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8.1.4Space Physics

Production of Elements — Oxford AQA International GCSE Combined Science - Physics Revision Notes & Topical Questions

5 min read 6 parts Lesson 5 of 10

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Part 1 of 4Stars as element factories

Source of energy
  • Source of energy Fusion reactions in the core of a star release the energy that makes it shine.
Source of elements
  • Source of elements The same reactions build heavier nuclei from lighter ones, so stars made all the naturally occurring elements.
The early Universe
  • The early Universe Before any stars existed there was no fusion, so the early Universe contained only hydrogen.
    • Every heavier element had to be made later in stars.

Part 2 of 4Life of a star larger than the Sun

1Main sequence
  • Main sequence Hydrogen nuclei fuse to form helium nuclei, releasing large amounts of energy.
    • The huge supply of hydrogen lets the star shine steadily for millions of years.
2Hydrogen runs out
  • Hydrogen runs out When the hydrogen in the core is used up, fusion slows and the core contracts.
    • The cooler outer layers swell and glow redder, so the star becomes a red supergiant.
3Heavier fusion
  • Heavier fusion Helium nuclei fuse to form carbon.
    • Further fusion makes nuclei such as nitrogen and oxygen, and heavier elements up to iron.
4Core collapse
  • Core collapse When fusion can no longer continue, the core collapses suddenly.
5Supernova
  • Supernova The outer layers are blown away in a gigantic explosion called a supernova.

Part 3 of 4What a supernova does

1
The sudden collapse of the core triggers an explosion that throws the outer layers of the star into space.
2
Temperatures inside the explosion are so high that nuclei can fuse to form elements heavier than iron.
3
All the elements heavier than iron are created in supernovae.
4
The explosion scatters these elements, along with those made earlier, out into space.
5
The material can later gather in new clouds of gas and dust, from which new stars and their planets can form.

Part 4 of 4Where elements are made

StageElements formed
Early Universe, before starsHydrogen only
Main sequence starHelium, from the fusion of hydrogen
Red supergiantCarbon, nitrogen, oxygen and heavier nuclei up to iron
SupernovaElements heavier than iron, and dispersal of all the elements

Key terms

TermMeaning
Red supergiantA very large, cool, red star formed when a massive star runs out of hydrogen in its core.
SupernovaThe explosion of a massive star at the end of its life, which scatters elements into space.
Nuclear fusionThe joining of light nuclei to form a heavier nucleus, releasing energy.
Main sequenceThe stable stage of a star's life in which hydrogen is fused to helium.
Naturally occurring elementAn element found in nature, as opposed to one made artificially in a laboratory.

Avoid these mistakes

1
Saying that elements heavier than iron are made in the red supergiant stage. They form in the extreme conditions of a supernova.
2
Believing that the Big Bang made all the elements. The early Universe contained only hydrogen; fusion in stars made the rest.
3
Forgetting that the supernova also spreads the elements. Without the explosion the new elements would stay locked inside the star.
4
Describing the red supergiant as hotter than the main sequence star. Its surface expands and cools, which is why it looks redder.
5
Writing that stars run out of energy because the hydrogen has burned. It is used up in fusion reactions, not by burning.

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