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IGCSE · Cambridge (CIE) · 0625

Trace the planetary nebula and white dwarf branch

Follow a less-massive red giant into expelled material surrounding a white dwarf remnant.

Stars and stellar evolution pathway · 6.2.2

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

  • Recall the mass-dependent giant branches.
  • Distinguish a gas cloud from a compact object.

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

Quick readiness check

Which branch follows a less-massive red giant?

What you will learn

  • Follow a less-massive red giant into expelled material surrounding a white dwarf remnant.
  • Distinguish the planetary nebula cloud from the central remnant and from planets.
The cloud and remnant coexist after shedding; the cards do not imply the cloud becomes the central white dwarf.Less-massive stellar endpointLess-massive branchRed giantPlanetarynebulaShed gasWhite dwarfCentralremnantCloud and remnant are separateSchematic · no time or mass scale
The cloud and remnant coexist after shedding; the cards do not imply the cloud becomes the central white dwarf.

Follow the less-massive route

In the syllabus’s less-massive route, a red giant sheds outer material that forms a planetary nebula. A white dwarf remains at its centre. The cloud and remnant are different outcomes from different parts of the evolved star; the white dwarf is not the whole extended nebula.

Despite its name, a planetary nebula is not a newly created planet or the collection of ordinary planets in a Solar System. The historical name describes an observed appearance, not a planetary classification.

Keep the endpoint distinct

A white dwarf is a compact stellar remnant that can radiate stored thermal energy as it cools. Its appearance does not imply continuing central hydrogen fusion like the earlier stable stage. Nor is a Sun-like star expected to follow the massive-star supernova branch in this syllabus model.

A schematic arrow gives evolutionary ordering, not an instantaneous event or a diagram whose equal boxes measure equal durations, radii or masses. Use the initial-mass condition when selecting this route.

Pause and explain

Is a planetary nebula a planet?

Put the idea to work

Worked example

Label the extended cloud and compact centre after a less-massive red giant sheds its outer layers.

Show the worked solution
  1. Identify expelled outer material.
  2. Name the surrounding planetary nebula.
  3. Name the central white dwarf remnant.

Answer Cloud: planetary nebula; centre: white dwarf.

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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

Complete stable less-massive star → red giant → __ with __ at its centre.

Give me a hint

Identify the expelled cloud separately from the compact remnant.

Compare my reasoning
  1. Follow the less-massive condition.
  2. Name a planetary nebula as the cloud.
  3. Name a white dwarf at the centre.

Planetary nebula with a white dwarf at its centre.

Look for these in your work

  • Name both outcomes.
  • Keep cloud and centre separate.
2 · Independent

Explain why the phrase planetary nebula does not prove a new planet has formed.

Give me a hint

Use the physical origin, not the sound of its historical name.

Compare my reasoning
  1. Material is shed from an evolved star.
  2. It forms an extended gas cloud.
  3. The centre is a stellar remnant, not evidence of a new planet.

It describes expelled stellar gas; the name does not establish planet formation.

Look for these in your work

  • State the cloud origin.
  • Avoid name-based classification.
3 · Transfer

A Sun-like star is placed on a poster ending in a supernova and black hole. Repair the route.

Give me a hint

Select the less-massive branch before choosing its endpoint.

Compare my reasoning
  1. Use a red-giant stage.
  2. Then identify a planetary nebula.
  3. Place a white dwarf at the centre.

Sun-like stable star → red giant → planetary nebula and central white dwarf.

Look for these in your work

  • Use the correct branch.
  • Include both cloud and remnant.

Common mistakes

  • Planetary nebula does not mean planet.
  • White dwarf and nebula are distinct.
  • The Sun-like branch does not end in a massive-star supernova.
Recall without your notes

What can you explain now?

Is a planetary nebula a planet?

Compare with the explanation

No; it is expelled gas surrounding a remnant

The name does not classify the cloud as an orbiting rocky or giant planet.

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

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Make it stick

Distinguish the planetary nebula cloud from the central remnant and from planets.

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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