GCSE · Physics · Edexcel · Spec 1PH0
Nuclear fusion
Smash two tiny nuclei together fast enough and a sliver of their mass becomes energy. That's what powers the Sun.
One fusion event, start to finish
Two very light nuclei, such as hydrogen nuclei, head towards each other. Each one contains protons, so each one is positively charged.
Drag along the path to follow two nuclei from pushing apart to joining. Keep an eye on the last two stops.
Predict, then check
Fusion needs nuclei moving at very high speeds, which means very high temperatures.
Where in nature would you expect fusion to be happening all the time, on a huge scale?
WHAT YOU'VE LEARNED
A quick recap of today's lesson.
How two tiny nuclei become one, and where the missing mass goes.
What you need to know
- Nuclear fusion is two light nuclei joining to form a heavier nucleus, with energy released.
- Nuclei repel each other strongly because protons are positive, so fusion needs the nuclei to move at very high speeds, which means very high temperatures.
- The products have slightly less mass than the original nuclei. That mass difference is converted into the energy released (E = mc²).
- The number of nucleons and the number of protons are the same before and after a fusion reaction.
- Fusion is the energy source of stars: in the core of a star like the Sun, the temperature and pressure are so high that hydrogen nuclei fuse.
The big picture
Nuclear fusion is when two light nuclei join to form a heavier nucleus. Nuclei are positively charged and repel each other strongly, so they only get close enough to join if they are moving at very high speeds, which needs very high temperatures. The products have slightly less mass than the nuclei that went in, even though the numbers of nucleons and protons stay the same, and that lost mass is released as energy (E = mc²). Fusion is the energy source of stars like the Sun.
Key points
Worked example
Problem
Explain why nuclear fusion needs very high temperatures.
⚠ Watch out
Saying fusion destroys some nucleons or protons. Both counts are the same before and after; what goes down is the mass.
Memory hook
The count stays, the mass pays. After fusion every nucleon and every proton is still there, but a sliver of mass has been paid out as energy.
Check yourself
A friend says the Sun is 'basically a giant bonfire of hydrogen'. Using what you now know about fusion, what would you tell them is wrong with that?
Flashcards
(12)What is nuclear fusion?
Why is it hard to make two nuclei fuse?
How does the mass of the products compare with the mass of the nuclei that fused?
What happens to the mass that is 'missing' after fusion?
Which two numbers are the same before and after a fusion reaction?
What is a nucleon?
Hydrogen-2 + hydrogen-1 fuse to give…?
Hydrogen-2 + hydrogen-3 fuse to give…?
An unknown product has 1 nucleon and 0 protons. What is it?
Is fusion the same as burning hydrogen?
What is the energy source of stars?
Why can hydrogen nuclei fuse in the core of a star like the Sun?
Tap any card to flip it, or use Study as deck to go through them one at a time. In the full lesson these run as a spaced-repetition deck — you rate each card Hard, Good or Easy and the tricky ones keep coming back until they stick.
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