Step 1: Given that:
Time of revolution of the satellite around earth = T
Depends on = The universal gravitational constant G, the mass of Earth M, and the radius of circular orbit R.
Step 2: Determining the expression for T:
Let, the time of revolution of the satellite around the earth(T) depends on power a of The universal gravitational constant G, power b of the mass of the earth and power c of the radius of circular orbit R.
That is; T∝GaMbRc
Now,
T∝GaMbRc
T=kGaMbRc.........(1)
Writing the dimensions of the quantities on both sides, we get;
[T]=[M−1L3T−2]a[M]b[L]c
[T]=[M−a+bL3a+cT−2a]
Comparing the powers of similar quantities on both sides, we get
−a+b=0
3a+c=0
−2a=1
Solving these equations, we get;a=−12
b=−12
c=32
Putting these values in equation (1), we get;T=kG−12M−12R32
T=kR32G12M12
T=k√R3√GM
T=k√R3GM
Thus,