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ESO 3.6 m Telescope

Coordinates: 29°15′39″S 70°43′54″W / 29.26097°S 70.73169°W / -29.26097; -70.73169
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"ADONIS" redirects here. For the encryption machine, see KL-7. For other uses, see adonis (disambiguation).
ESO 3.6 m Telescope
Alternative namesThe ESO 3.6m at La Silla Edit this at Wikidata
Part ofLa Silla Observatory Edit this on Wikidata
Location(s)Chile Edit this at Wikidata
Coordinates29°15′39″S 70°43′54″W / 29.26097°S 70.73169°W / -29.26097; -70.73169 Edit this at Wikidata
OrganizationEuropean Southern Observatory Edit this on Wikidata
Altitude2,400 m (7,900 ft) Edit this at Wikidata
First light1977 Edit this on Wikidata
Telescope styleinfrared telescope
reflecting telescope Edit this on Wikidata
Diameter3.566 m (11 ft 8.4 in) Edit this at Wikidata
Angular resolution0.2 arcsecond Edit this on Wikidata
Collecting area8.8564 m2 (95.329 sq ft) Edit this at Wikidata
Websitewww.eso.org/sci/facilities/lasilla/telescopes/3p6.html Edit this at Wikidata
ESO 3.6 m Telescope is located in Chile
ESO 3.6 m Telescope
Location of ESO 3.6 m Telescope
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ESO 3.6 m Telescope

The ESO 3.6 m Telescope is an optical reflecting telescope run by the European Southern Observatory at La Silla Observatory, Chile since 1977, with a clear aperture of about 3.6 metres (140 in) and 8.6 m2 (93 sq ft) area.

The telescopes uses the HARPS instrument and has discovered more than 130 exoplanets. In 2012, it discovered Alpha Centauri Bb, a now-disproven possible planet in the Alpha Centauri system only 4.4 light-years away.[1]

ESO collaborated with CERN on building the telescope.[2][3] It saw first light in 1976 and entered full operations in 1977.[4] When completed it was one of the world's largest optical telescopes. 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 ADONIS, one of the first adaptive optics system available to the astronomical community in the 1980s.

Instruments

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Since 22, the ESO 3.6 m telescope has hosted HARPS, the High Accuracy Radial Velocity Planet Searcher and NIRPS, the Near Infra Red Planet Searcher. HARPS is a fibre-fed high resolution echelle spectrograph dedicated to the discovery of extrasolar planets. Other instruments on the telescope, now decommissioned, include:[5]

  • CES: is a spectrograph that provides a resolving power of up to 235,000 in the 346–1028 nm region.
  • EFOSC2: the ESO Faint Object Spectrograph and Camera (v.2), is a very versatile instrument for low resolution spectroscopy and imaging.
  • TIMMI-2: the Thermal Infrared MultiMode Instrument dedicated to the 3–25 μm spectrum.
  • ADONIS: is the acronym for Adaptive Optics Near Infrared System, and was a second-generation adaptive optics system for the astronomical community.[6] More than 40 peer-reviewed scientific articles were published based on this instrument data.[7] 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 ESO instrument,[8] then decommissioned in 2001. ADONIS was the first AO system offered to a large community of astronomers.

Recent scientific achievements

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The ESO 3.6 backdropped by the southern sky, and annotated note for the recently discovered Nova Centauri 2013

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, Gliese 581e, with only twice the mass of the Earth,[9] and the richest planetary system known at the time, with up to seven planets orbiting a Sun-like star.[10]

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 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.[11]

The discovery of the extrasolar planet Gliese 581 c by the team of Stéphane Udry at University of Geneva's Observatory in Switzerland was announced on April 24, 2007.[12] The team used the telescope's HARPS spectrograph, and employed the radial velocity technique to identify the planet's influence on the star.[12][13]

By 2009, the telescope was used to discover 75 exoplanet candidates.[14] In 2011, another 50 exoplanet candidates were announced.[15]

Contemporaries on commissioning

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Largest optical astronomical telescopes in 1976
# Name
(observatory) 		Image Aperture M1
area 		Altitude First
light 		Special advocate
1. BTA-6
(Special Astrophysical Obs) 		238 inch
605 cm 		26 m2 2,070 m (6,790 ft) 1975 Mstislav Keldysh
2. Hale Telescope
(Palomar Observatory) 		200 inch
508 cm 		20 m2 1,713 m (5,620 ft) 1949 George Ellery Hale
3. Mayall Telescope
(Kitt Peak National Obs.) 		158 inch
401 cm 		10 m2 2,120 m (6,960 ft) 1973 Nicholas Mayall
4. Víctor M. Blanco Telescope
(CTIO Observatory) 		158 inch
401 cm 		10 m2 2,200 m (7,200 ft) 1976 Nicholas Mayall
5. Anglo-Australian Telescope
(Siding Spring Observatory) 		153 inch
389 cm 		12 m2 1,742 m (5,715 ft) 1974 Prince Charles
6. ESO 3.6 m Telescope
(La Silla Observatory) 		140 inch
357 cm 		8.8 m2 2,400 m (7,900 ft) 1976 Adriaan Blaauw
7. Shane Telescope
(Lick Observatory) 		120 inch
305 cm 		~7 m2 1,283 m (4,209 ft) 1959 Nicholas Mayall
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Telescope and site

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  • The ESO 3.6-metre telescope.
    The ESO 3.6-metre telescope.
  • The road to the telescope at La Silla.
    The road to the telescope at La Silla.
  • Euler Telescope and the ESO 3.6 m Telescope (background).
    Euler Telescope and the ESO 3.6 m Telescope (background).
  • Panoramic view of the ESO 3.6-metre telescope's dome.
    Panoramic view of the ESO 3.6-metre telescope's dome.
  • La Silla—Early evening scenery (in the distant right: the ESO 3.6 m T.)
    La Silla—Early evening scenery (in the distant right: the ESO 3.6 m T.)
  • Construction of the ESO 3.6-metre telescope.[16]
    Construction of the ESO 3.6-metre telescope.[16]

Images from telescope

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See also

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References

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  1. ^ http://www.planetary.org, Bruce Betts, B. Betts - First Planet Discovered in Alpha Centauri System - TPS, 18 October 2012
  2. ^ Madsen, Claus (2012). The jewel on the mountaintop : fifty years of the European Southern Observatory. [Weinheim]: Wiley-VCH. ISBN 978-3-527-41203-7. OCLC 818323656.
  3. ^ Reiz, Anders (1974). ESO/SRC/CERN Conference on Research Programmes for the New Large Telescopes, Geneva, 27-31 May 1974: Proceedings. Organizing Committee of the Conference.
  4. ^ "Telescopes and Instrumentation, the ESO 3.6-metre Telescope" (Table on the right of the page). Retrieved 2011-05-02.
  5. ^ "The ESO 3.6m Telescope". Retrieved 2011-05-26.
  6. ^ Jack B. Zirker (2005). An acre of glass: a history and forecast of the telescope. JHU Press. pp. 204. ISBN 978-0-8018-8234-0.
  7. ^ ADS query results for "ADONIS"
  8. ^ Gérard Rousset and Jean-Luc Beuzit (1999). "The COME-ON/ADONIS systems". In François Roddier (ed.). Adaptive optics in astronomy. Cambridge University Press. pp. 171 et seq. ISBN 978-0-521-55375-9.
  9. ^ "Lightest exoplanet yet discovered". ESO. 2009-04-21. Retrieved 2011-05-26.
  10. ^ "Richest Planetary System Discovered". ESO. 2010-08-24. Retrieved 2011-05-26.
  11. ^ "Pulsating Star Mystery Solved". ESO. 2010-11-24. Retrieved 2011-05-26.
  12. ^ a b Than, Ker (2007-04-24). "Major Discovery: New Planet Could Harbor Water and Life". space.com. Retrieved 2007-04-29.
  13. ^ Than, Ker (2007-02-24). "Planet Hunters Edge Closer to Their Holy Grail". space.com. Retrieved 2007-04-29.
  14. ^ "32 planets discovered outside solar system - CNN.com". CNN. 19 October 2009. Retrieved 4 May 2010.
  15. ^ 50 new exoplanets discovered by HARPS
  16. ^ "Three Very Different Telescopes at La Silla". ESO Picture of the Week. Retrieved 8 May 2012.
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