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Ch 24 E.5 Fusion and stars: complete notes

Neat, exam-ready notebook-style notes for Ch 24 E.5 Fusion and stars, following the IB Diploma syllabus, SL and HL. This chapter is part of the complete Physics Notes for IB Diploma Students (SL and HL): All 24 Topics.

Cover of Physics Notes for IB Diploma Students (SL and HL): All 24 Topics
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Free preview: Ch 24 E.5 Fusion and stars notes

A quick look at the chapter from our IB Diploma Physics notes. The full chapter notes have the detailed explanations, diagrams and practice questions with answers.

Topics in this chapter

  1. What you must be able to do
  2. Why stars are stable
  3. Fusion: the energy source
  4. Stellar evolution
  5. The Hertzsprung–Russell (HR) diagram
  6. Luminosity, temperature and radius
  7. Stellar parallax and distance units

“I can” checklist: what you must be able to do

  • I can explain stellar equilibrium, and the conditions needed for fusion.
  • I can calculate the energy released in a fusion reaction and the rate of fusion in a star.
  • I can describe how a star's mass decides its evolution and end state.
  • I can sketch and interpret an HR diagram, including lines of constant radius.
  • I can use parallax to find distances, and convert between AU, ly and pc.
  • I can find a star's radius from its luminosity and surface temperature, and its temperature from its spectrum.

What is inside the full chapter notes

  • Concept notes with 8 worked examples
  • Figures: equilibrium, HR diagram, parallax
  • Common mistakes; investigation (IA) ideas
  • 15 Paper 1A-style MCQs, explained
  • 3 Paper 2-style structured questions with mark schemes, plus a data-based question
  • Quick-reference sheet and "I can" checklist
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What you get in the pack

All chapters in this pack

  1. Ch 1 A.1 Kinematics
  2. Ch 2 A.2 Forces and momentum
  3. Ch 3 A.3 Work, energy and power
  4. Ch 4 A.4 Rigid body mechanics
  5. Ch 5 A.5 Galilean and special relativity
  6. Ch 6 B.1 Thermal energy transfers
  7. Ch 7 B.2 Greenhouse effect
  8. Ch 8 B.3 Gas laws
  9. Ch 9 B.4 Thermodynamics
  10. Ch 10 B.5 Current and circuits
  11. Ch 11 C.1 Simple harmonic motion
  12. Ch 12 C.2 Wave model
  13. Ch 13 C.3 Wave phenomena
  14. Ch 14 C.4 Standing waves and resonance
  15. Ch 15 C.5 Doppler effect
  16. Ch 16 D.1 Gravitational fields
  17. Ch 17 D.2 Electric and magnetic fields
  18. Ch 18 D.3 Motion in electromagnetic fields
  19. Ch 19 D.4 Induction
  20. Ch 20 E.1 Structure of the atom
  21. Ch 21 E.2 Quantum physics
  22. Ch 22 E.3 Radioactive decay
  23. Ch 23 E.4 Fission
  24. Ch 24 E.5 Fusion and stars
← Ch 23 E.4 Fission