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Learning objective

Understand that the subsequent stages in a star's life cycle depend on its mass: (a) a small mass star (similar to the Sun) evolves from red giant to white dwarf and planetary nebula; (b) a large mass star becomes a red supergiant, then a supernova, and may turn into a neutron star; (c) a very large mass star also becomes a red supergiant, then a supernova, and can form a black hole.

Read the explanation, check the common trap, then practise with flashcards and questions.

Exam focus

  • Read the explanation.
  • Check key terms.
  • Practise with linked questions.
Cambridge IGCSE Combined ScienceSpace physicsCore content

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Quick explanation

Understand that the subsequent stages in a star's life cycle depend on its mass: (a) a small mass star (similar to the Sun) evolves from red giant to white dwarf and planetary nebula; (b) a large mass star becomes a red supergiant, then a supernova, and may turn into a neutron star; (c) a very large mass star also becomes a red supergiant, then a supernova, and can form a black hole

  • This point belongs to Stars and the Universe, especially Stars and the Universe outcomes.
  • You need to be able to understand that the subsequent stages in a star's life cycle depend on its mass: (a) a small mass star (similar to the Sun) evolves from red giant to white dwarf and planetary nebula; (b) a large mass star becomes a red supergiant, then a supernova, and may turn into a neutron star; (c) a very large mass star also becomes a red supergiant, then a supernova, and can form a black hole.
  • The key ideas to know are Outline and Describe.
  • Use the linked flashcards and practice questions to check recall, then practise applying the idea in an exam-style answer.

Key concepts

OutlineDescribe

Why it matters

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Paper 3 structured question: Stars and the Universe

Paper 3Theory (Core)2 marks

Description

Star Life Cycle

Different mass stars evolve through distinct stages in their life cycles, leading to various end states.

  1. a

    Describe the life cycle of a small mass star and a large mass star.

    Aim for approximately 2 distinct marking points.

    [2]
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