Technique measuring absorption of infrared light to identify molecular composition of materials.Infrared spectroscopy is a technique that identifies molecules by the way they absorb infrared light. Every molecule has a unique set of vibrational modes — bonds stretch, bend, and twist at specific frequencies. When infrared light matches one of these frequencies, the molecule absorbs it, leaving a characteristic 'fingerprint' in the spectrum. This allows scientists to determine what substances are present in a sample, from distant interstellar clouds to a speck of microplastic in the ocean.
The first practical infrared spectrometers were developed in the 1940s, building on earlier work in the 19th century by William Herschel, who discovered infrared radiation, and later by physicists like Coblentz who recorded spectra of organic compounds. The technique became routine in chemistry labs by the 1950s.
A beam of infrared light is passed through or reflected off a sample. The transmitted or reflected light is then analyzed to see which frequencies were absorbed. The resulting absorption spectrum is compared against reference libraries to identify the molecular bonds present. Modern variants, such as Fourier-transform infrared (FTIR) spectrometers, use interferometry to capture the entire spectrum quickly, and quantum-correlated spectroscopy can even enhance sensitivity beyond classical limits.
Used in chemistry, forensics, environmental monitoring (e.g., detecting microplastics), astronomy (identifying molecules in interstellar space), and medical diagnostics (e.g., identifying cancerous tissue via spectral signatures).
Infrared spectroscopy was used to identify the presence of water and organic molecules on Mars by the Mars rovers, helping confirm that the planet once had habitable conditions.














