Step 1: Kepler's Third Law
From Kepler's Third Law "The square of the time period (T) of revolution of a planet around the sun in an elliptical orbit is directly proportional to the cube of its semi-major axis (r)"
T2∝r3
So, T21∝r31 and T22∝r32
∴ T2=T1(r2r1)32 ....(1)
Step 2: Time period Calculation
Given, Time period of first satellite T1=24hr
Orbiting radius of first satellite
r1=5R+R=6R
Orbiting radius of second satellite
r2=2R+R=3R
∴ From Equation (1), Time period of second satellite:
T2=24 hr(3R6R)32=242√2hours
T2=6√2 hours
Hence time period of another satellite in hours at height 2R from the surface of earth is 6√2 hours. Option (A)