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Orbits and the Wider Universe

Deriving Kepler's third law

  • 3 things to know
  • A2 Unit 4 Section A

Overview

Recall questions on Deriving Kepler's third law.

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Key term

State Kepler's third law.

Key term

Write Kepler's third law as a proportionality.

Key term

State the constant of proportionality in T² = kr³.

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    State Kepler's third law.

    Model answer

    The square of a planet's orbital period is proportional to the cube of its mean orbital radius.

  2. 2

    Write Kepler's third law as a proportionality.

    Model answer

    T² is proportional to r³, where T is the orbital period and r the mean orbital radius.

  3. 3

    Set out the derivation of Kepler's third law for a circular orbit.

    Model answer

    Setting GMm/r² equal to mrω² and cancelling m gives GM/r² = rω², and substituting ω = 2π/T then rearranging gives T² = 4π²r³/(GM).

  4. 4

    State the constant of proportionality in T² = kr³.

    Model answer

    k is 4π² divided by GM, where M is the mass of the central body.

  5. 5

    Why is the constant different for the moons of Jupiter?

    Model answer

    The central mass in the expression is Jupiter's rather than the Sun's, and the two differ.

  6. 6

    What is plotted to test Kepler's third law as a straight line?

    Model answer

    The square of the period against the cube of the orbital radius, which gives a straight line through the origin.

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