
Thin layers of material applied to a mirror surface to reflect specific wavelengths of light.Mirror coatings are thin films, often just a few hundred nanometers thick, deposited on a mirror's surface to control which wavelengths of light it reflects. By stacking layers of different materials, engineers can create mirrors that reflect over 99.99% of specific laser light, or that selectively reflect certain colors while transmitting others. These coatings are crucial in everything from telescopes to laser cavities to everyday mirrors.
The principles of thin-film interference were understood in the 19th century, but practical multilayer dielectric coatings were developed in the mid-20th century, notably by Alexander Smakula at Zeiss in the 1930s for anti-reflection coatings.
The coating works through interference: light reflects off the top and bottom surfaces of each thin layer, and the reflections add constructively for desired wavelengths and destructively for others. By choosing layer thicknesses (typically quarter-wave optical thickness) and materials with different refractive indices, the coating is 'tuned' to reflect a specific band. Dielectric coatings use alternating high- and low-index materials to achieve high reflectivity without absorbing light, unlike simple metallic coatings.
Used in laser optics (to keep light bouncing in the cavity), astronomical telescope mirrors (to maximize light collection), and in everyday items like eyeglasses and camera lenses to reduce glare.
The most reflective mirrors, used in gravitational wave detectors like LIGO, are coated with alternating layers of silica and tantala, achieving reflectivity of 99.999% — a coating so perfect that if it were a window, it would take a thousand years for a single photon to leak through.
























