When a body of mass m is undergoing a circular motion of radius r around a body of mass M, the variation of the force of gravitation (F) with distance (r) is given as F = GMmrn
Then, the variation of the time period (T) with orbital distance (R) for a circular orbit will be
(A) T∝R n (B) T∝R –n (C) T∝R (n + 1)/2 (D) T∝R (n – 1)/2
Dear student
In the question the force is not clearly shown. Since the force is always inversely proportional to the distance 'r' then we will assume the force as
Now in the case of circular motion -
gravitational force = mass x centripetal acceleration , therefore
I hope it will help you
regards
In the question the force is not clearly shown. Since the force is always inversely proportional to the distance 'r' then we will assume the force as
Now in the case of circular motion -
gravitational force = mass x centripetal acceleration , therefore
I hope it will help you
regards