Expression for critical velocity:

Let,
M = mass of the earth
R = radius of the earth
h = height of the satellite from the earth’s surface
m = mass of the satellite
vc = critical velocity of the satellite in the given orbit
r = (R + h) = radius of the circular orbit
For the circular motion of the satellite, the necessary centripetal force is given as,
FCP = \(\frac{mv^2_c}{r}\) ..........(1)
The gravitational force of attraction between the earth and the satellite is given by,
FG = \(\frac{GMm}{r^2}\) ...........(2)
Gravitational force provides the centripetal force necessary for the circular motion of the satellite.
∴ FCP = FG
∴ \(\frac{mv^2_c}{r}\) = \(\frac{GMm}{r^2}\) ….[From equations (1) and (2)]
∴ \(v^2_c\) = \(\frac{Gm}{r}\)
∴ vc = \( \sqrt{\frac{GM}{r}}\) .......(3)
But, r = R + h
∴ vc = \( \sqrt{\frac{GM}{r+h}}\) .......(4)
Also, GM = gh (R + h)2
where, gh is acceleration due to gravity at height ‘h’ above earth’s surface.
∴ vc = \( \sqrt{g_h(R+H)}\) .......(5)
Equations (4) and (5) represent critical velocities of satellite orbiting at a certain height above the earth’s surface.