Las Campanas Observatory
Alternative names | LCO |
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Organization | |
Observatory code | 304, I05 |
Location | Atacama Region, Chile |
Coordinates | 29°00′57″S 70°41′31″W / 29.01597°S 70.69208°W |
Altitude | 2,380 m (7,810 ft) |
Established | 1969 |
Website | www |
Telescopes |
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Related media on Commons | |
Las Campanas Observatory (LCO) is an astronomical observatory owned and operated by the Carnegie Institution for Science (CIS). It is in the southern Atacama Desert of Chile in the Atacama Region approximately 100 kilometres (62 mi) northeast of the city of La Serena. The LCO telescopes and other facilities are near the north end of a 7 km (4.3 mi) long mountain ridge. Cerro Las Campanas, near the southern end and over 2,500 m (8,200 ft) high, is the future home of the Giant Magellan Telescope.[1]
LCO was established in 1969 and is the primary observing facility of CIS. It supplanted Mount Wilson Observatory in that role due to increasing light pollution in the Los Angeles area. The headquarters of Carnegie Observatories is located in Pasadena, California, while the main office in Chile is in La Serena next to the University of La Serena and a short distance from the Association of Universities for Research in Astronomy facility.[2]
It is served by Pelicano Airport, 23 kilometres (14 mi) to the southwest.
Telescopes
- The 6.5 m (260 in) Magellan Telescopes are two identical single-mirror reflecting telescopes. The Walter Baade Telescope saw first light in 2000, and the Landon Clay Telescope in 2002. They are managed by LCO for an international consortium of institutions which includes LCO.[3][4]
- The 2.5 m (98 in) du Pont Telescope is named after industrialist
- The 1.0 m (39 in) Swope Telescope was the first telescope installed at LCO, and began operating in 1971. It is named after CIS astronomer
Tenant telescopes
- The 1.3 m (51 in) Warsaw Telescope is the main instrument of the Ritchey-Chrétien design built by DFM Engineering.[9] Exact location: 29°00′35.8″S 70°42′05.9″W / 29.009944°S 70.701639°W± 1 meter, altitude of the base of the building 2,275 metres (7,464 ft) over mean sea level.
- The variable stars. It consists of two wide-field telescopes, one narrow field telescope, and one ultra-wide field telescope. A prototype system was installed in 1996 and a second in 1997, both in the same enclosure as the 10-inch astrograph. The three larger telescopes were installed in 2000. The ultra-wide device was added in 2002 when the existing telescopes were moved to a new, smaller enclosure.[10] Location: 29°00′36.9″S 70°42′05.1″W / 29.010250°S 70.701417°W± 5 meter.
- The Hungarian Automated Telescope South (HAT-South) facility is part of the transit method. It consists of a pair of four 0.18 m (7.1 in) Takahasi reflecting astrographs on a common mount. It was installed in 2009.[11]
- The Birmingham Solar Oscillations Network (BiSON) operates at station at LCO.[12]
- The Local Volume Mapper of the SDSS-V consists of four telescopes (siderostats) each with 0.16 m diameter near 29°00′39.0″S 70°42′02.34″W / 29.010833°S 70.7006500°W.[13][14][15]
Former telescopes
- The 4.0 m (13.1 ft) NANTEN millimeter-wavelength radio telescope was located at LCO from 1995 to 2004. It is now located at the Pampa La Bola site of the Llano de Chajnantor Observatory and is known as the NANTEN2 Observatory.[16]
- The 0.61 m (24 in) Helen Sawyer Hogg Telescope (HSHT) was operated at LCO by the University of Toronto Southern Observatory from 1971 to 1997. It is now located at Leoncito Astronomical Complex.[17]
- A 0.25 m (10 in) astrograph operated at the site for some time, and was used to discover Supernova 1987A (SN 1987A).[18]
- The Pi of the Sky project operated two wide-angle cameras that searched for the optical signature of gamma ray bursts at LCO starting in 2004. The installation was moved to a commercial telescope hosting site in San Pedro de Atacama in 2011.[19]
Future telescopes
- The Giant Magellan Telescope is an extremely large telescope under construction[20] at LCO, with commissioning expected to begin in 2029. It is 24.5 m (80 ft) effective aperture design with seven 8.4 m (28 ft) segments. The telescope will have a light-gathering area of 368 m2 (3,960 sq ft), which is roughly fifteen times greater than one of the Magellan telescopes. The mirrors are being fabricated by the Steward Observatory Mirror Laboratory, and the first was started in 2005.[21]
Discoveries
On February 24, 1987 at LCO, Ian Shelton and Oscar Duhalde became the first official observers of Supernova 1987A (SN 1987A).[18]
On August 17, 2017 at LCO,
Gallery
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du Pont telescope
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Warsaw telescope dome and control building
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Warsaw telescope
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Clay telescope (one of the Magellan telescopes)
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Magellan telescopes
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Magellan telescopes, Warsaw and Swope telescopes (LTR)
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ASAS telescopes
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BiSON Solar Telescope
See also
References
- ^ Overbye, D., Zegers, M. (April 18, 2023), "A Giant Telescope Grows in Chile", The New York Times, retrieved 22 April 2023
- ^ "History | The Carnegie Observatories". The Carnegie Observatories. Retrieved 2012-01-24.
- ^ "Magellan Telescopes (6.5m) | The Carnegie Observatories". The Carnegie Observatories. Retrieved 2012-01-24.
- ^ "Magellan Telescopes — Las Campanas Observatory". Las Campanas Observatory. Retrieved 2012-01-24.
- ^ "The du Pont Telescope | The Carnegie Observatories". The Carnegie Observatories. Retrieved 2012-01-24.
- ^ "The Irénée du Pont Telescope — Las Campanas Observatory". Las Campanas Observatory. Retrieved 2012-01-24.
- ^ "The Swope Telescope | The Carnegie Observatories". The Carnegie Observatories. Retrieved 2012-01-24.
- ^ "The Henrietta Swope Telescope — Las Campanas Observatory". Las Campanas Observatory. Retrieved 2012-01-24.
- ^ "General Description of OGLE". Warsaw University Observatory. Retrieved 2012-01-24.
- ^ "All Sky Automated Survey - The ASAS-3 System". Warsaw University Observatory. Retrieved 2012-01-24.
- ^ "HAT-South homepage". Harvard Smithsonian Center for Astrophysics. Archived from the original on 2014-02-18. Retrieved 2012-01-24.
- ^ "High-Resolution Optical Spectroscopy - University of Birmingham". University of Birmingham. Retrieved 2012-01-24.
- arXiv:1711.03234 [astro-ph.GA].
- ^ "SDSS-V Pioneering panoptic spectroscopy". Bulletin of the AAS. 51 (7). 2020.
- ^
Herbst, T.; Bilgi, Pavaman (2020). "The SDSS-V local volume mapper telescope system". In Marshall, Heather K; Spyromilio, Jason; Usuda, Tomonori (eds.). Ground-based and Airborne Telescopes VIII. Vol. 11445. SPIE. p. 114450J. S2CID 230583048.
- ^ "The NANTEN2 Telescope | NANTEN". University of Birmingham. Retrieved 2012-01-24.
- ^ "Complejo Astronómico El Leoncito - Helen Sawyer Hogg Telescope". Complejo Astronómico El Leoncito. Retrieved 2012-01-23.
- ^ Bibcode:2007eso..pres....8.
- ^ "Pi of the Sky". Pi of the Sky. Archived from the original on 2012-12-21. Retrieved 2012-01-24.
- ^ "The Giant Magellan Telescope Organization Breaks Ground in Chile" (Press release). GMTO Corporation. 11 November 2015.
- ^ "Overview - Giant Magellan Telescope". GMTO Corporation. Archived from the original on 2011-06-09. Retrieved 2012-01-24.
- S2CID 206664790.