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IGCSE · Cambridge (CIE) · 0625

Explain hydrogen fusion as the stable star energy source

Explain that stable stars release nuclear energy through hydrogen fusion into helium.

Sun as a star pathway · 6.2.1

Extended only (Supplement); Physics 0625, 2026–2028. Use supplied distances, periods and stated orbital models. Drawings are not to scale. Written practice is self-checked.

Before you begin

  • Distinguish atoms from nuclei.
  • Recall fusion and fission as different nuclear processes.

Work on paper. Try each question before revealing help, and explain why your method works.

Quick readiness check

What happens in fusion?

What you will learn

  • Explain that stable stars release nuclear energy through hydrogen fusion into helium.
  • Separate nuclear fusion from chemical burning, fission and gravitational contraction.
The sequence represents net hydrogen fusion and released energy, not a complete single-step nuclear equation.Stable-stage nuclear fusionHydrogen nucleiNuclear reactionsNet product: heliumEnergy is releasedStable-stage radiationFinite nuclear fuel
The sequence represents net hydrogen fusion and released energy, not a complete single-step nuclear equation.

Identify the nuclear change

In a stable hydrogen-fusing star, nuclear reactions combine hydrogen nuclei through a sequence whose net product is helium. Energy released by those reactions sustains the star’s radiation. This is fusion: small nuclei combine, rather than a large nucleus splitting as in fission.

The sequence has intermediate reactions and other particles. A simple hydrogen-to-helium arrow is a net process, not one instantaneous collision between four neutral atoms. Detailed reaction chains, binding-energy calculations and neutrino balances are beyond this requirement.

Separate heating stages and fuel supplies

A protostar heats as its gas contracts under gravity before sustained hydrogen fusion is established. Gravitational contraction therefore matters for formation, but it is not the principal continuing energy source of the stable hydrogen-fusing stage.

Chemical burning needs chemical reactants and rearranges electron bonds; stellar hydrogen fusion changes nuclei and does not need external oxygen. The star’s fuel is finite. Stable means a long-lived approximate balance, not an unlimited energy source or unchanging properties forever.

Pause and explain

What powers the stable hydrogen-fusing stage?

Put the idea to work

Worked example

A learner says the Sun shines because hydrogen burns with oxygen. Replace the mechanism.

Show the worked solution
  1. Identify a nuclear rather than chemical process.
  2. Hydrogen nuclei take part in fusion to form helium.
  3. The reactions release energy that supports radiation.

Answer Nuclear fusion of hydrogen into helium releases energy; ordinary oxygen burning is not the mechanism.

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From guided practice to a new situation

Write your answer and reasoning first. Use a hint only if you are stuck. The model solution is for self-checking; your written work is not automatically marked.

1 · Guided

State the stellar fuel, net product and energy mechanism.

Give me a hint

Answer three separate parts: starting nuclei, ending nuclei and process.

Compare my reasoning
  1. Start with hydrogen nuclei.
  2. Identify helium as the net product.
  3. Name energy-releasing nuclear fusion.

Hydrogen; helium; energy-releasing nuclear fusion.

Look for these in your work

  • Name nuclei or a nuclear reaction.
  • Distinguish fuel from product.
2 · Independent

Compare a collapsing protostar with a stable hydrogen-fusing star.

Give me a hint

Do not give both stages the same principal energy source.

Compare my reasoning
  1. Contraction increases the protostar temperature.
  2. Sustained nuclear reactions power the stable stage.
  3. Both statements concern different evolutionary conditions.

Formation heating is gravitational contraction; stable-stage energy is nuclear fusion.

Look for these in your work

  • Retain the stage boundary.
  • Name both mechanisms.
3 · Transfer

A cartoon joins four H icons into one He icon without intermediates. Explain its use and limit.

Give me a hint

A net arrow does not describe every reaction step or emitted particle.

Compare my reasoning
  1. It represents hydrogen conversion into helium.
  2. It identifies the nuclear energy source.
  3. It omits intermediate reactions and particles.

Useful as a net fusion model; not a complete single-collision reaction equation.

Look for these in your work

  • Explain the retained idea.
  • State the omitted detail.

Common mistakes

  • Fusion is not fission.
  • Fusion is not oxygen burning.
  • A net arrow is not a complete reaction chain.
Recall without your notes

What can you explain now?

What powers the stable hydrogen-fusing stage?

Compare with the explanation

Nuclear fusion forming helium

Nuclear reactions release energy while hydrogen nuclei are converted into helium.

After trying it yourself, choose your next review. This is your self-assessment.

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Make it stick

Separate nuclear fusion from chemical burning, fission and gravitational contraction.

If you needed the solution, close it and solve the problem again from a blank page. A correct answer is stronger when you can explain the reason for each step.

Keep learning Physics

Course scope and assessment

491 sequenced Physics lessons provide 1473 guided, independent and application problems. 58 of 58 syllabus sections have full linked teaching sequences; 0 sections remain pending. Three earlier starter overviews remain available but are not counted as full sequences. The map covers all six subject areas for 2026–2028 and keeps review and assessment limits visible. This is available content, not full programme completion, an exam grade or certified mastery. Written practice is self-checked. Supervised practical experience, cumulative assessment and human subject-teacher review remain pending. Paper method exercises do not demonstrate practical competence or complete either practical-assessment route.

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