An 8.2-meter optical-infrared telescope at Mauna Kea, Hawaii, used for wide-field imaging and spectroscopy.The Subaru Telescope is an 8.2-meter optical-infrared telescope located at the summit of Mauna Kea in Hawaii, operated by the National Astronomical Observatory of Japan. Its name comes from the Japanese word for the Pleiades star cluster. It is renowned for its exceptionally wide field of view — a single exposure can cover an area of sky about nine times the size of the full Moon — making it ideal for surveys of faint objects and transient events.
The Subaru Telescope was built by the National Astronomical Observatory of Japan and saw first light in January 1999, after about eight years of construction.
The telescope uses a thin, lightweight primary mirror made of ULE glass, which is supported by 261 actuators that actively adjust its shape to compensate for gravitational deformation as it moves. This active optics system, combined with a corrector lens, delivers sharp images across a 30-arcminute field. Its instruments include wide-field cameras and spectrographs that can capture light from the near-ultraviolet to the mid-infrared, allowing it to study everything from nearby asteroids to galaxies at the edge of the observable universe.
It is used for deep-sky surveys, discovering supernovae and gamma-ray bursts, studying the formation of planets around young stars, and mapping the structure of the Milky Way's halo.
The Subaru Telescope's primary mirror is so precisely polished that if it were scaled up to the size of the Earth, the largest imperfection would be only about 2.5 centimeters high.









