McMath–Pierce solar telescope: Difference between revisions
Removed "until the Daniel K. Inouye telescope was built." The DKIST is under construction as of this date, so the McMath-Pierce Telescope is still the largest solar telescope in the world. |
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*[http://nsokp.nso.edu/mp/cphistory.html A History of the McMath–Pierce] |
*[http://nsokp.nso.edu/mp/cphistory.html A History of the McMath–Pierce] |
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*[http://www.noao.edu/outreach/kptour/mcmath_sch.html Schematic diagram of the McMath–Pierce telescope] |
*[http://www.noao.edu/outreach/kptour/mcmath_sch.html Schematic diagram of the McMath–Pierce telescope] |
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*[http://www.noao.edu/noao/staff/keller/irao/ Adaptive optics at the McMath–Pierce telescope] |
*[https://web.archive.org/web/20160221131712/http://www.noao.edu/noao/staff/keller/irao/ Adaptive optics at the McMath–Pierce telescope] |
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Revision as of 05:50, 14 May 2017
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| Alternative names | McMath–Pierce Telescope |
|---|---|
| Named after | Keith Pierce, Robert Raynolds McMath  |
| Part of | Kitt Peak National Observatory |
| Location(s) | Arizona |
| Coordinates | 31°57′30″N 111°35′42″W / 31.95833°N 111.59500°W |
| Organization | National Solar Observatory |
| Altitude | 2,096 m (6,877 ft) |
| Observing time | 79 percent |
| Wavelength | Visible and infrared |
| Built | 1960–1962 |
| First light | 1962 |
| Telescope style | Unobstructed-aperture Off Axis Prime focus reflecting telescope |
| Number of telescopes | 3 |
| Diameter | 161 cm |
| Secondary diameter | 2.03 m (primary heliostat) |
| Tertiary diameter | 1.52 m |
| Angular resolution | 0.07 arcsec @ 500nm (theoretical) |
| Collecting area | 2.04 m² |
| Focal length | 87 m |
| Mounting | Equatorial mount with heliostat |
| Enclosure | Slanted tower |
| Website | [1] |
  Location of McMath-Pierce Solar Telescope | |
 Related media on Commons | |
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[1] from President Kennedy starting with:
The great new solar telescope at the Kitt Peak National Observatory in Arizona is a source of pride to the nation. The largest instrument for solar research in the world, it presents American astronomers with a unique tool for investigating the nearest of the stars, our sun. This project is of exceptional interest to all our citizens...
Construction
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. [2]
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.
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.[2]
The enclosure of the telescope was designed and engineered by the Chicago office of Skidmore, Owings and Merrill.[3]
Instruments
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.
The auxiliary telescopes can only be used for imaging on static optical tables and do not provide image rotation correction.
See also
References
- ^ "NSO/KP History of the MP Facility". Retrieved 2008-05-16.
- ^ a b "McMath-Pierce Telescope and Instruments". National Solar Observatory. National Solar Observatory. Retrieved 28 March 2017.
- ^ "McMath–Pierce Solar Telescope". Retrieved 2012-03-16.
External links
Media related to McMath–Pierce solar telescope at Wikimedia Commons- Kitt Peak virtual tour: McMath–Pierce Solar Telescope
- "McMath Solar Telescope of the Kitt Peak National Observatory", A. K. Pierce, Applied Optics, 3, 1337–1346, 1964.
- A History of the McMath–Pierce
- Schematic diagram of the McMath–Pierce telescope
- Adaptive optics at the McMath–Pierce telescope