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The telescope was also involved in solving a decades-old mystery regarding the mass of
Cepheid variable stars. By using the HARPS instrument, astronomers detected for the first time a double star where a pulsating Cepheid variable and another star pass in front of one another, which allows to measure
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system for the astronomical community. More than 40 peer-reviewed scientific articles were published based on this instrument data. ADONIS is the final version of diverse
Adaptive Optics (AO) prototypes named Come-on and Come-on +. It was offered in its final version in October 1996 as an official
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The ESO 3.6 m telescope has made several scientific discoveries since it saw first light. Recent astronomical achievements were made possible by HARPS, a "top-class" instrument. This include finding the lightest exoplanet known at the time of discovery in,
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the mass of the
Cepheid. The study concluded that the mass prediction coming from the theory of stellar pulsation was correct while the value calculated was at odds with the theory of stellar evolution.
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383:. It received an overhaul in 1999 and a new secondary in 2004. The ESO 3.6-metre Telescope has supported many scientific achievements and presented
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on building the telescope. It saw first light in 1976 and entered full operations in 1977. When completed it was one of the
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instrument, then decommissioned in 2001. ADONIS was the first AO system offered to a large community of astronomers.
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dedicated to the discovery of extrasolar planets. Other instruments on the telescope, now decommissioned, include:
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ESO/SRC/CERN Conference on
Research Programmes for the New Large Telescopes, Geneva, 27-31 May 1974: Proceedings
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since 1977, with a clear aperture of about 3.6 metres (140 in) and 8.6 m (93 sq ft) area.
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Gérard
Rousset and Jean-Luc Beuzit (1999). "The COME-ON/ADONIS systems". In François Roddier (ed.).
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The ESO 3.6 backdropped by the southern sky, and annotated note for the recently discovered
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The jewel on the mountaintop : fifty years of the
European Southern Observatory
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and NIRPS, the Near Infra Red Planet
Searcher. HARPS is a fibre-fed high resolution
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candidates. In 2011, another 50 exoplanet candidates were announced.
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B. Betts - First Planet
Discovered in Alpha Centauri System - TPS
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was announced on April 24, 2007. The team used the telescope's
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1129:"Telescopes and Instrumentation, the ESO 3.6-metre Telescope"
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Since 22, the ESO 3.6 m telescope has hosted HARPS, the
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system available to the astronomical community in the 1980s.
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technique to identify the planet's influence on the star.
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1314:"Major Discovery: New Planet Could Harbor Water and Life"
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An acre of glass: a history and forecast of the telescope
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19:"ADONIS" redirects here. For the encryption machine, see
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1357:"32 planets discovered outside solar system - CNN.com"
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List of largest optical telescopes in the 20th century
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Panoramic view of the ESO 3.6-metre telescope's dome.
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1336:"Planet Hunters Edge Closer to Their Holy Grail"
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529:Largest optical astronomical telescopes in 1976
516:By 2009, the telescope was used to discover 75
1511:Space Telescope European Coordinating Facility
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935:and the ESO 3.6 m Telescope (background).
422:ESO Faint Object Spectrograph and Camera (v.2)
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1396:"Three Very Different Telescopes at La Silla"
1036:List of largest optical reflecting telescopes
977:Construction of the ESO 3.6-metre telescope.
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401:High Accuracy Radial Velocity Planet Searcher
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1117:. Organizing Committee of the Conference.
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489:The discovery of the extrasolar planet
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204:3.566 m (11 ft 8.4 in)
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920:The road to the telescope at La Silla.
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1384:50 new exoplanets discovered by HARPS
1268:"Richest Planetary System Discovered"
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432:Thermal Infrared MultiMode Instrument
16:Optical reflecting telescope in Chile
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446:Adaptive Optics Near Infrared System
1775:Astronomical observatories in Chile
1247:"Lightest exoplanet yet discovered"
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381:world's largest optical telescopes
372:system only 4.4 light-years away.
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298:Location of ESO 3.6 m Telescope
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783:1,742 m (5,715 ft)
737:2,200 m (7,200 ft)
691:2,120 m (6,960 ft)
645:1,713 m (5,620 ft)
599:2,070 m (6,790 ft)
343:European Southern Observatory
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135:European Southern Observatory
1685:Astronomy & Astrophysics
1219:Adaptive optics in astronomy
908:The ESO 3.6-metre telescope.
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1334:Than, Ker (2007-02-24).
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1150:"The ESO 3.6m Telescope"
1060:http://www.planetary.org
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356:The telescopes uses the
315:Related media on Commons
1400:ESO Picture of the Week
1225:. pp. 171 et seq.
1169:Jack B. Zirker (2005).
962:—Early evening scenery
670:Kitt Peak National Obs.
25:adonis (disambiguation)
1076:Madsen, Claus (2012).
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375:ESO collaborated with
45:Alternative names
23:. For other uses, see
1111:Reiz, Anders (1974).
983:Images from telescope
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444:: is the acronym for
110:29.26097°S 70.73169°W
1550:(under construction)
1496:La Silla Observatory
1432:at Wikimedia Commons
1005:(captured by EFOSC2)
808:La Silla Observatory
499:University of Geneva
405:echelle spectrograph
347:La Silla Observatory
231:Collecting area
187:reflecting telescope
179:Telescope style
115:-29.26097; -70.73169
62:La Silla Observatory
1506:Paranal Observatory
1430:ESO 3.6-m Telescope
802:ESO 3.6 m Telescope
624:Palomar Observatory
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387:, one of the first
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219:0.2 arcsecond
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1765:Optical telescopes
1446:ADONIS ESO webpage
1023:colliding galaxies
895:Telescope and site
652:George Ellery Hale
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501:'s Observatory in
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472:Nova Centauri 2013
215:Angular resolution
183:infrared telescope
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1436:ESO 3.6m homepage
1428:Media related to
1365:. 19 October 2009
1291:. ESO. 2010-11-24
1270:. ESO. 2010-08-24
1249:. ESO. 2009-04-21
1232:978-0-521-55375-9
1192:978-0-8018-8234-0
1089:978-3-527-41203-7
1066:, 18 October 2012
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