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IB Physics IA idea · Space and astronomy data

IB Physics IA idea: test Kepler's third law with real satellite data

Hundreds of satellites share one law. Use their public orbital data to test it and weigh the Earth.

  • Space and astronomy data
  • SL ideal
  • HL ideal
  • Database Modelling Extended Essay potential
  • Syllabus: D.1, A.2

These ideas are starting points, not an IA to copy. Never copy an idea blindly: make the question, method and analysis your own, and check your plan with your teacher.

Example research question

To adapt, never to copy

How does the square of orbital period depend on the cube of orbital radius, from 6,800 km to 42,200 km, for 12 near-circular satellites with public two-line element sets, and what mass of the Earth follows?

Change the system, the range or the method so the question is yours. Check it against the research question checklist in our Physics IA guide.

Variables

You change
orbital radius, 6,800 to 42,200 km for 10 or more satellites
You measure
orbital period, 90 to 1,436 minutes
You keep the same
  • same central body
  • data epoch
  • elliptical versus circular
  • source of data

Method

Download two-line element sets for satellites at various altitudes (ISS, Starlink, GPS, geostationary) and compute period and semi-major axis. Choose near-circular orbits.

Data analysis

Plot T^2 against a^3; the gradient gives 4 pi^2/(G M_earth). Compare M_earth with the accepted value; include the effect of eccentricity as a systematic error.

How it works

You change Orbital radius cubed (km³) and measure Orbital period squared (min²) in Earth satellites, keeping Near-circular orbits, Data source, Epoch of data the same. Expect a graph of T² / min² against a³ / km³: The gradient gives 4π²/(GM_Earth).

Make it yours

Add Molniya or other highly elliptical orbits and test the semi-major-axis form.

Extended Essay angle

Include J2 precession and atmospheric drag decay of the orbit.

Safety

None.

Data sources

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