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United Kingdom Infrared Telescope (UKIRT)

The United Kingdom Infrared Telescope (UKIRT) is a 3.8-meter reflector telescope specialized in infrared astronomical observations, located at the Mauna Kea Observatory in Hawaii. Considered one of the largest infrared telescopes in the world, it was originally operated by the United Kingdom and is now managed by the University of Hawaii with funding from NASA. Its classic Cassegrain design with an English equatorial mount features a notably thin and lightweight primary mirror, supported by a computerized system of 80 pistons that enhance its optical performance. This structure reduces heat generation, which is crucial for infrared observations, making UKIRT a valuable tool in modern astronomy.
Maunakea Observatories Complex

Mauna Kea Access Road, Mauna Kea,, Hawai (HI 96720)

United States

The Maunakea Observatories Complex is a group of world-class telescopes located near the summit of Maunakea volcano in Hawaii. Thanks to its ideal conditions for astronomy, it hosts facilities from various countries and is one of the most important observation centers in the world.

Descripción

The United Kingdom Infrared Telescope (UKIRT) is a 3.8-meter diameter reflector telescope specifically designed for infrared observations, located at the Mauna Kea Observatory in Hawaii. This telescope is one of the largest and most advanced in its category, with a history of significant contributions to the field of infrared astronomy. Originally operated by the United Kingdom through the Joint Astronomy Centre (JAC), in 2014 the telescope’s ownership was transferred to the University of Hawaii. It is now funded by NASA and operated in collaboration with institutions such as Lockheed Martin Advanced Technology Center and the United States Naval Observatory.

The telescope features a classic Cassegrain design with an English equatorial mount. One of its standout features is its primary mirror, which is thinner and lighter than those of other telescopes of its class, weighing only 6.5 tons. This allows for the use of less powerful motors and control systems, reducing heat generation, which is crucial for infrared observations where heat can interfere with the data. The mirror is supported by 80 aluminum pistons that are computer-controlled to maintain its optimal shape during observations. Although its equatorial mount limits access to objects at certain declinations, the telescope remains highly effective for a wide range of astronomical research, including the study of Solar System objects, star formation, and the observation of distant galaxies.

Datos técnicos del telescopio

  • Tipo de óptica: Telescopio Maksutov-Cassegrain
  • Tipo de montura: Montura Ecuatorial
  • Tipo de Funcionamiento de la Montura: Montura Computerizada
  • Subtipo de Funcionamiento de la Montura: Otros

Telescopios

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The NASA Infrared Telescope Facility (IRTF) is a 3-meter diameter telescope optimized for infrared astronomy, located at the Mauna Kea Observatory in Hawaii. Initially built to support the Voyager missions, it now serves as the United States' national facility for infrared astronomy, dedicating at least 50% of its observation time to planetary science. Operated by the University of Hawaii under a cooperative agreement with NASA, the IRTF has made significant contributions to the observation of Solar System objects, the solar neighborhood, and deep space.
The United Kingdom Infrared Telescope (UKIRT) is a 3.8-meter reflector telescope specialized in infrared astronomical observations, located at the Mauna Kea Observatory in Hawaii. Considered one of the largest infrared telescopes in the world, it was originally operated by the United Kingdom and is now managed by the University of Hawaii with funding from NASA. Its classic Cassegrain design with an English equatorial mount features a notably thin and lightweight primary mirror, supported by a computerized system of 80 pistons that enhance its optical performance. This structure reduces heat generation, which is crucial for infrared observations, making UKIRT a valuable tool in modern astronomy.
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