Kepler's third law from Newton: a maths EPQ idea
A title to start from
How can Kepler's third law be derived from Newton's laws, and how well does it fit the planets and moons?
Why it works as an EPQ
A short derivation for circular orbits, then a log–log test on real data, then an evaluation of the approximations.
Scope and difficulty
Solid. Solid. Circular orbits derived; elliptical orbits discussed.
The maths
Builds on these A Level topics: Forces and Newton's laws · Kinematics · Exponentials and logarithms · Sampling and data.
You would learn:
- Circular motion
- Newton's law of gravitation
- Log–log graphs
One possible plan
- Derive T² ∝ r³ for circular orbits.
- Collect orbital data from a reliable source.
- Fit a power law on a log–log graph.
- Evaluate the circular-orbit assumption and the role of the central mass.
Pitfalls
- Data without units or sources.
- Calling the fit a proof.
Where to start reading
- NASA planetary fact sheets
- Search for: Kepler third law derivation circular orbit
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