1. Bohr's Postulates
- Electrons occupy stationary orbits with quantised angular momentum, , and do not radiate while in them.
- A photon is emitted or absorbed only on a jump between orbits: .
2. Orbit Radius & Energy
n=1 (ground state): E₁ = −13.6 eV, r₁ = 0.529 Å (the Bohr radius). Ionisation energy from the ground state = 13.6 eV.
3. The Shrinking-Gap Ladder — the exam trap
Intuition says higher levels should spread further apart. They don’t, the gaps shrink as n increases, converging toward E = 0 (ionisation) at n → ∞:
- n=1 → n=2: gap = 10.2000 eV (by far the largest gap)
- n=2 → n=3: gap = 1.8889 eV
- n=3 → n=4: gap = 0.6611 eV
- n=4 → n=5: gap = 0.3060 eV
- n=5 → n=6: gap = 0.1662 eV
See it live: interactive energy-level simulation →
4. Spectral Series
- Lyman (final level n=1): ultraviolet.
- Balmer (final level n=2): visible — the only series with visible lines.
- Paschen (final level n=3): infrared.
Within any series, lines bunch up toward a sharp series limit (transition from n=∞ to that series’ final level) as the starting level rises.
5. Quick Formula: Wavelength Shortcut
Balmer series limit: E = 3.4000 eV → λ ≈ 364.7 nm. Lyman series limit (n=1): E = 13.6000 eV → λ ≈ 91.2 nm.
6. Limitations
Only accurate for hydrogen and other single-electron (hydrogen-like) ions — e.g. He⁺, Li²⁺. Fails once a second electron adds electron-electron repulsion to the picture.
Full derivations and worked examples: detailed notes →
