Nicholas U. Mayall Telescope facts for kids
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| Alternative names | Mayall 4-meter Telescope |
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| Part of | Kitt Peak National Observatory  |
| Location(s) | Arizona |
| Coordinates | 31°57′48″N 111°36′00″W / 31.9634°N 111.6°W |
| Organization | NOIRLab |
| Altitude | 2,120 m (6,960 ft) |
| First light | February 27, 1973 |
| Discovered | Methane ice on Pluto |
| Telescope style | optical telescope Ritchey–Chrétien telescope |
| Diameter | 4 m (13 ft 1 in) |
| Collecting area | 11.4 m2 (123 sq ft) |
| Website | noirlab |
 Location of Nicholas U. Mayall Telescope
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The Nicholas U. Mayall Telescope, also known as the Mayall 4-meter Telescope, is a four-meter (158 inches) reflector telescope located at the Kitt Peak National Observatory in Arizona and named after Nicholas U. Mayall. It saw first light on February 27, 1973, and was the second-largest telescope in the world at that time. Initial observers included David Crawford, Nicholas Mayall, and Arthur Hoag. It was dedicated on June 20, 1973 after Mayall's retirement as director. The mirror has an f/2.7 hyperboloidal shape. It is made from a two-foot (61 cm (24 in)) thick fused quartz disk that is supported in an advanced-design mirror cell. The prime focus has a field of view six times larger than that of the Hale reflector. It is host to the Dark Energy Spectroscopic Instrument. The identical Víctor M. Blanco Telescope was later built at Cerro Tololo Inter-American Observatory, in Chile.
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Planning & construction
In 1961, after work had moved forward on other telescopes, Mayall proposed an even larger 150-inch mirror telescope for Kitt Peak. Site construction began in 1968 and by 1971 the mirror was delivered to the site. The mirror was made by Owens-Illinois and made of fused quartz, valued for its low coefficient of thermal expansion. The blank was ground at the Kitt Peak optical lab.
The telescope primary mirror is designed to function as the first element in a Ritchey–Chrétien optical design. The telescope was originally designed with three focal point options: the prime focus, a wide-field R/C focus, and a coudé focus.
The telescope was dedicated in the summer of 1973, at which time it was the second largest telescope by aperture in the world. The telescope was named after Mayall who was the director of Kitt Peak National Observatory for over a decade.
Instruments
Examples of instruments over its lifetime include various spectrographs, Cryogenic Camera, the Phoenix spectrometer, and the DLIRIM.
The KNPO Mosaic camera was installed in 1998, and was designed for the prime focus. This camera had eight 2048 × 4096 CCD sensors. This led to another camera Mosaic II for the CTIO 4-m telescope in the southern hemisphere.
- Mosaic3
Mosaic3 was an imaging camera for the Mayall telescope. This prime focus camera was used for a 3-band survey in support of the upcoming DESI instrument.
- Fourier Transform Spectrograph
One instrument used with telescope was the Fourier Transform Spectrograph. The FTS was used between 1975 and 1995, creating an archive of recorded spectra. It was noted for collecting infrared spectrum before the advent of infrared imaging arrays.
Over the time of its operation 10,000 spectra were taken of 800 different astronomical targets, and these were made available in the SpArc data archive in the early 21st century.
- DESI
An instrument designed to help understand dark energy, installation of the Dark Energy Spectroscopic Instrument (DESI) was completed in late 2019. Very little is known about dark energy, the supposed pressure responsible for the accelerating expansion rate of the universe.
DESI has five thousand fiber optic sensors, each one being robotically targetable at the focal plane. Planned to examine the nature of millions of galaxies and quasars, the instrument has been a decade in construction and features contributions from hundreds of researchers.
The telescope control software was also upgraded in the 2010s to prepare for DESI.
DESI achieved first light in 2019 and was commissioned in March of 2020. Due to the COVID-19 pandemic, full operations have been delayed until mid-2021.
Discoveries & observations
In 1976 the Mayall Telescope was used to discover methane ice on planet Pluto.
The FTS on Mayall was also used to study methane in the outer solar system in the 1980s. The study included observation of monodeutered methane on Titan, a moon of Saturn noted for its thick atmosphere. The Mayall was also one of several large telescopes that was part of a study of the Andromeda galaxy. The observations helped understand the history of that galaxy, which in turn helps understand Earth's galaxy, the Milky Way.
Contemporaries on commissioning
The Mayall was the second-largest telescope when inaugurated, between the Hale (5 m) and Shane (3 m).
Largest telescopes 1973:
| # | Name / Observatory |
Image | Aperture | Altitude | First Light |
Special advocate |
|---|---|---|---|---|---|---|
| 1 | Hale Telescope Palomar Obs. |
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200 inch 508 cm |
1713 m (5620 ft) |
1949 | George Ellery Hale |
| 2 | Mayall Telescope Kitt Peak National Obs. |
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158 inch 401 cm |
2120 m (6955 ft) |
1973 | Nicholas Mayall |
| 3 | Shane Telescope Lick Observatory |
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120 inch 305 cm |
1283 m (4209 ft) |
1959 | Nicholas Mayall C. Donald Shane |
| 4 | Harlan J. Smith Telescope McDonald Observatory |
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107 in 270 cm |
2070 m (6791 ft) |
1968 | Harlan J. Smith |
Here is the dedication of the telescope with its namesake at the eyepiece:
Images for kids
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Looking out at Kitt Peak from Mayall
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DESI Installed on the Mayall 4-meter Telescope
See also
In Spanish: Telescopio Mayall para niños
- List of astronomical observatories
- List of largest optical reflecting telescopes
- List of largest optical telescopes in the 20th century
- List of the largest optical telescopes in North America
- Lists of telescopes
