WJEC A-Level Physics 1420QS
Basic Physics
Kinematics
Dynamics
Energy Concepts
Solids Under Stress
Using Radiation to Investigate Stars
Particles and Nuclear Structure
Conduction of Electricity
Resistance
D.C. Circuits
The Nature of Waves
Wave Properties
Refraction of Light
Photons
Lasers
Circular Motion
Vibrations
Kinetic Theory
Thermal Physics
Nuclear Decay
Nuclear Energy
Capacitance
Electrostatic and Gravitational Fields of Force
Orbits and the Wider Universe
Magnetic Fields
Electromagnetic Induction
Option A: Alternating CurrentsOption A
Option B: Medical PhysicsOption B
Option C: The Physics of SportsOption C
Option D: Energy and the EnvironmentOption D
Mathematical Requirements (Appendix C)
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.
What you need to know
Answer each one before you reveal it.
Write Kepler's third law as a proportionality.
State the constant of proportionality in T² = kr³.
Questions from this subtopic
Each one with the model answer underneath.
- 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
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
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
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
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
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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