For every planet orbiting the Sun

PHYSICS · Single correct · A Level · Physics · Fields and their consequences · Fields and their consequences

Problem

For every planet orbiting the Sun, the ratio T2a3\dfrac{T^{2}}{a^{3}} (where TT is the orbital period and aa is the semi-major axis) is (a) directly proportional to the planet’s mass (b) greater for planets that are farther from the Sun (c) the same constant for all planets (d) zero for perfectly circular orbits

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