A ground-based optical and infrared telescope used for high-resolution spectroscopy.The Keck Telescope refers to the twin 10-meter optical and infrared telescopes at the W. M. Keck Observatory on Mauna Kea, Hawaii. They are among the largest ground-based telescopes in the world, designed for high-resolution spectroscopy and imaging across visible and infrared wavelengths. Their size and advanced instrumentation allow astronomers to study distant galaxies, exoplanets, and stellar phenomena with exceptional detail.
The first Keck telescope began operations in 1993, with the second following in 1996. The design was pioneered by Jerry Nelson and the Lawrence Berkeley Laboratory team, funded by the W. M. Keck Foundation.
Each Keck telescope uses a primary mirror made of 36 hexagonal segments that work together as a single 10-meter mirror, a technique called segmented mirror design. Adaptive optics systems correct for atmospheric distortion in real time, while spectrographs split light into component wavelengths to reveal the composition, temperature, and motion of celestial objects.
Used for high-resolution spectroscopy of distant quasars, exoplanet atmospheres, and galaxy formation studies, as well as supporting NASA missions like the search for habitable exoplanets.
The Keck telescopes are so sensitive they can detect a candle flame on the Moon's surface.



