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Rydberg Equation Calculator — Hydrogen Spectral Lines

Calculate the exact wavelength of light emitted or absorbed when a hydrogen electron transitions between two energy levels — enter the lower (n₁) and upper (n₂) principal quantum numbers.
Final principal quantum number — must be less than n₂
Initial quantum number — must be greater than n₁
Wavelength
656.11nm

Visible — Balmer series (n₁ = 2)

Photon energy
1.8897 eV
Wavenumber
15,241.3 cm⁻¹
Series
Balmer (n₁ = 2)
Spectral region
Visible
Transition
n = 3 → n = 2
656 nm
Step by step
  1. 1

    1 ÷ n₁²

    1 ÷ 2² = 0.25
  2. 2

    1 ÷ n₂²

    1 ÷ 3² = 0.111111
  3. 3

    Inverse wavelength 1/λ = R∞ × (1/n₁² − 1/n₂²)

    1.097 × 10⁷ × (0.25 − 0.111111) = 1,524,129 m⁻¹
    R∞ = 1.0974 × 10⁷ m⁻¹ (Rydberg constant, NIST 2018 CODATA).
  4. 4

    Wavelength λ = 10⁹ ÷ (1/λ)

    10⁹ ÷ 1,524,129 = 656.11
Results are estimates for general information only and are not professional advice — always verify important results independently before relying on them. Read the full disclaimer.
Quick answer

How does this calculator work?

The Rydberg equation 1/λ = R∞(1/n₁² − 1/n₂²) gives the wavelength of a photon emitted (or absorbed) by a hydrogen atom transitioning between principal quantum levels n₁ and n₂. The Rydberg constant R∞ = 1.097 × 10⁷ m⁻¹; photon energy E = hc/λ. Named series: Lyman (n₁=1, UV), Balmer (n₁=2, partly visible), Paschen (n₁=3, IR). The equation is exact for hydrogen; hydrogen-like ions scale by Z².

Formula
1/λ = R∞ × (1/n₁² − 1/n₂²) • R∞ = 1.097 × 10⁷ m⁻¹ • E = hc/λ
How this is calculated

The Rydberg equation, 1/λ = R∞ × (1/n₁² − 1/n₂²), predicts the wavelength of light produced when a hydrogen atom's single electron moves between two principal quantum number shells. n₁ is the lower (final) level and n₂ is the higher (initial) level; emission occurs when the electron falls from n₂ to n₁, releasing a photon of exactly that wavelength. Absorption is the reverse — a photon of that wavelength is absorbed when the electron is promoted from n₁ to n₂. The Rydberg constant R∞ = 1.0973731568539 × 10⁷ m⁻¹ is one of the most precisely measured constants in physics (NIST 2018 CODATA).

Grouped by n₁, the lines form named series: n₁ = 1 is the Lyman series (all ultraviolet), n₁ = 2 is the Balmer series (partly visible — the familiar red Hα at 656 nm, blue-green Hβ at 486 nm, and violet lines), n₁ = 3 is the Paschen series (near infrared), n₁ = 4 is Brackett, and n₁ = 5 is Pfund. The photon energy E = hc/λ (using Planck's constant h and the speed of light c) is expressed in electron-volts for convenience.

The Rydberg equation applies exactly only to hydrogen (one proton, one electron). For hydrogen-like ions (He⁺, Li²⁺) the constant scales by Z² (atomic number squared). Multi-electron atoms require quantum-mechanical perturbation theory and do not follow the simple Rydberg formula. This calculator uses the infinite nuclear mass approximation; reduced-mass corrections shift wavelengths by less than 0.05% for hydrogen.

Frequently asked questions

R∞ = 1.0973731568539 × 10⁷ m⁻¹ is derived from fundamental constants: R∞ = mₑe⁴/(8ε₀²h³c), where mₑ is electron mass, e is elementary charge, ε₀ is permittivity of free space, h is Planck's constant and c is the speed of light. Empirically, it was discovered by Johannes Rydberg in 1888 by fitting hydrogen spectral data — quantum mechanics later explained why.

The Balmer series (n₁ = 2) includes all transitions that end at the second energy level. The first four lines fall in the visible spectrum: Hα (n₂=3, 656 nm, red), Hβ (n₂=4, 486 nm, blue-green), Hγ (n₂=5, 434 nm, violet) and Hδ (n₂=6, 410 nm, violet). Higher n₂ lines converge on the series limit at 365 nm (UV). The Balmer series is the reason hydrogen nebulae glow red (Hα dominates).

Directly, no — the Rydberg equation is derived for one-electron (hydrogen-like) atoms. For hydrogen-like ions with atomic number Z, multiply R∞ by Z² (e.g. He⁺ uses 4R∞). For multi-electron atoms, electron screening shifts energy levels and the Rydberg formula fails; spectroscopy tables or quantum-mechanical calculations are required.

Also known as

rydberg equation calculator
hydrogen spectral lines
balmer series calculator
lyman series wavelength
atomic emission wavelength calculator
quantum number wavelength
hydrogen atom photon energy

APA

TG we-Calculate Editorial Team. (2026). Rydberg Equation Calculator — Hydrogen Spectral Lines [Online calculator]. TG we-Calculate. https://we-calculate.com/calculator/rydberg-equation-calculator

Chicago

TG we-Calculate Editorial Team. "Rydberg Equation Calculator — Hydrogen Spectral Lines." TG we-Calculate. 2026. https://we-calculate.com/calculator/rydberg-equation-calculator.

IEEE

TG we-Calculate Editorial Team, "Rydberg Equation Calculator — Hydrogen Spectral Lines," TG we-Calculate, 2026. [Online]. Available: https://we-calculate.com/calculator/rydberg-equation-calculator

BibTeX

@misc{wecalculate_rydberg_equation_calculator, title = {Rydberg Equation Calculator — Hydrogen Spectral Lines}, author = {{TG we-Calculate Editorial Team}}, howpublished = {\url{https://we-calculate.com/calculator/rydberg-equation-calculator}}, year = {2026}, note = {TG we-Calculate} }

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