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. LIST-I: P. v₁/v₂; Q. L₁/L₂; R. K₁/K₂; S. T₁/T₂. LIST-II: 1. 1/8; 2. 1; 3. 2; 4. 8.