Class 12 · CBSE / NCERT · Physics

Atoms — Class 12

Bohr's model tames the atom with three simple rules. Compute hydrogen energy levels and transition energies for the spectral lines.

Rutherford's modelMost of the atom is empty space with a tiny, dense, positively-charged nucleus; electrons orbit around it (from the gold-foil experiment).
Bohr's postulatesElectrons orbit only in fixed "stationary" orbits (angular momentum = nh/2π) without radiating; they emit/absorb a photon only when jumping between orbits.
Energy levels of hydrogenThe allowed energies are Eₙ = −13.6/n² eV. The negative sign means the electron is bound; n = 1 is the ground state.
Spectral seriesTransitions to n = 1 give the Lyman series (UV), to n = 2 the Balmer series (visible), to n = 3 the Paschen series (IR).

Hydrogen energy-level calculator Interactive

Enter the orbit number n to get the energy and radius of that level in a hydrogen atom.

Energy, Eₙ = −13.6/n²eV
Radius, 0.529·n²Å

Higher orbits are larger and less tightly bound (energy closer to zero); n = ∞ means the electron is free (E = 0).

Numericals practice Interactive

Energy-level and transition problems with steps.

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Solved numericals

Q1. Find the energy released when an electron jumps from n = 3 to n = 2 in hydrogen.

E₃ = −13.6/9 = −1.51 eV; E₂ = −13.6/4 = −3.4 eV

ΔE = E₂ − E₃... energy emitted = E₃ − E₂ = −1.51 − (−3.4)

ΔE = 1.89 eV (a red line of the Balmer series)

Q2. What is the ionization energy of a hydrogen atom in its ground state?

Ground state energy E₁ = −13.6 eV

Ionization means moving the electron to n = ∞ (E = 0)

Ionization energy = 0 − (−13.6) = 13.6 eV

Formula sheet

QuantityFormulaSI unit
Radius of nth orbitrₙ = 0.529 n² Åångström
Energy of nth orbitEₙ = −13.6 / n²eV
Transition energyΔE = 13.6 (1/n₁² − 1/n₂²)eV
Angular momentum (Bohr)L = n h / 2πJ·s

Common mistakes & exam wins

  • Energy Eₙ = −13.6/n² is NEGATIVE because the electron is bound to the nucleus.
  • Balmer series (jumps to n = 2) lies in the visible region — the lines you actually see.
  • The ground state (n = 1) is the most stable and most tightly bound.
  • Ionization energy of hydrogen = 13.6 eV (energy to remove the electron from n = 1).

Frequently asked questions

What are Bohr's postulates?

Electrons revolve in fixed stationary orbits (with angular momentum nh/2π) without radiating energy, and emit or absorb a photon only when jumping between orbits.

What is the energy of the nth orbit of hydrogen?

Eₙ = −13.6/n² eV; the negative sign shows the electron is bound, and n = 1 is the lowest (ground) state.

What is the Balmer series?

The set of spectral lines emitted when electrons fall to the n = 2 level of hydrogen; these lie in the visible region.

What was the conclusion of the Rutherford gold-foil experiment?

That the atom is mostly empty space with a tiny, dense, positively charged nucleus at its centre.