Kepler's third law of planetary motion states that :(Symbols have their usual meaning)
A
V0=√Rg
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B
→F12=−→F21
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C
r2∝T3
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D
r3∝T2
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Solution
The correct option is Dr3∝T2 According to kepler's third law of planetary motion, The square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit. ⇒T2∝R3