McMath–Pierce solar telescope

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McMath–Pierce Solar Telescope
Mcmath-pierce-telescope.jpg
Alternative names McMath–Pierce Telescope
Named after Robert Raynolds McMath, Keith Pierce Edit this on Wikidata
Location(s) Kitt Peak National Observatory Edit this on Wikidata, United States of America Edit this on Wikidata
Coordinates 31°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[1]
Organization National Solar Observatory Edit this on Wikidata
Altitude 2,096 m (6,877 ft)
Observing time 79 percent sign Edit this on Wikidata
Wavelength Visible and infrared
Built  ()
Telescope style reflecting telescope, solar telescope Edit this on Wikidata
Number of telescopes 3
Diameter 161 cm (5 ft 3 in)
Angular resolution 0.7 second of arc Edit this on Wikidata
Collecting area 2.04 m2 (22.0 sq ft)
Focal length 87 m (285 ft)
Mounting Equatorial mount with heliostat
Enclosure Slanted tower
Website nsokp.nso.edu/mp/
McMath–Pierce solar telescope is located in the US
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. At the dedication in 1962, Dr. Waterman read a letter[2] from President Kennedy starting with:

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. [3]

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.[4]

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.[3]

The enclosure of the telescope was designed and engineered by the Chicago office of Skidmore, Owings and Merrill.[5]

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.

See also[edit]

References[edit]

  1. ^ http://nsokp.nso.edu/mp/site.html.
  2. ^ "NSO/KP History of the MP Facility". Retrieved 2008-05-16. 
  3. ^ a b "McMath-Pierce Telescope and Instruments". National Solar Observatory. National Solar Observatory. Retrieved 28 March 2017. 
  4. ^ Keller, Christopher. "Low-Cost Solar Adaptive Optics". noao.edu. Archived from the original on 21 February 2016. Retrieved 14 May 2017. 
  5. ^ "McMath–Pierce Solar Telescope". Retrieved 2012-03-16. 

External links[edit]