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According to Kepler, the period of revolution of a planet ( T ) and its mean distance from the sun ( r ) are related by the equationA. `T^(2)r`= ConstantB. `T^(2)r^(-3)=` ConstantC. `T^(2)r^(3)="Constant"`D. `T^(3)r^(3)=` Constant |
Answer» Correct Answer - b `T^(2)=(4pi^(2))/(GM)r^(3)` `(T^(2))/(T^(3))=(4pi^(2))/(GM)="constant"` `T^(2)r^(-3) = "constant."` |
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