A planet of mass M, has two natural satellites with masses m 1 and m 2 . The radii of their circular orbits are R 1 and R 2 respectively. Ignore the gravitational force between the satellites. Define v 1 ,L 1 ,K 1 and T 1 to be respectively, the orbital speed, angular momentum, kinetic energy and time period of revolution of satellite 1; and v 2 ,L 2 ,K 2 and T 2 to be the corresponding quantities of satellite 2. Given m 1 /m 2 = 2 and R 1 /R 2 = 1/4, match the ratios in List – I to the numbers in List -II.
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