A planet of mass M, has two natural satellites with masses m1 ​ and m2 ​ . The radii of their circular orbits are R1 ​ and R2 ​ respectively. Ignore the gravitational force between the satellites. Define v1 ​ ,L1 ​ ,K1 ​ and T1 ​ to be, respectively, the orbital speed, angular momentum, kinetic energy and time period of revolution of satellite 1; and v2,L2,K2 ​ and T2 ​ to be the corresponding quantities of satellite 2. Given m1/m2=2 and R1/R2=1/4, match the ratios in List - I to the numbers in List-II.