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Very Large Array

  (vĕr'ē) pronunciation
n. (Abbr. VLA)

A Y-shaped pattern of radio telescopes in New Mexico with a radius of 21 kilometers (13 miles).


 
 

Radio telescope system consisting of 27 parabolic dishes. The most powerful radio telescope in the world, it has been operated on the plains of San Agustin near Socorro, N.M., U.S., by the National Radio Astronomy Observatory since 1980. Each dish is 82 ft (25 m) in diameter and can be moved independently by transporter along rails laid out in an enormous Y pattern whose arms are about 13 mi (21 km) long. The radio signals received by the dishes are integrated by computer, so the entire array acts as a single radio antenna (an interferometer). The VLA, which has a maximum angular resolution better than a tenth of an arc second, has been responsible for producing many of the most detailed radio images of quasars; galaxies; supernovas; and the Milky Way Galaxy's nucleus.

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Wikipedia: Very Large Array


Very Large Array
USA.NM.VeryLargeArray.02.jpg
Organization: National Radio Astronomy Observatory [1]
Location: Socorro, New Mexico, USA
Coordinates: 34°04′43.497″N, 107°37′03.819″W
Altitude: 2124 m (6970 ft)
Wavelength: radio
Diameter: 27 x 25m
Angular resolution: 0.05 to 700 arcsec

The Very Large Array (VLA) is a radio astronomy observatory located on the Plains of San Augustin, between the towns of Magdalena and Datil, some fifty miles (80 km) west of Socorro, New Mexico, USA. U.S. Route 60 passes through the complex. The VLA stands at an altitude of 6970 ft (2124 m) above sea level. It is a component of the National Radio Astronomy Observatory (NRAO).

Characteristics

The observatory consists of 27 independent radio antennae, each of which has a dish diameter of 25 meters (82 feet) and weighs 209 metric tonnes (230 tons).

The antennas are arrayed along the three arms of a Y-shape (each of which measures 21 km/13 miles long). Using the railroad tracks that follow each of these arms – and that, at one point, intersect with U.S. Route 60 at a level crossing – and a specially designed lifting locomotive, the antennas can be physically relocated to a number of prepared positions, allowing aperture synthesis interferometry with a maximum baseline of 36 km (22.3 miles): essentially, the array acts like a single antenna with that diameter. The smallest angular resolution that can be reached is about 0.05 arcseconds at a wavelength of 7 mm.

Detail of one dish.
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Detail of one dish.

There are four commonly used configurations, designated A (the largest) through D (the tightest, when all the dishes are within 600 m of the center point). The observatory normally cycles through all the various possible configurations (including several hybrids) every 16 months; the antennas are moved every three to four months. Moves to smaller configurations are done in two stages, first shortening the east and west arms and later shortening the north arm. This allows for a short period of improved imaging of extremely northerly or southerly sources.

The Array Operations Center (AOC) for the VLA is located on the campus of New Mexico Tech in Socorro. The AOC also currently serves as the control center for the Very Long Baseline Array (VLBA), a VLBI array of ten 25-meter dishes located from Hawaii in the west to the U.S. Virgin Islands in the east that constitutes the world's largest dedicated, full-time astronomical instrument.

Key science

The VLA is a multi-purpose instrument designed to allow investigations of many astronomical topics. Objects that are commonly studied include radio galaxies, quasars, pulsars, supernova remnants, gamma ray bursts, radio-emitting stars, the sun and planets, astrophysical masers, black holes, and the hydrogen gas that comprises a large portion of the Milky Way galaxy as well as external galaxies. In 1989 the VLA was used to receive radio communications from the Voyager 2 spacecraft as it flew by Neptune.

Past and future

Antenna Assembly Building at VLA
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Antenna Assembly Building at VLA

Congressional approval for the VLA project was given in August 1972, and construction began some six months later. The first antenna was put into place in September 1975 and the complex was formally inaugurated in 1980, after a total investment of USD $78.5 million.

With a view to upgrading the venerable 1970s technology with which the VLA was built, recent funding has been allocated for the conversion of the VLA into the Expanded Very Large Array ("EVLA"). The upgrade will enhance the instrument's sensitivity, frequency range, and resolution, and will install new hardware at the San Augustin site. A second phase of this upgrade to add up to eight additional dishes in other parts of the state of New Mexico, up to 300 km away, is currently unfunded.

Pop culture

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The VLA is the setting of the beginning of the1982 film 2010: The Year We Make Contact. (The novel 2010: Odyssey Two, from which the film was made, set this scene at the radio telescope at the Arecibo Observatory in Puerto Rico.)

The VLA also featured prominently in Carl Sagan's science documentary Cosmos and 1985 novel/film Contact, albeit expanded to 131 dishes and renamed the "Argus Array." When the time came for Hollywood to make the motion picture version (Contact, 1997), much of the outdoor footage was shot at the VLA site. The number of dishes visible on screen was artificially increased by means of CGI, however, and the canyon depicted as being in the vicinity of the VLA is actually Canyon de Chelly in neighboring Arizona.

In the 1996 film Independence Day the alien invaders were initially detected by SETI at the VLA.

New Jersey rock band Bon Jovi shot the music video for "Everyday", at the VLA. This was the first single and music video from the band's Island Records album, Bounce, released on October 8, 2002 in the U.S.

The cover for the Dire Straits album On The Night features the VLA.

The VLA can be visited in Auto Assault, a massively multiplayer online game set in post-apocalyptic America.

Matt Harding can be seen dancing at Very Large Array in his second video.

Visiting

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The VLA site is open to visitors year round during daylight hours. A visitor center houses a museum and a gift shop. A self-guided walking tour is available, as the visitor center is not staffed continuously. Visitors unfamiliar with the area are warned that there is little food onsite, or in the sparsely populated surroundings; those unfamiliar with the high desert are warned that the weather is quite variable, and can remain cold into April.

See also

External links



 
 

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Copyrights:

Dictionary. The American Heritage® Dictionary of the English Language, Fourth Edition Copyright © 2007, 2000 by Houghton Mifflin Company. Updated in 2007. Published by Houghton Mifflin Company. All rights reserved.  Read more
Britannica Concise Encyclopedia. Britannica Concise Encyclopedia. © 2006 Encyclopædia Britannica, Inc. All rights reserved.  Read more
Wikipedia. This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Very Large Array" Read more

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