VISTA (telescope)
The VISTA (Visible and Infrared Survey Telescope for Astronomy) is a wide-field reflecting telescope with a 4.1 metre mirror, located at the Paranal Observatory in Chile. It is operated by the European Southern Observatory and started science operations in December 2009. VISTA was conceived and developed by a consortium of universities in the United Kingdom led by Queen Mary University of London and became an in-kind contribution to ESO as part of the UK's accession agreement, with the subscription paid by the UK Science and Technology Facilities Council (STFC).
VISTA (Credit: ESO) | |
| Alternative names | Visible and Infrared Survey Telescope for Astronomy |
|---|---|
| Part of | Paranal Observatory |
| Location(s) | Atacama Desert |
| Coordinates | 24°36′57″S 70°23′51″W |
| Organization | European Southern Observatory |
| Altitude | 2,518 m (8,261 ft) |
| Wavelength | 0.85 μm (350 THz)–2.3 μm (130 THz) |
| First light | 1 December 2009 |
| Telescope style | Ritchey–Chrétien telescope |
| Diameter | 4.1 m (13 ft 5 in) |
| Secondary diameter | 1.24 m (4 ft 1 in) |
| Angular resolution | 0.34 arcsecond |
| Focal length | 12.1 m (39 ft 8 in) |
| Mounting | altazimuth mount |
| Website | www |
Location of VISTA | |
| Related media on Commons | |
VISTA is a survey telescope working at infrared wavelengths, and is by far the largest telescope in the world dedicated to surveying the sky at near-infrared wavelengths. The telescope has only one instrument: VIRCAM, the Vista InfraRed CAMera. This is a 3-tonne camera containing 16 special detectors sensitive to infrared light, with a combined total of 67 million pixels.
A second-generation instrument called 4MOST, a 2400-object fibre-fed multi-object spectrograph, is under development for installation around 2022.
Observing at wavelengths longer than those visible to the human eye allows VISTA to study objects that may be almost impossible to see in visible light because they are cool, obscured by dust clouds or because their light has been stretched towards redder wavelengths by the expansion of space during the light's long journey from the early Universe.