Very Large Telescope

Very Large Telescope
The four Unit Telescopes that form the VLT together with the four Auxiliary Telescopes (VST at right)
Alternative namesVLT Edit this at Wikidata
Part ofParanal Observatory Edit this on Wikidata
Location(s)Antofagasta Region, Chile
Coordinates24°37′38″S 70°24′15″W / 24.62733°S 70.40417°W / -24.62733; -70.40417 Edit this at Wikidata
OrganizationEuropean Southern Observatory Edit this on Wikidata
Altitude2,635 m (8,645 ft) Edit this at Wikidata
Observing time320 nights per year Edit this on Wikidata
Wavelength300 nm – 20 μm (N-UV, visible light, NIR, SWIR, MWIR, and LWIR)
First light1998; 26 years ago (1998) (for the first Unit Telescope)
Telescope styleastronomical observatory Edit this on Wikidata
Diameter
  • 4 × 8.2-metre Unit Telescopes (UT)
  • 4 × 1.8-metre moveable Auxiliary Telescopes (AT)
Angular resolution0.002 arcsecond Edit this on Wikidata
Focal length120 m (393 ft 8 in) Edit this at Wikidata
Websitewww.eso.org/vlt Edit this at Wikidata
Very Large Telescope is located in Chile
Very Large Telescope
Location of Very Large Telescope
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The Very Large Telescope (VLT) is an astronomical facility operated since 1998 by the European Southern Observatory, located on Cerro Paranal in the Atacama Desert of northern Chile. It consists of four individual telescopes, each equipped with a primary mirror that measures 8.2 meters in diameter. These optical telescopes, named Antu, Kueyen, Melipal, and Yepun (all words for astronomical objects in the Mapuche language), are generally used separately but can be combined to achieve a very high angular resolution.[1] The VLT array is also complemented by four movable Auxiliary Telescopes (ATs) with 1.8-meter apertures.

The VLT is capable of observing both visible and infrared wavelengths. Each individual telescope can detect objects that are roughly four billion times fainter than what can be seen with the naked eye. When all the telescopes are combined, the facility can achieve an angular resolution of approximately 0.002 arcsecond. In single telescope mode, the angular resolution is about 0.05 arcseconds.[2]

The VLT is one of the most productive facilities for astronomy, second only to the Hubble Space Telescope in terms of the number of scientific papers produced from facilities operating at visible wavelengths.[3] Some of the pioneering observations made using the VLT include the first direct image of an exoplanet, the tracking of stars orbiting around the supermassive black hole at the centre of the Milky Way, and observations of the afterglow of the furthest known gamma-ray burst.[4]

  1. ^ "The Very Large Telescope". ESO. Retrieved 2011-08-05.
  2. ^ "FAQ VLT/Paranal". eso.org.
  3. ^ Trimble, V.; Ceja, J. A. (2010). "Productivity and impact of astronomical facilities: A recent sample" (PDF). Astronomische Nachrichten. 331 (3): 338. Bibcode:2010AN....331..338T. doi:10.1002/asna.200911339. S2CID 54516166.
  4. ^ "The Very Large Telescope – The World's Most Advanced Visible-light Astronomical Observatory handout". ESO. Retrieved 2011-08-05.