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Bohr Model Calculator

Energy levels, orbital radii & photon wavelengths for hydrogen-like atoms (H, He⁺, Li²⁺, muonium, custom Z) — with reduced-mass correction.

Radius & Energy — hydrogen-like atom

Famous hydrogen lines (reference)

LineTransitionSeriesλRegion
Lyman-α2 → 1Lyman121.5684 nmUltraviolet
Lyman-β3 → 1Lyman102.5734 nmUltraviolet
H-α3 → 2Balmer656.4696 nmRed (visible)
H-β4 → 2Balmer486.2738 nmBlue-green
H-γ5 → 2Balmer434.1730 nmViolet
Paschen-α4 → 3Paschen1875.6274 nmInfrared
He⁺ Lyman-α2 → 1Lyman30.3797 nmUltraviolet

All values computed with CODATA 2018 constants and the reduced-mass correction, matching NIST ASD line positions.

Formulas & honest limits

rₙ = n²a₀ / Z  ·  a₀ = 5.29177210903×10⁻¹¹ m
Eₙ = −13.6057 · Z²/n² eV  (× μ/mₑ with correction)
ΔE = 13.6057·Z²(1/n₁² − 1/n₂²) eV  ·  λ = hc/ΔE  ·  hc = 1239.842 eV·nm
vₙ = Z·α·c / n  ·  α = 1/137.036  ·  Tₙ = 2πrₙ/vₙ

Limits: the Bohr model is exact only for one-electron systems. For multi-electron atoms inner electrons screen the nucleus (it predicts helium's first ionization as 54.4 eV; measured: 24.58 eV). It also misses fine structure, the Lamb shift, and real orbital shapes — quantum mechanics replaced circular orbits with probability clouds in 1926.

Frequently asked questions

What is the Bohr radius of hydrogen?

The Bohr radius a₀ = 5.29177210903×10⁻¹¹ m is the most probable electron–nucleus distance in hydrogen's ground state. This calculator gives r₁ = 52.9465 pm (0.052947 nm) for hydrogen n=1, including the reduced-mass correction; the textbook infinite-nuclear-mass value is 52.9177 pm. Radius scales as rₙ = n²a₀/Z, so n=2 sits at 211.7862 pm and n=3 at 476.5189 pm.

What is the energy of hydrogen's ground state?

E₁ = −13.5983 eV for hydrogen (n=1), including the reduced-mass correction — the infinite-mass Bohr value is −13.6057 eV. The measured ionization energy of hydrogen is 13.59844 eV, which is exactly why this calculator applies the correction by default instead of the textbook value.

How do you calculate hydrogen energy levels?

Eₙ = −13.6/n² eV is the handy approximation. Full-precision values for hydrogen: E₂ = −3.39957 eV, E₃ = −1.510921 eV, E₄ = −0.849893 eV, E₅ = −0.543931 eV, E₆ = −0.377730 eV. For hydrogen-like ions multiply by Z²: He⁺ ground state −54.4153 eV, Li²⁺ ground state −122.4417 eV.

What is the wavelength of the Lyman-alpha line?

121.5684 nm (ultraviolet), from the n=2→1 transition with ΔE = 10.19872 eV. You will often see 121.567 nm quoted — that comes from a rounded Rydberg constant; 121.5684 nm is the full-precision CODATA 2018 value with reduced-mass correction. Without the correction the Bohr model gives 121.5023 nm.

What is the H-alpha wavelength?

656.4696 nm — the famous red line of the Balmer series (n=3→2), with photon energy ΔE = 1.88865 eV. Its siblings are H-beta at 486.2738 nm (n=4→2, blue-green) and H-gamma at 434.1730 nm (n=5→2, violet).

What are the hydrogen spectral series?

Each series is named by its lower level n₁: Lyman (n₁=1, ultraviolet), Balmer (n₁=2, visible), Paschen (n₁=3, infrared), Brackett (n₁=4), Pfund (n₁=5), Humphreys (n₁=6). Example: Paschen-alpha (n=4→3) is 1875.6274 nm, deep in the infrared; Lyman-beta (n=3→1) is 102.5734 nm.

Does the Bohr model work for He⁺ and Li²⁺?

Yes — it works for any one-electron (hydrogen-like) ion: scale energies by Z² and radii by 1/Z. He⁺ ground state is −54.4153 eV and its 2→1 line sits at 30.3797 nm; Li²⁺ ground state is −122.4417 eV. It fails for multi-electron atoms because the inner electrons screen the nuclear charge.

What is muonium, and why is it in this calculator?

Muonium (μ⁺e⁻) is an exotic hydrogen-like atom: a positive muon orbited by an electron, studied in precision spectroscopy. Because the muon is only ~207× heavier than the electron, μ/mₑ = 0.995187, so its ground state is −13.54021 eV — about 0.5% less bound than hydrogen — and its Lyman-alpha line is at 122.0899 nm instead of 121.5684 nm.

How fast does the electron move in the Bohr model?

For hydrogen's ground state v₁ = 2.187691×10⁶ m/s — about 0.73% of the speed of light (c/137.036, the fine-structure constant at work). One orbit takes T₁ = 1.5207×10⁻¹⁶ s. Speed scales as Z/n.

What is the reduced-mass correction?

Real nuclei are not infinitely heavy — nucleus and electron orbit their common center of mass. Including the reduced mass μ shifts every wavelength slightly: Lyman-alpha computes as 121.5023 nm without it and 121.5684 nm with it, matching measurement. The calculator applies it by default for H, He⁺, Li²⁺ and muonium (uncheck the box to see pure textbook values).

Where does the Bohr model fail?

Three honest limits: (1) multi-electron atoms — screening breaks the Z² scaling (it predicts helium's first ionization as 54.4 eV vs the measured 24.58 eV); (2) fine structure and the Lamb shift, which split lines the model says are single; (3) electrons do not travel in circular orbits — quantum mechanics replaced them with probability clouds in 1926. Use this tool for hydrogen-like spectra, not for chemistry.

How do I identify an unknown spectral line?

Enter the wavelength in the “Identify λ” tab. Example: 486.27 nm identifies as hydrogen 4→2 (H-beta, Balmer series) — predicted 486.2738 nm, a 0.0008% difference. The tool ranks the five closest hydrogen transitions so you can judge ambiguous cases.

Related tools

Convert the photon wavelength further: wavelength ⇄ frequency calculator.

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