Two planets of mass m1 and m2 are revolving around their sun in radius of their orbits r1 and r2 respectively. Angular momentum of planets are in ratio of 3 then \(\frac{T_1}{T_2}\) is (T1 and T2 are periods of revolutions)
(1) \(27(\frac{m_2}{m_1})^3\)
(2) \(\frac{1}{27}(\frac{m_2}{m_1})^3\)
(3) \((\frac{r_1}{r_2})^3\)
(4) \((\frac{r_2}{r_1})^{3/2}\)