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 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 F = GMmr2, here G is gravitational constant. The relation between G and K is described as
- K = G
- K = 1G
- GK = 4 2
- GMK = 4 2
Answer
(4) GMK = 4 2
Solution
The gravitational force provides the centripetal force:
GMmr2 = m 2 r = m ( 2 T )2 r
T2 = 4 2GMr3
Comparing with T2 = Kr3: K = 4 2GM
GMK = 4 2
Answer: (4)