Correct Answer - Option 4 : T ∝ R
3/2
CONCEPT:
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Kepler's Third Law: The square of the time period of a planet is directly proportional to the cube of the distance of its orbit.
T2 α R3
where T is the time period and R is the mean distance of the planet from the sun.
EXPLANATION:
According to Kepler's Law, planets' time period varies with their radius as given below:
T2 α R3
i.e. T ∝ R3/2
So the correct answer is option 4.