Time period of the satellite is given as
\(T = \frac{2π(R+h)^{3/2}}{\sqrt{GM}}\)
When the height of the satellite is h1, it takes T time to revolve around the Earth. Thus, at height h1
∴ \(T = \frac{2π(R+h_1)^{3/2}}{\sqrt{GM}}\) .... (i)
When the satellite takes \(2\sqrt{2}T\) time to revolve around the Earth, let it be at height h2. Thus,
\(2\sqrt{2}T =\frac{2π(R+h_2)^{3/2}}{\sqrt{GM}}\) .....(ii)
Dividing (ii) by (i), we get
\(2\sqrt{2} =\frac{(R+h_2)^{3/2}}{(R+h_1)^{3/2}}\)
\(2^{3/2} =\frac{(R+h_2)^{3/2}}{(R+h_1)^{3/2}}\)
\(2 =\frac{(R+h_2)}{(R+h_1)}\)
2R+2h1 = R+h2
∴ h2=R+2h1