The orbital velocity of a satellite revolving near a planet is.
A
directly proportional to density of planet
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B
directly proportional to square root of density of planet
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C
directly proportional to cube of density of planet
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D
directly proportional to square of density of planat
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Solution
The correct option is B directly proportional to square root of density of planet Orbital velocity, v=√GMr where r is the orbital radius and M is the mass of planet.
Now let density of planet be ρ
Thus, M=ρ×43πR3 where R is the radius of the planet