BITSAT 2016 Paper

(T) of a planet around the sun, is proportional to third powerof average distance r between sun and planet i.e. T2=Kr3here 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=

GMm

r2

, here G is gravitational constant. The relation between G and K is described as