is described as:

Kepler’s third law states that square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance r between sun and planet i.e. T2=Kr3 where K is constant.If the masses of sun and planet are M and m respectively then as per Newton’s law of gravitation force of attraction between them is F=GMmr2 , here G is gravitational constant The relation between G and K is described as:

Answer»

Kepler’s third law states that square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance r between sun and planet i.e. $T^{2} = K r^{3}$ where K is constant.If the masses of sun and planet are M and m respectively then as per Newton’s law of gravitation force of attraction between them is $F = \frac{G M m}{r^{2}}$ , here G is gravitational constant

The relation between G and K is described as:

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