An artificial satellite is revolving around a planet of mass M and radius R, in a circular orbit of radius r. From Kepler’s third law about the period of a satellite around a common central body, square of the period of revolution T is proportional to the cube of the radius of the orbit r. Show using dimensional analysis, that T = k/R √r3/g where k is a dimensionless constant and g is acceleration due to gravity.
An artificial satellite is revolving around a planet of mass M and radius R, in a circular orbit of radius r. From Kepler’s third law about the period of a satellite around a common central body, square of the period of revolution T is proportional to the cube of the radius of the orbit r. Show using dimensional analysis, that T = k/R √r3/g where k is a dimensionless constant and g is acceleration due to gravity.

Kepler’s third law states that,

T^{2} \propto a^{3} i.e., square of time period \left(T^{2}\right) of a satellite revolving around a planet, is proportional to the cube of the radius of the orbit \left(a^{3}\right).

On applying Kepler’s third law,

T^{2} \propto r^{3} \Rightarrow T \propto r^{3 / 2}

Also, T depends on R and g.

Let T \propto r^{3 / 2} g^{a} R^{b}
\Rightarrow \quad T=k r^{3 / 2} R^{a} g^{b}…..(i)

where,
k= dimensionless constant.

On writing the dimensions of various quantities on both the sides, we get

\begin{aligned} \left[M^{0} L^{0} T\right] &=[L]^{3 / 2}\left[L T^{-2}\right]^{a}[L]^{b} \\ &=\left[M^{0} L^{a+b+3 / 2} T^{-2 a}\right] \end{aligned}

Comparing the dimensions of both sides,

a+b+\frac{3}{2}=0…..(ii)

-2=a \quad \Rightarrow \quad a=-1 / 2…..(iii)

From Eq. (ii), we get

b-\frac{1}{2}+\frac{3}{2}=0 \Rightarrow b=-1

Putting the values of a and b in Eq. (i), we get

T=k r^{3 / 2} R^{-1} g^{-1 / 2} \Rightarrow T=\frac{k}{R} \sqrt{\frac{r^{3}}{g}}