Class 12 · CBSE / NCERT · Physics

Nuclei — Class 12

A tiny loss of mass releases enormous energy (E = mc²). Learn mass defect, binding energy and half-life, and compute the energy of nuclear reactions.

Nucleus & isotopesThe nucleus contains protons and neutrons (nucleons). Isotopes have the same Z but different mass number A. Nuclear radius R = R₀A^(1/3).
Mass defectThe mass of a nucleus is slightly LESS than the sum of its nucleons; this missing mass Δm is converted to binding energy.
Binding energyThe energy that holds the nucleus together, E = Δm·c². Using 1 u = 931.5 MeV, E = 931.5 × Δm MeV. Higher BE/nucleon = more stable.
Radioactivity & half-lifeUnstable nuclei decay (α, β, γ). The half-life T is the time for half the nuclei to decay; N = N₀/2^(t/T).

Binding-energy calculator Interactive

Enter the mass defect (in atomic mass units) to get the energy released, using 1 u = 931.5 MeV.

Energy, E = 931.5·ΔmMeV

Just 1 atomic mass unit of "lost" mass releases 931.5 MeV — the reason nuclear energy dwarfs chemical energy.

Numericals practice Interactive

Mass-defect energy and half-life problems with steps.

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Solved numericals

Q1. Find the energy released if a mass defect of 0.2 u occurs in a reaction.

E = 931.5 × Δm

E = 931.5 × 0.2

E = 186.3 MeV

Q2. A radioactive substance has a half-life of 4 days. What fraction remains after 12 days?

12 days = 3 half-lives

Fraction left = (1/2)³ = 1/8

So 1/8 (12.5%) of the sample remains.

Formula sheet

QuantityFormulaSI unit
Nuclear radiusR = R₀ A^(1/3)m (R₀ = 1.2 fm)
Mass–energyE = Δm c²joule (J)
Binding energy (shortcut)E = 931.5 × ΔmMeV (Δm in u)
Radioactive decayN = N₀ e^(−λt)
Half-lifeT = 0.693 / λsecond (s)

Common mistakes & exam wins

  • Use E = 931.5 × Δm(in u) to get the energy in MeV directly.
  • Binding energy per nucleon peaks near iron (A ≈ 56) — the most stable nuclei.
  • Fusion (light nuclei joining) and fission (heavy nuclei splitting) both move towards higher BE/nucleon, releasing energy.
  • After n half-lives, the fraction remaining is (1/2)ⁿ.

Frequently asked questions

What is mass defect?

The difference between the sum of the masses of the individual nucleons and the actual (smaller) mass of the nucleus; this missing mass becomes the binding energy.

What is binding energy?

The energy needed to break a nucleus into its separate nucleons (or released when they combine), E = Δm·c² = 931.5 × Δm MeV.

What is half-life?

The time taken for half the radioactive nuclei in a sample to decay; after n half-lives, (1/2)ⁿ of the sample remains.

What is the difference between nuclear fission and fusion?

Fission is the splitting of a heavy nucleus into lighter ones; fusion is the joining of light nuclei into a heavier one. Both release energy.