Calculate photon energy, frequency, wavelength, and wavenumber from any one input, with spectrum region shown for radio to gamma rays.

undefined

Photon energy; wavelength and spectroscopic wavenumber are in vacuum. Spectrum boundaries are approximate.

Frequency To Energy Formula

The calculator converts between photon frequency, vacuum wavelength, and energy using the Planck relation and the vacuum speed of light.

E = h × f; λ = c / f; E = h × c / λ
  • E = photon energy in joules (J)
  • f = frequency in hertz (Hz)
  • λ = wavelength in meters (m)
  • h = Planck constant = 6.62607015 × 10⁻³⁴ J·s
  • c = speed of light in vacuum = 299,792,458 m/s

Select the calculation path matching the known value:

  • Frequency path. You enter f. The calculator returns E from E = h·f and λ from λ = c/f.
  • Wavelength or wavenumber path. You enter λ (or a wavenumber in cm⁻¹, which is converted with λ = 1/wavenumber). It returns f = c/λ and E = h·c/λ.
  • Photon-energy path. You enter E in any supported unit. It returns f = E/h and λ = c/f.

Energy results are also shown in eV, kJ/mol, and kcal/mol. The conversion to eV uses 1 eV = 1.602176634 × 10⁻¹⁹ J. Per-mole values use Avogadro’s number, 6.02214076 × 10²³ mol⁻¹.

Reference Tables

Use these tables to sanity-check a result. Spectrum boundaries are approximate vacuum-wavelength conventions, with overlapping definitions; the visible band used here is 380–750 nm.

Region Wavelength Frequency Photon energy
Radio> 1 m< 300 MHz< 1.2 µeV
Microwave1 mm – 1 m300 MHz – 300 GHz1.2 µeV – 1.2 meV
Infrared750 nm – 1 mm300 GHz – 400 THz1.2 meV – 1.65 eV
Visible380 – 750 nm400 – 790 THz1.65 – 3.26 eV
Ultraviolet10 – 380 nm790 THz – 30 PHz3.26 – 124 eV
X-ray0.01 – 10 nm30 PHz – 30 EHz124 eV – 124 keV
Gamma< 0.01 nm> 30 EHz> 124 keV
Energy unit Equivalent in joules
1 eV1.602177 × 10⁻¹⁹ J
1 kJ/mol1.660539 × 10⁻²¹ J per photon
1 kcal/mol6.947695 × 10⁻²¹ J per photon
1 hartree4.359745 × 10⁻¹⁸ J
1 cm⁻¹ (wavenumber)1.986446 × 10⁻²³ J

Worked Examples

Example 1: Green light at 520 nm. Convert to frequency and energy.

f = c / λ = (2.998 × 10⁸ m/s) / (5.20 × 10⁻⁷ m) = 5.765 × 10¹⁴ Hz.
E = h · f = (6.626 × 10⁻³⁴ J·s)(5.765 × 10¹⁴ Hz) = 3.820 × 10⁻¹⁹ J = 2.384 eV.

Example 2: A 2.45 GHz microwave photon.

E = h · f = (6.626 × 10⁻³⁴)(2.45 × 10⁹) = 1.623 × 10⁻²⁴ J = 1.013 × 10⁻⁵ eV.
λ = c / f = (2.998 × 10⁸) / (2.45 × 10⁹) = 0.1224 m.

FAQ

Why is photon energy proportional to frequency, not wavelength? The Planck relation E = h·f comes from quantum theory. Frequency counts oscillations per second, and each photon carries one quantum of that oscillation. Wavelength is just c/f, so longer wavelengths mean lower frequency and lower energy.

What’s the quick shortcut for nm to eV? E (eV) ≈ 1240 / λ (nm). It’s accurate to about four digits and works well for visible, UV, and near-IR light.

When should I use kJ/mol instead of eV? Use kJ/mol or kcal/mol when comparing photon energy to chemical bond energies or activation energies. Use eV for single-photon physics, spectroscopy, and semiconductor band gaps.

What does a wavenumber in cm⁻¹ mean? Wavenumber is 1/λ expressed per centimeter. It’s standard in IR spectroscopy. Multiply cm⁻¹ by 100 to get m⁻¹, then take the reciprocal to get wavelength in meters.