Bok Telescope

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Bok Telescope
Bokscope.jpg
Alternative namesthe 90-inch Edit this at Wikidata
Part ofKitt Peak National Observatory Edit this on Wikidata
Location(s)Arizona
Coordinates31°57′46″N 111°36′00″W / 31.9629°N 111.6°W / 31.9629; -111.6Coordinates: 31°57′46″N 111°36′00″W / 31.9629°N 111.6°W / 31.9629; -111.6 Edit this at Wikidata
OrganizationSteward Observatory Edit this on Wikidata
Altitude6,900 ft (2,100 m) Edit this at Wikidata
First light23 June 1969 Edit this on Wikidata
Telescope styleinfrared telescope
optical telescope Edit this on Wikidata
Diameter2.3 m (7 ft 7 in) Edit this at Wikidata
Bok Telescope is located in the United States
Bok Telescope
Location of Bok Telescope
Related media on Wikimedia Commons

The Bok Telescope (also known as the 90-inch) is the largest telescope operated solely by Steward Observatory. It finds much use from astronomers from University of Arizona, Arizona State University, and Northern Arizona University, with instruments capable of both imaging and spectroscopy.[1] The telescope operates year-round, except during the August summer-shutdown when maintenance is performed while the weather is poor (Arizona's monsoon season lasts from roughly July through August).

History[]

The telescope

The Bok Telescope was named after the prolific astronomer and director of Steward Observatory from 1966–1969, Bart Bok, one of the most beloved astronomers in Tucson. It was used on March 18, 2007 by Bruno Sicardy to view Pluto's occultation of a star in Sagittarius.[2] The building itself features a very long spiral staircase leading to the telescope and a balcony called "The Bok Walk".

In the 2010s the Bok telescope helped support a survey with KNPO telescopes in preparation for the DESI instrument on the 4-m Mayall telescope.[3] The Bok telescope was used along with the 90 Prime imager to take g-band and r-band observations.[3]

Instruments[]

Panorama of the control room

There are currently 3 instruments that are mainly used at the 90-inch, two that work in the optical and one in the near-IR. The instrument, whose principal investigator is , is a prime focus, wide-field imager capable of imaging 1 square degree on the sky, while the does spectroscopy. The , which has been available at the telescope since 1991,[4] uses a NICMOS array which was built during the development of the NICMOS instrument on the HST. The 90-inch is also fitted with an eyepiece for direct viewing by a human observer, uncharacteristic for telescopes of this size.[1]

See also[]

References[]

  1. ^ a b "90-inch Website".
  2. ^ "Arizona Telescopes Focus On Pluto Early March 18".
  3. ^ a b Dey, Arjun; Rabinowitz, David; Karcher, Armin; Bebek, Chris; Baltay, Charles; Sprayberry, David; Valdes, Frank; Stupak, Bob; Donaldson, John; Emmet, Will; Hurteau, Tom (August 2016). Evans, Christopher J; Simard, Luc; Takami, Hideki (eds.). "Mosaic3: a red-sensitive upgrade for the prime focus camera at the Mayall 4m telescope". Ground-based and Airborne Instrumentation for Astronomy VI. 9908: 99082C. Bibcode:2016SPIE.9908E..2CD. doi:10.1117/12.2231488. S2CID 125204403.
  4. ^ "256x256 Page".

External links[]

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