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
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
| Stage | Elements formed |
|---|---|
| Early Universe, before stars | Hydrogen only |
| Main sequence star | Helium, from the fusion of hydrogen |
| Red supergiant | Carbon, nitrogen, oxygen and heavier nuclei up to iron |
| Supernova | Elements heavier than iron, and dispersal of all the elements |
Key terms
| Term | Meaning |
|---|---|
| Red supergiant | A very large, cool, red star formed when a massive star runs out of hydrogen in its core. |
| Supernova | The explosion of a massive star at the end of its life, which scatters elements into space. |
| Nuclear fusion | The joining of light nuclei to form a heavier nucleus, releasing energy. |
| Main sequence | The stable stage of a star's life in which hydrogen is fused to helium. |
| Naturally occurring element | An 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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