Mass and energy are equivalent: E=mc2. A nucleus has less mass than its separate protons and neutrons; this mass defectΔm corresponds to the binding energyc2Δm, the energy needed to separate the nucleus into its nucleons. Binding energy per nucleon peaks near iron-56. Splitting heavy nuclei (fission) or joining light ones (fusion) moves towards the peak, releasing energy.
Cambridge 9702 Paper 4Edexcel YPH11 WPH15AQA 7408 Paper 2≈ 40 minRevision 6 · updated 2026-10-27
Section 1 of 14
Learning objectives
Use E=mc2 and the unified atomic mass unit.
Define and calculate mass defect and binding energy.
Sketch and interpret the binding energy per nucleon curve.
Calculate energy released in fission and fusion.
Pause and think
A helium-4 nucleus is lighter than two protons and two neutrons weighed separately. Where did the missing mass go?
Section 2 of 14
Core idea
Start hereThe whole weighs less than its parts
Weigh two protons and two neutrons separately, then a helium nucleus made of them: the nucleus is lighter. The missing mass became energy when they bound together. That's where nuclear power and starlight come from.
The big idea
Mass defect Δm; binding energy Δmc2. Binding energy per nucleon peaks near iron: fusion (light) and fission (heavy) both release energy.
1. Mass defect
E=Δmc2,1 u≡931.5 MeV
where
Δm
mass of separate nucleons − mass of nucleus.
Worked exampleHelium-4
Nucleus 4.001506 u; mp=1.007276 u, mn=1.008665 u.
Goal
Binding energy per nucleon.
Strategy
Defect × 931.5.
1
2(1.007276)+2(1.008665)=4.031882 u
Separate nucleons.
2
Δm=0.030376 u
Subtract.
3
0.030376×931.5=28.3 MeV
Binding energy.
4
28.3÷4=7.07 MeV
Per nucleon.
Answer7.07 MeV per nucleon.
✓ CheckHelium sits high on the curve for a light nucleus ✓.
2. The curve
Binding energy per nucleon against nucleon numberMoving towards the peak from either side increases the binding energy per nucleon, releasing energy: fusion of light nuclei, fission of heavy ones.
✓ CheckMatches the accepted ~200 MeV per fission ✓.
⚠️ Common misconceptionMore binding energy = less stable?Higher binding energy per nucleon means more stable.
Pause and think
Why don't stars release energy by fusing iron?
Summary
ΔE=Δmc2.
Peak near Fe-56.
Key words
Mass defect
Mass lost when nucleons bind.
📜 HistoryMeitner on a winter walk.Over Christmas 1938, Lise Meitner and her nephew Otto Frisch, walking in the Swedish snow, realised that Hahn's uranium experiments meant the nucleus was splitting in two. Using E=mc2, they calculated about 200 MeV per fission, and named it after cell division.
🤯 Fun factThe Sun loses weight.The Sun converts about 4 million tonnes of mass into energy every second by fusing hydrogen into helium. Even so, in its whole 10-billion-year life it will lose less than 0.1% of its mass this way.
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