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Las Campanas Observatory

Coordinates:29°00′57″S70°41′31″W / 29.01597°S 70.69208°W /-29.01597; -70.69208
From Wikipedia, the free encyclopedia
Observatory
Las Campanas Observatory
Telescopes at Las Campanas Observatory
Alternative namesLCOEdit this at Wikidata
Organization
Observatory code 304, I05 Edit this on Wikidata
LocationAtacama Region, Chile
Coordinates29°00′57″S70°41′31″W / 29.01597°S 70.69208°W /-29.01597; -70.69208
Altitude2,380 m (7,810 ft)Edit this at Wikidata
Established1969 Edit this on Wikidata
Websitewww.lco.clEdit this at Wikidata
Telescopes
Las Campanas Observatory is located in Chile
Las Campanas Observatory
Location of Las Campanas Observatory
Map
 Related media on Commons

Las Campanas Observatory (LCO) is anastronomicalobservatory managed by theCarnegie Institution for Science (CIS). Located inChile'sAtacama Region, it sits about 100 kilometres (62 mi) northeast of the city ofLa Serena. The LCO's telescopes and facilities are positioned near the northern end of a 7 km (4.3 mi)mountain ridge. Cerro Las Campanas, situated near the southern end of this ridge and standing over 2,500 m (8,200 ft) tall, will be the future site of theGiant Magellan Telescope.[1]

Established in 1969, LCO is CIS's primary observatory, having taken over this role fromMount Wilson Observatory due to increasing light pollution in theLos Angeles area. The headquarters of Carnegie Observatories is inPasadena, California, while the main office in Chile is in La Serena, close to theUniversity of La Serena and near theAssociation of Universities for Research in Astronomy facility.[2]

The observatory is served byPelicano Airport, located 23 kilometres (14 mi) to the southwest. Prior to the establishment of the observatory on Cerro Las Campanas the mountain ofCerro Morado was surveyed in late 1962 and early 1963 as a potential site.[3]

Telescopes

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Tenant telescopes

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Former telescopes

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Future telescopes

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  • TheGiant Magellan Telescope is anextremely large telescope under construction[21] at LCO, with commissioning expected to begin in 2029. It is 24.5 m (80 ft) effectiveaperture 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 theSteward Observatory Mirror Laboratory, and the first was started in 2005.[22]

Discoveries

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On February 24, 1987 at LCO,Ian Shelton and Oscar Duhalde became the first official observers of Supernova 1987A (SN 1987A).[19]

On August 17, 2017 at LCO,SSS17a, the optical counterpart to the gravitational wave sourceGW170817, was discovered with the Swope telescope.[23]

Gallery

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  • du Pont telescope
    du Pont telescope
  • Warsaw telescope dome and control building
    Warsaw telescope dome and control building
  • Warsaw telescope
    Warsaw telescope
  • Clay telescope (one of the Magellan telescopes)
    Clay telescope (one of the Magellan telescopes)
  • Magellan telescopes
    Magellan telescopes
  • Magellan telescopes, Warsaw and Swope telescopes (LTR)
    Magellan telescopes, Warsaw and Swope telescopes (LTR)
  • ASAS telescopes
    ASAS telescopes
  • BiSON Solar Telescope
    BiSON Solar Telescope

See also

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References

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  1. ^Overbye, D., Zegers, M. (April 18, 2023),"A Giant Telescope Grows in Chile",The New York Times, retrieved22 April 2023
  2. ^"History | The Carnegie Observatories". The Carnegie Observatories. Archived fromthe original on 2013-08-09. Retrieved2012-01-24.
  3. ^"Windows to the Universe (multiple locations): AURA Observatory, Chile".Portal to the Heritage of Astronomy. Retrieved2025-07-01.
  4. ^"Magellan Telescopes (6.5m) | The Carnegie Observatories". The Carnegie Observatories. Archived fromthe original on 2017-05-25. Retrieved2012-01-24.
  5. ^"Magellan Telescopes — Las Campanas Observatory". Las Campanas Observatory. Retrieved2012-01-24.
  6. ^"The du Pont Telescope | The Carnegie Observatories". The Carnegie Observatories. Retrieved2012-01-24.[permanent dead link]
  7. ^"The Irénée du Pont Telescope — Las Campanas Observatory". Las Campanas Observatory. Retrieved2012-01-24.
  8. ^"The Swope Telescope | The Carnegie Observatories". The Carnegie Observatories. Archived fromthe original on 2017-10-18. Retrieved2012-01-24.
  9. ^"The Henrietta Swope Telescope — Las Campanas Observatory". Las Campanas Observatory. Retrieved2012-01-24.
  10. ^"General Description of OGLE". Warsaw University Observatory. Retrieved2012-01-24.
  11. ^"All Sky Automated Survey - The ASAS-3 System". Warsaw University Observatory. Retrieved2012-01-24.
  12. ^"HAT-South homepage". Harvard Smithsonian Center for Astrophysics. Archived fromthe original on 2014-02-18. Retrieved2012-01-24.
  13. ^"High-Resolution Optical Spectroscopy - University of Birmingham". University of Birmingham. Retrieved2012-01-24.
  14. ^Kollmeier, Juna A.; Zasowski, Gail; Rix, Hans-Walter; Johns, Matt; Anderson, Scott F.; Drory, Niv; Johnson, Jennifer A.; Pogge, Richard W.; Bird, Jonathan C.; Blanc, Guillermo A.; Brownstein, Joel R.; Crane, Jeffrey D.; De Lee, Nathan M.; Klaene, Mark A.; Kreckel, Kathryn; MacDonald, Nick; Merloni, Andrea; Ness, Melissa K.; O'Brien, Thomas; Sanchez-Gallego, Jose R.; Sayres, Conor C.; Shen, Yue; Thakar, Ani R.; Tkachenko, Andrew; Aerts, Conny; Blanton, Michael R.; Eisenstein, Daniel J.; Holtzman, Jon A.; Maoz, Dan; et al. (2017). "SDSS-V: pioneering panoptic spectroscopy".arXiv:1711.03234 [astro-ph.GA].
  15. ^"SDSS-V Pioneering panoptic spectroscopy".Bulletin of the AAS.51 (7). 2020.
  16. ^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.doi:10.1117/12.2561419.ISBN 9781510636774.S2CID 230583048.
  17. ^"The NANTEN2 Telescope | NANTEN". University of Birmingham. Retrieved2012-01-24.
  18. ^"Complejo Astronómico El Leoncito - Helen Sawyer Hogg Telescope". Complejo Astronómico El Leoncito. Retrieved2012-01-23.
  19. ^ab"SN1987A's Twentieth Anniversary".ESO Press Release: 8. 2007.Bibcode:2007eso..pres....8.
  20. ^"Pi of the Sky". Pi of the Sky. Archived fromthe original on 2012-12-21. Retrieved2012-01-24.
  21. ^"The Giant Magellan Telescope Organization Breaks Ground in Chile" (Press release). GMTO Corporation. 11 November 2015.
  22. ^"Overview - Giant Magellan Telescope". GMTO Corporation. Archived fromthe original on 2011-06-09. Retrieved2012-01-24.
  23. ^Coulter, D. A.; Foley, R. J.; Kilpatrick, C. D.; Drout, M. R.; Piro, A. L.; Shappee, B. J.; Siebert, M. R.; Simon, J. D.; Ulloa, N. (2017-10-16)."Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source".Science.358 (6370):1556–1558.arXiv:1710.05452.Bibcode:2017Sci...358.1556C.doi:10.1126/science.aap9811.ISSN 0036-8075.PMID 29038368.S2CID 206664790.

External links

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