AQA GCSE Fusion reactions in stars (Physics)

Fusion reactions in stars

Stars such as our Sun contain a mixture of hydrogen and helium. 

In a nuclear fusion reaction, the hydrogen is converted into helium. 

This is carried out through a series of reactions, rather than a single reaction. 

You do not need to know the individual stages, you just need to know that overall hydrogen is fused to form helium. 

The individual stages have been given to provide slightly more detail.

1st Stage

In our Sun, two hydrogen nuclei are fused to form heavy hydrogen nuclei and energy is released. 

hydrogen nuclei fusing to form heavy hydrogen

2nd Stage

Hydrogen nuclei fuses with heavy hydrogen nuclei to form a helium nucleus. 

hydrogen nuclei fusing to form helium

3rd stage

Two of the Helium-3 nuclei will fuse to form Helium-4 nuclei and hydrogen nuclei, also releasing energy.

Two helium 3 nuclei fusing to form helium 4 nuclei

In stars of a similar size to our sun, fusion occurs to form elements that do not have a mass greater than iron. 

In stars with a mass greater than our Sun, fusion will occur to form elements heavier than iron. During the supernova stage of the life cycle of a massive star, the core is compressed so much that heavier elements such as uranium are formed.

Practice Questions

1.Name the process which allows for the formation of carbon in stars

2. Write a nuclear fusion equation to explain how three helium-4 nuclei could fuse to form a carbon 12 nucleus.

3. Explain how very heavy elements such as uranium are formed by stars.