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NEET UG PHYSICS MCQ: GRAVITATION

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According to Kelper’s law of planetary motion if T represent time period and rr is orbital radius, then for two planets these are related as
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Correct option: D
(T1T2)2=(r1r2)3{\left( {\frac{{{T_1}}}{{{T_2}}}} \right)^2} = {\left( {\frac{{{r_1}}}{{{r_2}}}} \right)^3}
Option D ((T1T2)2=(r1r2)3{\left( {\frac{{{T_1}}}{{{T_2}}}} \right)^2} = {\left( {\frac{{{r_1}}}{{{r_2}}}} \right)^3}) is correct because it represents Kepler's Third Law, relating the period and orbital radius of two planets.

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