weirdfacts

The mass of a bound nucleus is less than the total mass of its separated nucleons. The difference corresponds to binding energy. In a reaction, a lower total final rest mass means energy has been released into kinetic energy and radiation.

Fission splits a heavy nucleus and can release neutrons that sustain a chain reaction. Fusion joins light nuclei; high temperatures help nuclei overcome electrostatic repulsion. Both can release energy when the products have greater binding energy per nucleon.

INTERACTIVE MODEL

Rest mass becomes energy

READ THE GRAPH

Explore the relationship

E = Δmc² with c = 3.00 × 10⁸ m s⁻¹.

Released energy / 10⁻¹³ J023.6347.2570.8894.502.557.510Mass defect per reaction / 10⁻²⁹ kg
Released energy / 10⁻¹³ J

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View plotted data as a table
Explore the relationship
SeriesMass defect per reaction / 10⁻²⁹ kgReleased energy / 10⁻¹³ J
Released energy / 10⁻¹³ J00
Released energy / 10⁻¹³ J0.1666671.5
Released energy / 10⁻¹³ J0.3333333
Released energy / 10⁻¹³ J0.54.5
Released energy / 10⁻¹³ J0.6666676
Released energy / 10⁻¹³ J0.8333337.5
Released energy / 10⁻¹³ J19
Released energy / 10⁻¹³ J1.1666710.5
Released energy / 10⁻¹³ J1.3333312
Released energy / 10⁻¹³ J1.513.5
Released energy / 10⁻¹³ J1.6666715
Released energy / 10⁻¹³ J1.8333316.5
Released energy / 10⁻¹³ J218
Released energy / 10⁻¹³ J2.1666719.5
Released energy / 10⁻¹³ J2.3333321
Released energy / 10⁻¹³ J2.522.5
Released energy / 10⁻¹³ J2.6666724
Released energy / 10⁻¹³ J2.8333325.5
Released energy / 10⁻¹³ J327
Released energy / 10⁻¹³ J3.1666728.5
Released energy / 10⁻¹³ J3.3333330
Released energy / 10⁻¹³ J3.531.5
Released energy / 10⁻¹³ J3.6666733
Released energy / 10⁻¹³ J3.8333334.5
Released energy / 10⁻¹³ J436
Released energy / 10⁻¹³ J4.1666737.5
Released energy / 10⁻¹³ J4.3333339
Released energy / 10⁻¹³ J4.540.5
Released energy / 10⁻¹³ J4.6666742
Released energy / 10⁻¹³ J4.8333343.5
Released energy / 10⁻¹³ J545
Released energy / 10⁻¹³ J5.1666746.5
Released energy / 10⁻¹³ J5.3333348
Released energy / 10⁻¹³ J5.549.5
Released energy / 10⁻¹³ J5.6666751
Released energy / 10⁻¹³ J5.8333352.5
Released energy / 10⁻¹³ J654
Released energy / 10⁻¹³ J6.1666755.5
Released energy / 10⁻¹³ J6.3333357
Released energy / 10⁻¹³ J6.558.5
Released energy / 10⁻¹³ J6.6666760
Released energy / 10⁻¹³ J6.8333361.5
Released energy / 10⁻¹³ J763
Released energy / 10⁻¹³ J7.1666764.5
Released energy / 10⁻¹³ J7.3333366
Released energy / 10⁻¹³ J7.567.5
Released energy / 10⁻¹³ J7.6666769
Released energy / 10⁻¹³ J7.8333370.5
Released energy / 10⁻¹³ J872
Released energy / 10⁻¹³ J8.1666773.5
Released energy / 10⁻¹³ J8.3333375
Released energy / 10⁻¹³ J8.576.5
Released energy / 10⁻¹³ J8.6666778
Released energy / 10⁻¹³ J8.8333379.5
Released energy / 10⁻¹³ J981
Released energy / 10⁻¹³ J9.1666782.5
Released energy / 10⁻¹³ J9.3333384
Released energy / 10⁻¹³ J9.585.5
Released energy / 10⁻¹³ J9.6666787
Released energy / 10⁻¹³ J9.8333388.5
Released energy / 10⁻¹³ J1090
Released energy / 10⁻¹³ J: 0

Explore: Change the mass defect and see how energy release scales.

E=Δmc2E=\Delta m c^2
WORKED EXAMPLE

A reaction loses 2.0 × 102910^{-29} kg of rest mass. Use c = 3.0 × 10810^{8} ms1\mathrm{m}\,\mathrm{s}^{-1}.

  1. E = 2.0 × 102910^{-29} × (3.0 × 10810^{8})².
  2. E = 1.8 × 101210^{-12} J.
Assumed knowledge

Scientific notation and squaring.

Learning checkpoints & sourceYOUR LEARNING CHECKPOINT
  • Relate mass defect to energy release.
  • Compare fission, fusion and chain reactions.
QCAA Physics · Unit 1 · Ionising radiation and nuclear reactions
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