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💡 Quick rule: E (eV) ≈ 1240 / λ (nm). Green 550 nm → 2.25 eV. UV 300 nm → 4.13 eV.
Photon Energy

Sources & Methodology

Planck constant and speed of light from NIST CODATA 2018 exact values. Electronvolt definition from BIPM SI.
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NIST CODATA 2018 — Planck Constant
Exact defined value h = 6.62607015×10⁻³⁴ J·s (exact since 2019 SI redefinition), used for all photon energy calculations E = hc/λ in this calculator.
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BIPM SI Units — Electronvolt Definition
BIPM definition: 1 eV = 1.602176634×10⁻¹⁹ J (exact by definition since 2019 SI redefinition), used for all joules-to-eV conversions in this calculator.
Methodology: E (J) = h×c/λ. E (eV) = E(J) / 1.602176634×10⁻¹⁹. Convenient: E (eV) = 1239.84 eV·nm / λ(nm). Frequency f = c/λ. Wavenumber k = 2π/λ (rad/m). Spectroscopic wavenumber = 1/λ(cm) (cm⁻¹). Molar energy = E(J) × 6.02214076×10²³ / 1000 (kJ/mol). Constants used: h = 6.62607015×10⁻³⁴ J·s, c = 299792458 m/s, 1 eV = 1.602176634×10⁻¹⁹ J, N_A = 6.02214076×10²³.

⏱ Last reviewed: April 2026

How to Calculate Photon Energy from Wavelength

Photon energy is the energy carried by a single quantum of electromagnetic radiation. It depends entirely on frequency (and therefore wavelength): shorter wavelength means higher frequency means higher energy. This is why UV light causes sunburn and X-rays penetrate tissue, while radio waves pass through the body harmlessly.

The Planck-Einstein Formula

E = hc / λ     E (eV) ≈ 1240 / λ (nm)
h = 6.626×10⁻³⁴ J·s (Planck constant)  •  c = 2.998×10⁸ m/s  •  λ = wavelength (m)

Green light 550 nm: E = 1240/550 = 2.25 eV = 3.61×10⁻¹⁹ J
UV-B 300 nm: E = 1240/300 = 4.13 eV = 6.62×10⁻¹⁹ J
X-ray 0.1 nm: E = 1240/0.1 = 12,400 eV = 12.4 keV

Photon Energy by Spectrum Region

Spectrum RegionWavelengthEnergy (eV)Effect
FM radio3 m4.1×10⁻⁷ eVNon-ionising, penetrates walls
Microwave (WiFi)12.5 cm9.9×10⁻⁶ eVNon-ionising, heats water molecules
IR (thermal)10 µm0.124 eVFelt as heat, absorbed by skin
Red light700 nm1.77 eVVisible, used in laser therapy
Green light550 nm2.25 eVPeak human eye sensitivity
Violet light380 nm3.26 eVVisible, highest visible energy
UV-A350 nm3.54 eVTanning, mild DNA damage
UV-C254 nm4.88 eVGermicidal, breaks DNA bonds
Soft X-ray10 nm124 eVIonising, medical imaging
Hard X-ray0.1 nm12,400 eVDeep tissue penetration
💡 Ionisation threshold: Radiation becomes ionising when photon energy exceeds about 10 eV (λ < 124 nm), enough to eject electrons from atoms. UV-C at 4.9 eV is below the ionisation threshold but can break DNA’s hydrogen bonds (about 3–4 eV). X-rays at 12+ keV easily ionise tissue atoms. Radio waves and microwave photons (<0.001 eV) cannot cause ionisation regardless of intensity.
Frequently Asked Questions
E = hf = hc/λ. Using h = 6.626×10⁻³⁴ J·s and c = 2.998×10⁸ m/s. Convenient: E(eV) = 1240/λ(nm). For green 550 nm: E = 1240/550 = 2.25 eV = 3.61×10⁻¹⁹ J. Higher frequency (shorter wavelength) = higher energy per photon.
1 eV = 1.602176634×10⁻¹⁹ J (exact). It is the energy gained by one electron accelerating through 1 volt of potential. Photon energy ranges: radio ~10⁻⁷ eV, visible light 1.8–3.3 eV, UV 3–124 eV, X-rays 100 eV–100 keV, gamma rays >100 keV. The eV is convenient because atomic bond energies are typically 1–10 eV.
Visible light (380–700 nm): 1.77 eV (red, 700 nm) to 3.26 eV (violet, 380 nm). Green at 550 nm: 2.25 eV. A 1 mW green laser emits 2.25×10¹⁵ photons/second. One mole of 550 nm photons carries 217 kJ of energy (one einstein). This is enough to break weak chemical bonds and drive photochemical reactions like photosynthesis.
UV-A (315–400 nm): 3.10–3.94 eV. UV-B (280–315 nm): 3.94–4.43 eV. UV-C (100–280 nm): 4.43–12.4 eV. UV-C at 254 nm (4.88 eV) is used for germicidal sterilisation because its energy can break pyrimidine dimers in DNA (requiring ~4–5 eV). Ozone absorbs UV-C and most UV-B, protecting Earth’s surface.
Soft X-rays (10–0.1 nm): 124 eV to 12.4 keV. Hard X-rays (<0.1 nm): >12.4 keV. Medical chest X-ray: 20–150 keV photons. Quick formula: E(eV) = 1240/λ(nm). For 0.01 nm: E = 1240/0.01 = 124,000 eV = 124 keV. These energies easily exceed atomic ionisation potentials (hydrogen: 13.6 eV), making X-rays strongly ionising.
Inversely proportional: E = hc/λ. Halving wavelength doubles energy. Radio at 1 m: ~1.2×10⁻⁶ eV. Visible green at 550 nm: 2.25 eV. UV at 100 nm: 12.4 eV. X-ray at 0.1 nm: 12,400 eV. Gamma at 1 pm: 1.24 MeV. This 13-order-of-magnitude energy span explains why different EM radiation has radically different biological effects.
λ(nm) = 1240/E(eV). For 2.0 eV: λ = 620 nm (red). For 3.0 eV: 413 nm (violet). For 10 eV: 124 nm (UV). For 10 keV: 0.124 nm (X-ray). The constant 1240 eV·nm = h×c converted to eV·nm units. Exact value: h×c = 6.626×10⁻³⁴ × 2.998×10⁸ = 1.986×10⁻²⁵ J·m = 1239.84 eV·nm.
h = 6.62607015×10⁻³⁴ J·s (exact by 2019 SI redefinition). It relates photon energy to frequency: E = hf. Reduced form: ℏ = h/(2π) = 1.0546×10⁻³⁴ J·s. Planck constant is fundamental to all of quantum mechanics, setting the scale of quantisation in atomic energy levels, the uncertainty principle, and blackbody radiation.
FM radio at 100 MHz: E = hf = 6.626×10⁻³⁴ × 10⁸ = 6.6×10⁻²⁶ J = 4.1×10⁻⁷ eV per photon. This is far too small to ionise atoms or break chemical bonds (which require ≥1 eV). Radio waves are non-ionising; they heat tissue only through bulk dielectric losses. Their safety limit is determined by heating power density, not individual photon energy.
One einstein = energy of one mole of photons = E(J) × 6.022×10²³. For 550 nm green: 3.61×10⁻¹⁹ J × 6.022×10²³ = 217 kJ/mol. This is used in photochemistry to compare light energy to bond dissociation energies (C-H bond: 413 kJ/mol). Photosynthesis requires about 8 einsteins per mole of CO₂ reduced. UV-B at 300 nm: 399 kJ/mol, close to the energy of carbon-carbon double bonds (614 kJ/mol).
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