Wavenumber to Frequency Converter
Common Conversions
| cm⁻¹ | Hz |
|---|---|
| 1 | 29980000000 |
| 10 | 299800000000 |
| 100 | 2998000000000 |
| 500 | 14990000000000 |
| 1000 | 29980000000000 |
| 2000 | 59960000000000 |
| 3000 | 89940000000000 |
| 4000 | 119900000000000 |
| 5000 | 149900000000000 |
| 10000 | 299800000000000 |
| 20000 | 599600000000000 |
| 50000 | 1499000000000000 |
Why this conversion matters in chemistry
Wavenumber is what spectroscopy reports because it's proportional to energy and reads cleanly in the IR range. Frequency in hertz is what the underlying physics wants — photon energy is E = hν, force-constant calculations are built around vibrational frequencies, quantum-mechanical models return frequencies directly. Multiplying cm⁻¹ by the speed of light in cm/s (2.998 × 10¹⁰ cm/s) converts one to the other. A 1650 cm⁻¹ amide-I C=O stretch becomes 4.95 × 10¹³ Hz, or 49.5 THz. The step shows up every time a molecular dynamics simulation or ab initio calculation outputs vibrational frequencies and you need to compare them against an experimental spectrum.
Formula
Worked Examples
Mid-IR fingerprint region. Roughly 30 THz — a clean anchor worth remembering for spectral bookkeeping.
C–H stretching region. Any aliphatic spectrum shows peaks clustered here.
A generic carbonyl C=O stretch. The exact position shifts with chemical context — aldehydes near 1725, ketones 1715, esters 1735, amides 1650–1680 — which is what makes the band so diagnostic.
Far-IR / THz range. Low-energy lattice vibrations and some metal-ligand modes live here.