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Define the term orbital velocity. Establish a relation for the orbital velocity of a satellite very close to the surface of the earth. Find the ratio of orbital velocity and escape velocity.

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Orbital velocity is the minimum velocity that is needed to put the satellite into a given orbit around Earth. Consider a satellite of mass ‘m’ moving around in an orbit at height ‘h’ above the ground. Let M be mass of Earth, R be the radius of earth and the orbital velocity be Vo.

We know that, Fg\(\frac{GMm}{(R+h)^2}\)

and centrifugal force FC\(\frac{GV_o^2}{(R+h)}\)

In equilibrium i.e., while rotating around the orbit

(Since, h << R ; R + h = R)

\(\frac{V_o}{V_{esc}} \) \(\frac {\sqrt {gR}}{\sqrt {2gR}} = \frac {1} {\sqrt2}\).

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