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Physics · Theme E: Nuclear and quantum physics

E.5 — Fusion and stars

Physics · SL / HL · syllabus-mapped notes

  1. Fusion in stars

    Stellar equilibrium, fusion as a star’s energy source, the conditions for it, and stellar evolution.

  2. The Hertzsprung–Russell diagram

    The main regions of the HR diagram and the properties of stars in each.

  3. Measuring stars

    Stellar parallax and distance units, and determining stellar radii from luminosity and temperature.

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