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 3.6m (11.8feet) and 8.6m2 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.
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]
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,[6] and the richest planetary system known at the time, with up to seven planets orbiting a Sun-like star.[7]
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.[8]
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.[9] The team used the telescope's HARPS spectrograph, and employed the radial velocity technique to identify the planet's influence on the star.[10]
By 2009, the telescope was used to discover 75 exoplanet candidates.[11] In 2011, another 50 exoplanet candidates were announced.[12]
| width=18 | Name (observatory) | Image | Aperture | width=60 | M1 area | Altitude | width=60 | First light | Special advocate | |
|---|---|---|---|---|---|---|---|---|---|---|
| align=left | BTA-6 | bgcolor=#ddd | 238 inch 605 cm | 26 m2 | 2070m (6,790feet) | 1975 | Mstislav Keldysh | |||
| align=left | Hale Telescope | bgcolor=#ddd | 200 inch 508 cm | 20 m2 | 1713m (5,620feet) | 1949 | ||||
| align=left | Mayall Telescope | bgcolor=#ddd | 158 inch 401 cm | 10 m2 | 2120m (6,960feet) | --> | 1973 | Nicholas Mayall | ||
| align=left | Víctor M. Blanco Telescope | bgcolor=#ddd | 158 inch 401 cm | 10 m2 | 2200m (7,200feet) | 1976 | Nicholas Mayall | |||
| align=left | Anglo-Australian Telescope | bgcolor=#ddd | 153 inch 389 cm | 12 m2 | 1742m (5,715feet) | 1974 | ||||
| align=left | ESO 3.6 m Telescope | bgcolor=#ddd | 140 inch 357 cm | 8.8 m2 | 2400m (7,900feet) | 1976 | Adriaan Blaauw | |||
| align=left | Shane Telescope | bgcolor=#ddd | 120 inch 305 cm | ~7 m2 | 1283m (4,209feet) | 1959 | Nicholas Mayall |