(a) State Kepler’s third law of planetary motion. (b) Explain qualitatively how the…

PHYSICS · Subjective · A Level · Physics · Fields and their consequences · Fields and their consequences

Problem

(a) State Kepler’s third law of planetary motion. (b) Explain qualitatively how the balance between the gravitational attraction of the Sun on a planet and the centripetal requirement of uniform circular motion leads to the proportionality T2∝r3T^{2}\propto r^{3}. (c) Why does this proportionality imply that planets farther from the Sun move more slowly along their orbits than the inner planets?

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