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Keck telescopes

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W. M. Keck Observatory
The summit of Mauna Kea is considered one of the most important astronomical viewing sites in the world. The twin Keck telescopes are the largest optical/near-infrared instruments.
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The summit of Mauna Kea is considered one of the most important astronomical viewing sites in the world. The twin Keck telescopes are the largest optical/near-infrared instruments.
OrganizationCalifornia Association for Research in Astronomy
LocationMauna Kea, Hawai'i, USA
Wavelength regimeoptical, near infrared
Completion dateKeck I 1993, Keck II 1996
Webpagehttp://www.keckobservatory.org/
Physical characteristics
Telescope stylereflector
Diameter10m each
Effective Angular Resolution85m
Focal length17.5 m (f/1.75)
Mountingalt/az
Domespherical

The W. M. Keck Observatory is home to the two largest optical/near-infrared telescopes in the world, at the 4,145 meter (13,600 ft) summit of Mauna Kea in Hawai'i. At the heart of each 10-meter (400-inch) Keck telescope is a revolutionary primary mirror composed of 36 hexagonal segments that work together as a single piece of reflective glass.

Each Keck telescope sits on an altitude-azimuth design. Extensive computer analysis determined the greatest strength and stiffness for the least amount of steel--about 270 tons per telescope. On the telescope, each segment's figure is kept stable by a system of extremely rigid support structures and adjustable warping harnesses. During observing, a computer-controlled system of sensors and actuators adjusts the position of each segment, relative to its neighbors, to an accuracy of four nanometers. This twice-per-second adjustment effectively counters varying distortions due to the tug of gravity.

Both Keck telescopes are equipped with adaptive optics, which compensates for the blurring due to atmospheric turbulence. In addition, the Keck I and Keck II telescopes can work together as the Keck Interferometer; the 85 m separation gives them the effective angular resolution in one direction of an 85 m mirror, comparable with the resolution of other astronomical interferometer arrays such as the VLTI (200 m separation) but with no interferometric imaging capability.

The W. M. Keck Observatory is managed by the California Association for Research in Astronomy, a non-profit 501 (c)(3) organization whose board of directors includes representatives from Caltech and the University of California. In 1996, the National Aeronautics and Space Administration (NASA) joined as a partner in the Observatory. The telescopes sit on land leased from the University of Hawai'i System based in Honolulu, Hawai'i. Construction of the telescopes were made possible through private grants totaling more than $140 million provided by the W. M. Keck Foundation. Headquarters for the W. M. Keck Observatory are located in Kamuela, Hawaii. Use of the telescopes is restricted to researchers from Caltech, the University of Hawai'i System, NASA and the University of California.

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