Question

Kepler's third law states that square of pero
revolution (T) of a planet around the sun, is
proportional to third power of average distancer
between sun and planet, i.e., T2 = kry, here 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
Fun, here G is gravitational constant. The
relation between G and K is described as
(AIPMT-2015]
(2) GK = 472
(1) Kaa
(3) GMK = 472
(4) K = G​

Answer 1

Answer:

Kepler's third law states that square of the period of revolution (T) of a planet around the sun, is proportional to the third power of average distance r between the sun and planet i.e, T2 =Kr3, here K is constant.