Template:Short description Template:Redirect Template:Infobox 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 Template:Convert and Template:Convert 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.<ref>http://www.planetary.org, Bruce Betts, B. Betts - First Planet Discovered in Alpha Centauri System - TPS, 18 October 2012</ref>
ESO collaborated with CERN on building the telescope.<ref>Template:Cite book</ref><ref>Template:Cite book</ref> It saw first light in 1976 and entered full operations in 1977.<ref name="eso.org">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> 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.
InstrumentsEdit
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:<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
- 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.<ref name=Zirker2005/> More than 40 peer-reviewed scientific articles were published based on this instrument data.<ref name=SIMBAD_ADONIS/> 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,<ref name=RoussetBeuzit1999/> then decommissioned in 2001. ADONIS was the first AO system offered to a large community of astronomers.
Recent scientific achievementsEdit
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,<ref>Template:Cite news</ref> and the richest planetary system known at the time, with up to seven planets orbiting a Sun-like star.<ref>Template:Cite news</ref>
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.<ref>Template:Cite news</ref>
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.<ref name="space.com">Template:Cite news</ref> The team used the telescope's HARPS spectrograph, and employed the radial velocity technique to identify the planet's influence on the star.<ref name="space.com" /><ref>Template:Cite news</ref>
By 2009, the telescope was used to discover 75 exoplanet candidates.<ref name="cnn.com">Template:Cite news</ref> In 2011, another 50 exoplanet candidates were announced.<ref>50 new exoplanets discovered by HARPS</ref>
Contemporaries on commissioningEdit
GalleryEdit
Telescope and siteEdit
- 3.6-m Telescope at La Silla.jpg
The ESO 3.6-metre telescope.
- 3,6-m Telescope at La Silla.jpg
The road to the telescope at La Silla.
- LaSillaByNight2.jpg
Euler Telescope and the ESO 3.6 m Telescope (background).
- La Silla 3.6m telescope.jpg
Panoramic view of the ESO 3.6-metre telescope's dome.
- ESO-The Milky Way above La Silla-phot-27-04-hires.jpg
La Silla—Early evening scenery (in the distant right: the ESO 3.6 m T.)
- Construction of the ESO 3.6-metre telescope.jpg
Construction of the ESO 3.6-metre telescope.<ref>Template:Cite news</ref>
Images from telescopeEdit
- NGC 520.tif
See alsoEdit
- List of largest optical reflecting telescopes
- List of largest optical telescopes in the 20th century