Learning objective
Explain the stages in the life cycle of a star, including: the formation from interstellar gas and dust containing hydrogen, the development of a protostar from a collapsing interstellar cloud, the stabilization of a star when gravitational forces are balanced by thermal pressure, the depletion of hydrogen as fuel for nuclear reactions, the expansion of most stars into red giants or red supergiants after hydrogen is converted to helium, the formation of a planetary nebula and white dwarf from a less massive star, the supernova explosion of a red supergiant leading to a nebula with new elements, and the potential for new stars and planets to form from the supernova remnants.
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 PhysicsSpace physicsSupplement content