McMath–Pierce solar telescope

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
McMath–Pierce Solar Telescope
Mcmath-pierce-telescope.jpg
Alternative namesMcMath–Pierce Telescope Edit this at Wikidata
Named afterKeith Pierce, Robert Raynolds McMath Edit this on Wikidata
Part ofKitt Peak National Observatory Edit this on Wikidata
Location(s)Arizona, US
Coordinates31°57′30″N 111°35′42″W / 31.9584°N 111.595°W / 31.9584; -111.595Coordinates: 31°57′30″N 111°35′42″W / 31.9584°N 111.595°W / 31.9584; -111.595 Edit this at Wikidata
OrganizationNational Solar Observatory Edit this on Wikidata
Altitude2,096 m (6,877 ft) Edit this at Wikidata
Observing time79 percentage Edit this on Wikidata
Telescope styleReflecting telescope
Solar telescope Edit this on Wikidata
Number of telescopesEdit this on Wikidata
Diameter161 cm (5 ft 3 in) Edit this at Wikidata
Angular resolution0.07 arcsecond Edit this on Wikidata
Collecting area2.04 m2 (22.0 sq ft) Edit this at Wikidata
Focal length87 m (285 ft 5 in) Edit this at Wikidata
MountingEquatorial mount Edit this on Wikidata Edit this at Wikidata
Websitensokp.nso.edu/mp/ Edit this at Wikidata
McMath–Pierce solar telescope is located in the United States
McMath–Pierce solar telescope
Location of McMath–Pierce solar telescope

McMath–Pierce solar telescope is a 1.6 m f/54 reflecting solar telescope at Kitt Peak National Observatory in Arizona, United States. The building was designed by Myron Goldsmith and built in 1962. It is the largest solar telescope and the largest unobstructed aperture telescope in the world. It is named for astronomers Robert McMath and Keith Pierce.

Construction[edit]

Results of adaptive optics
A painting by Tucson astronomer and space artist William K. Hartmann, done on site, showing the McMath-Pierce telescope glowing golden in the light of the setting sun.
The inside of the slanted shaft

The telescope is a triple instrument. In addition to the primary 1.61 m mirror fed by the 2.03 m heliostat, there are a pair of telescopes fed by 0.81 m heliostats mounted beside the main heliostat. These two instruments have 1.07 m and 0.91 m primary mirrors.[1]

The telescope uses the heliostat at the top of its main tower to direct the sun's light down a long shaft to the primary mirrors. The distinctive diagonal shaft continues underground, where the telescope's primary mirror is located. The theoretical resolution of the main telescope is 0.07 arcsec, although this is never reached because atmospheric distortions degrade the image quality severely. The image scale is 2.50 arcsec/mm at the image plane. Since 2002 the National Solar Observatory staff have developed an adaptive optics system designed for the unique needs of solar observatories that dramatically improve the resolution of science images.[2]

The secondary telescopes are called East and West. They are completely independent of the main telescope. These two auxiliary telescopes each have a 0.91-meter heliostat located beside the main heliostat. These auxiliary telescopes have a slightly shorter focal length and f-numbers of 50 and 44. The resolution of the auxiliary telescopes is 5.11 arcsec/mm and 5.75 arcsec/mm.[1]

The enclosure of the telescope was designed and engineered by the Chicago office of Skidmore, Owings and Merrill.[3]

At the dedication in 1962, Dr. Waterman read a letter[4] from President Kennedy starting with:

Instruments[edit]

The top of the tower.

The third mirror of the main telescope which sends the light down into the observing room can be moved above three different positions. Two of these have a vacuum spectrograph beneath them, one of 18 meter deep and the other 4 meter deep with lower resolution but higher light throughput. These two spectrographs are able to rotate to compensate for the rotation of the image caused by the use of a heliostat. The third position can only be equipped with a static optical table with no image rotation correction and is therefore rarely used.

A notification of 1992 rededication of the telescope.

The auxiliary telescopes can only be used for imaging on static optical tables and do not provide image rotation correction.

NSF divestment and reinvestment[edit]

In 2016, the National Science Foundation (NSF) announced that it would be divesting from the McMath-Pierce solar observatory. The operator, known as National Solar Observatory, began accepting proposals from new potential operators. A concept for retrofitting by the Kitt Peak visitor center manager was first provided to the NSF for consideration in July 2017. That concept was ultimately developed into a funding proposal to the NSF, submitted again in May 2018. This proposal was awarded in September 2018 by the NSF to the Association of Universities for Research in Astronomy, the organization that operates Kitt Peak National Observatory on behalf of the NSF.[5][6]

See also[edit]

References[edit]

  1. ^ a b "McMath-Pierce Telescope and Instruments". National Solar Observatory. National Solar Observatory. Retrieved 28 March 2017.
  2. ^ Keller, Christopher. "Low-Cost Solar Adaptive Optics". noao.edu. Archived from the original on 21 February 2016. Retrieved 14 May 2017.
  3. ^ "McMath–Pierce Solar Telescope". Archived from the original on 2011-11-17. Retrieved 2012-03-16.
  4. ^ "NSO/KP History of the MP Facility". Archived from the original on 2008-07-08. Retrieved 2008-05-16.
  5. ^ "National Science Foundation to Fund New "Windows on the Universe" Astronomy Outreach Center at Kitt Peak National Observatory". National Optical Astronomy Observatory (Press release).
  6. ^ Mace, Mikayla (27 September 2018). "$4.5M science foundation grant latest in Kitt Peak telescope revitalization". Arizona Daily Star.

External links[edit]