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Question

Question: If the moon describes a circular path of radius ‘r’ around the earth with uniform angular speed \[\o...

If the moon describes a circular path of radius ‘r’ around the earth with uniform angular speed ω\omega , what will the time period of revolution of the moon be?
A. 2πr2gR22\pi \sqrt {\dfrac{{{r^2}}}{{g{R^2}}}}
B. 2πgR2r22\pi \sqrt {\dfrac{{g{R^2}}}{{{r^2}}}}
C. 2πgR3r32\pi \sqrt {\dfrac{{g{R^3}}}{{{r^3}}}}
D. 2πr3gR22\pi \sqrt {\dfrac{{{r^3}}}{{g{R^2}}}}

Explanation

Solution

In this question it has been given that the moon describes a circular motion around earth. Hence the moon experiences 2 forces: centripetal force and gravitational force. For the moon to keep moving in the orbit we will equate centripetal force to gravitational force as our first step, from there we find ω\omega and then we will find the time period.

Formula Used:
Gravitational force=FG=GMmr2{F_G} = \dfrac{{GMm}}{{{r^2}}}
Where G=gravitational constant, M=mass of planet, r=radius of planet
Centripetal force =FC=mω2r{F_C} = m{\omega ^2}r
time period T=T=2πωT = \dfrac{{2\pi }}{\omega }
and acceleration due to gravity, g=GMR2.................(1)g = \dfrac{{GM}}{{{R^2}}}.................(1)

Complete answer:
In the given question the moon is moving around the earth and to allow this motion we need to know that centripetal force will be equal to gravitational force to keep the moon revolving. If this condition is not satisfied the moon would not orbit around the earth.
Hence:
Fc=Fg{F_c} = {F_g}
mω2r=GMmr2m{\omega ^2}r = \dfrac{{GMm}}{{{r^2}}}
ω2=GMmmr3{\omega ^2} = \dfrac{{GMm}}{{m{r^3}}}
ω=GMmmr3\omega = \sqrt {\dfrac{{GMm}}{{m{r^3}}}}
ω=GMr3...............(2)\omega = \sqrt {\dfrac{{GM}}{{{r^3}}}} ...............(2)
And from equation 1 we see that GM=gR2GM = g{R^2} hence we will substitute this value in equation 2
ω=gR2r3\omega = \sqrt {\dfrac{{g{R^2}}}{{{r^3}}}}
We have found the value of angular frequency ω\omega , hence now we will find time period T.
T=2πωT = \dfrac{{2\pi }}{\omega }
T=2πgR2r3T = \dfrac{{2\pi }}{{\sqrt {\dfrac{{g{R^2}}}{{{r^3}}}} }}
T=2πr3gR2T = 2\pi \sqrt {\dfrac{{{r^3}}}{{g{R^2}}}}
Hence the period of revolution of the moon will be T=2πr3gR2T = 2\pi \sqrt {\dfrac{{{r^3}}}{{g{R^2}}}}
Hence the correct answer to this question is option D.

Note: We can also solve this question taking frequency into consideration, as ω=2πf\omega = 2\pi f where ω\omega is angular frequency and f is frequency. After finding ω\omega we will find frequency. The time period is given by T=1fT = \dfrac{1}{f} and then we will solve the time period.