Very Large Array
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2008-07-02T22:58:32Z
TheGerm
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{{Unreferenced|date=June 2007}}
{{Infobox Telescope
|name = Very Large Array
|image = [[Image:USA.NM.VeryLargeArray.02.jpg|300px|The VLA, Socorro, New Mexico, USA]]
|organization = {{nowrap|[[NRAO|National Radio Astronomy Observatory]]}}
|location = [[Socorro, New Mexico]], [[USA]]
|coords = {{coor dms|34|04|43.497|N|107|37|03.819|W|type:landmark}}
|altitude = 2124 m (6970 ft)
|weather =
|wavelength = radio
|built =
|website =
|style =
|diameter = 27 x 25m
|angular_resolution = {{nowrap|0.05 to 700 [[Arcsecond|arcsec]]}}
|area =
|focal_length =
|mounting =
|dome =
|website = [http://www.vla.nrao.edu/ www.vla.nrao.edu]
}}
The '''Very Large Array''' ('''VLA''') is a [[radio astronomy]] [[observatory]] located on the [[Plains of San Augustin]], between the towns of [[Magdalena, New Mexico|Magdalena]] and [[Datil, New Mexico|Datil]], some fifty miles (80 km) west of [[Socorro, New Mexico|Socorro]], [[New Mexico]], [[United States|USA]]. [[U.S. Route 60]] passes through the complex, which is adjacent to the [[Boy Scout]] [[Double H High Adventure Base]]. 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 antennas, each of which has a dish diameter of 25 meters (82 feet) and weighs 209 [[metric tonne]]s (230 [[Short 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): in essence, the array acts as a single antenna with that diameter. The smallest angular resolution that can be reached is about 0.05 [[arcsecond]]s at a [[wavelength]] of 7 mm. [[Image:Very Large Array dish detail.jpg|250px|thumb|right|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 Institute of Mining and Technology|New Mexico Tech]] in Socorro. The AOC also currently serves as the control center for the [[Very Long Baseline Array]] (VLBA), a [[Very Long Baseline Interferometry|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 galaxy|radio galaxies]], [[quasar]]s, [[pulsar]]s, [[supernova]] remnants, [[gamma ray burst]]s, radio-emitting [[star]]s, the [[sun]] and [[planet]]s, [[astrophysical maser]]s, [[black hole]]s, 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==
[[Image:Vla maintenance.jpg|thumb|250px|Antenna Assembly Building at VLA]]
[[United States Congress|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 [[United States dollar|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==
[[Image:USA.NM.VeryLargeArray.01.jpg|thumb|250px|]]
The VLA featured prominently in [[Carl Sagan]]'s 1980 documentary ''[[Cosmos: A Personal Voyage]]'', and is the setting for the beginning of the 1984 film ''[[2010 (film)|2010]]''—with the same scene in the novel ''[[2010: Odyssey Two]]'', from which the film was adapted, being set at the radio telescope at the [[Arecibo Observatory]] in [[Puerto Rico]]. The 1985 novel ''[[Contact (novel)|Contact]]'' features a fictionalized version of the VLA, expanding the number of dishes to 131 and renaming it to the "Argus Array." For the 1997 film (''[[Contact (film)|Contact]]''), much of the outdoor footage was shot at the VLA site with the number of dishes visible on screen artificially increased by [[Computer-generated imagery|CGI]], and the canyon depicted as being in the vicinity of the VLA is actually [[Canyon de Chelly National Monument|Canyon de Chelly]] in neighboring [[Arizona]]. It is also seen in the final scene of the alien-invasion film ''[[The Arrival (film)|The Arrival]]'', and the beginning of ''[[Independence Day (film)|Independence Day]]'', when the alien invaders were initially detected by [[SETI]] at the VLA.
New Jersey rock band [[Bon Jovi]] shot the music video for "[[Everyday (Bon Jovi song)|Everyday]]", at the VLA and a "dish" can be seen on the album's cover, named [[Bounce]] . Likewise [[Matt Harding]] can be seen dancing at this location in his second video.
The cover for the [[Dire Straits]] album ''[[On The Night]]'' features the VLA.
The VLA features in plans to save the world from satellites being pulled from orbit in the second volume of the comic book series ''[[G.I. Joe: America's Elite]]'' published by [[Devil's Due Publishing|Devil's Due]].
The VLA can be visited in [[Auto Assault]], a [[massively multiplayer online game]] set in post-apocalyptic America.
==Visiting==
[[Image:USA.NM.VeryLargeArray.03.jpg|thumb|250px|]]
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==
* [[Very Long Baseline Interferometry]]
* [[List of radio telescopes]]
* The [[Very Small Array]]
* The VLA was once used for following up the [[Wow! signal]] from the [[SETI]] project
* British artist [[Keith Tyson]] made an epic 300 piece sculpture called [[Large Field Array]] named after the VLA
* [[Magdalena Ridge Observatory]] is a new observatory under construction a few miles South of the VLA includes an optical [[Interferometer]] and is also run by VLA collaborator [[New Mexico Tech]]
==External links==
* [http://www.vla.nrao.edu NRAO VLA] – official site.
* [http://antwrp.gsfc.nasa.gov/apod/ap060514.html Photo from] [[Astronomy Picture of the Day]]
* [http://www.dustrotter.com/blog/2007/11/north-american-farewell-tour-e-1.html Video of array and interview with VLA press representative]
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[[Category:Radio telescopes]]
[[Category:Interferometric telescopes]]
[[Category:Astronomical observatories in New Mexico]]
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