Life Cycle of a Star (CIE IGCSE Physics: Co-ordinated Sciences (Double Award))

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Katie M

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Katie M

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Life cycle of a star

Small mass star

  • A small mass star is one which has a similar mass as the Sun
  • After the stable star stage, a small mass star finishes its life cycle in the following evolutionary stages:

red giant → planetary nebula + white dwarf

  • Red giant:
    • Formed when a small mass star reaches the end of its life 
    • The outer layers of the star expand and cool
  • Planetary nebula:
    • Formed when the outer layers of the star are pushed away
  • White dwarf:
    • Formed when the core of the star collapses
    • Found at the centre of a planetary nebula

The life cycle of a small mass star

Lifecycle of Solar mass stars, downloadable IGCSE & GCSE Physics revision notes

The life cycle of a star that is similar to our Sun

Large mass star

  • A large mass star is one with a larger mass than the Sun
  • After the stable star stage, a large mass star finishes its life cycle in the following evolutionary stages:

red supergiant → supernova → neutron star

  • Red supergiant:
    • Formed when a large (or very large) mass star reaches the end of its life 
    • The outer layers of the star expand and cool
  • Supernova:
    • An exploding red supergiant
  • Neutron star:
    • Formed when the core of a large star collapses
    • Very dense, but not as much as a black hole

Very large mass star

  • A very large mass star is one with a much larger mass than the Sun
  • After the stable star stage, a very large mass star finishes its life cycle in the following evolutionary stages:

red supergiant → supernova → black hole

  • Black hole:
    • Formed when the core of a very large star collapses
    • Extremely dense

The life cycle of a large mass star

Lifecycle of Larger Mass Stars, downloadable IGCSE & GCSE Physics revision notes

The life cycle of a star much larger than our Sun

Formation of new stars and planets

Extended tier only

  • The nebula from a supernova may form new stars with orbiting planets
    • The heaviest elements (elements heavier than iron) are formed during a supernova and are ejected into space
    • These nebulae may form new planetary systems

A supernova

Supernova

The nebula formed from a supernova may eventually form new stars with orbiting planets

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Katie M

Author: Katie M

Expertise: Physics

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.