23.1 Mass Defect and Nuclear Binding Energy


2026 Syllabus Objectives

By the end of this topic, you should be able to:

  1. Understand the equivalence between energy and mass as represented by E = mc², and recall and use this equation.
  2. Represent simple nuclear reactions using nuclear equations.
  3. Define and use the terms mass defect and binding energy.
  4. Sketch the variation of binding energy per nucleon with nucleon number.
  5. Explain what is meant by nuclear fusion and nuclear fission.
  6. Explain the relevance of binding energy per nucleon to nuclear reactions, including fusion and fission.
  7. Calculate the energy released in nuclear reactions using E = c²Δm.

1. Mass–Energy Equivalence: E = mc²

The Big Idea

You may have learned in chemistry that mass is always conserved in a reaction — meaning the total mass of the reactants equals the total mass of the products. In nuclear physics, this is not quite true. A tiny amount of mass can actually disappear during a nuclear reaction — and that missing mass is converted directly into energy.

This idea was proposed by Albert Einstein and is summarised by one of the most famous equations in science:

E=mc2\boxed{E = mc^2}

Where:

  • E = energy (measured in Joules, J)
  • m = mass (measured in kilograms, kg)
  • c = the speed of light in a vacuum = 3.0 × 10⁸ m s⁻¹

What does it mean?

This equation tells us that mass and energy are two different forms of the same thing. You can convert mass into energy, and you can convert energy into mass.

  • If mass disappears during a reaction → energy is released.
  • If mass appears during a reaction → energy must be put in.

Because c² is an enormous number (9 × 10¹⁶), even a tiny amount of mass produces a huge amount of energy. This is why nuclear reactions release so much more energy than ordinary chemical reactions (like burning fuel).

Real-world examples of E = mc²:

  • Hydrogen fusing into helium inside the Sun — this powers all life on Earth.
  • Uranium splitting apart in nuclear power stations — producing electricity.
  • Nuclear weapons.
  • High-speed particle collisions in particle accelerators (like the Large Hadron Collider).

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