A satellite of mass m revolves around the earth of radius R at a height x from its surface. If g is the acceleration due to gravity on the surface of the earth, the orbital speed of the satellite is
A
√gx
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B
√gRR−x
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C
√gR2R−x
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D
√gR2R+x
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Solution
The correct option is D√gR2R+x
We have:
mv2R+x=GMm(R+x)2⇒v=√GMR+x=√GMR2×R2R+x=√gR2R+x
because the gravitational force provides the centripetal force for revolution.