The Life Cycle of Solar Mass Stars (Edexcel IGCSE Science (Double Award))

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The life cycle of solar mass stars

  • All stars, including the Sun, began as a cloud of dust and gas

  • Once a star has formed, it will spend its life going through a sequence of evolutionary stages, known as the life cycle of a star

Summary of the life cycles of stars

Lifecycle of stars 1, downloadable IGCSE & GCSE Physics revision notes

Flow diagram showing the life cycle of a star which is the same size as the Sun (solar mass) and the lifecycle of a star which is much more massive than the Sun

Star formation

  • All stars follow the same initial stages:

Nebula → protostar → main sequence star

Nebula

  • Stars form from a giant interstellar cloud of gas and dust called a nebula

Protostar

  • The force of gravity within a nebula pulls the particles closer together until a hot ball of gas forms, known as a protostar

  • As the particles are pulled closer together the density of the protostar will increase

  • This results in more frequent collisions between the particles which causes the temperature to increase

Main sequence star

  • Once the protostar becomes hot enough, nuclear fusion  reactions occur within its core

  • Once a star initiates fusion, it is known as a main-sequence star

  • During the main sequence, the star is in equilibrium and said to be stable

The life cycle of a solar mass star

  • After the main sequence, a low-mass star finishes its life cycle in the following evolutionary stages:

Red giant → planetary nebula → white dwarf

Red giant

  • After several billion years, the hydrogen causing the fusion reactions in the star will begin to run out

  • Once this happens, the fusion reactions in the core will start to die down

  • The star will begin to fuse helium which causes the outer part of the star to expand

  • As the star expands, its surface cools and it becomes a red giant 

White dwarf

  • Once the helium fusion reactions have finished, the star collapses and becomes a white dwarf

  • The white dwarf cools down over time and as a result, the amount of energy it emits decreases

The life cycle of a low-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

Examiner Tips and Tricks

Make sure you remember the life cycle for a solar mass star and ensure you can describe the sequence in a logically structured manner in case a 6 marker comes up in the exam!

Ensure you can remember the end stages for a solar mass star clearly (red giant, planetary nebula, white dwarf) as this is different for a star that is much larger than our Sun!

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Ashika

Author: Ashika

Expertise: Physics Project Lead

Ashika graduated with a first-class Physics degree from Manchester University and, having worked as a software engineer, focused on Physics education, creating engaging content to help students across all levels. Now an experienced GCSE and A Level Physics and Maths tutor, Ashika helps to grow and improve our Physics resources.