La Silla

ESO's first observatory


La Silla
La Silla
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NTT

Name: New Technology Telescope (NTT)
Type: optical and infrared telescope
Aperture: 3.58 m
Optical design: Ritchey–Chrétien
Field of View: [see instruments]
Mounting: altazimuth
Location: La Silla
Housing: rotating dome
Start of operations: 1989
Wavelength range: [see instruments]
Instrumentation: SOFI, EFOSC2
Note: first telescope using full active optics

ESO 3.6-metre telescope

Name: ESO 3.6-metre telescope
Type: optical and near-infrared telescope
Aperture: 3.57 m
Optical design: Cassegrain
Mounting: equatorial, horseshoe
Location: La Silla
Housing: dome
Start of operations: 1976
Wavelength range: 380–690 nm
Instrumentation: HARPS — High Accuracy Radial velocity Planet Searcher (fibre-fed, cross-dispersed Echelle spectrograph)
Detectors: mosaic of 2 CCDs (altogether 4k x 4k pixel)
Spectral Resolution 115 000
Start of Operations 2003 (HARPS only)
Science goals: search for exoplanets; asteroseismology

MPG/ESO 2.2-metre telescope

Name: MPG/ESO 2.2-metre telescope
Type: optical (and near-infrared) telescope
Aperture: 2.20 m
Optical design: Ritchey–Chrétien
Field of view: 33 arcminutes, free from vignetting
Mounting: equatorial, fork
Location: La Silla 
Housing: dome
Start of operations: 1983
Wavelength range: [see instruments]
Instrumentation: WFI, FEROS, GROND

Decommissioned La Silla telescopes

ESO 1.52 m telescope
ESO 1 m telescope
ESO 0.5 m telescope (now at the Observatorio UC in Santiago, Chile)
Swedish-ESO Submillimetre Telescope (SEST) 15 m
Coudé Auxiliary Telescope (CAT) 1.4 m
Schmidt 1 m
Grand Prism Objectif (GPO)
Marly 1 m
90 cm Dutch (National telescope)
50 cm Danish (National telescope)
Marseille 40 cm (National telescope)
Bochum 61 cm (National telescope)

The La Silla Observatory, 600 km north of Santiago de Chile and at an altitude of 2400 metres, has been an ESO stronghold since the 1960s. Here, ESO operates several of the most productive 4-metre class telescopes in the world.

The 3.58-metre New Technology Telescope (NTT) broke new ground for telescope engineering and design and was the first in the world to have a computer-controlled main mirror (active optics), a technology developed at ESO and now applied to most of the world's current large telescopes.

The ESO 3.6-metre telescope is now home to the world's foremost extrasolar planet hunter: HARPS (High Accuracy Radial velocity Planet Searcher), a spectrograph with unrivalled precision.

The La Silla Observatory is the first world-class observatory to have been granted certification for the International Organization for Standardization (ISO) 9001 Quality Management System. The infrastructure of La Silla is also used by many of the ESO member states for targeted projects such as the Swiss 1.2-metre Euler telescope, the Rapid-Eye Mount (REM) and TAROT gamma-ray burst chaser, as well as more common user facilities such as the 2.2-metre Max Planck and the 1.5-metre Danish telescopes. The 67-million pixel Wide Field Imager on the 2.2-metre telescope has taken many amazing images of celestial objects, some of which have now become icons in their own right.


With about 300 refereed publications attributable to the work of the observatory per year, La Silla remains at the forefront of astronomy. La Silla has led to an enormous number of scientific discoveries, including several "firsts". The HARPS spectrograph is the undisputed champion at finding low-mass extrasolar planets. It detected the system around Gliese 581, which contains what may be the first known rocky planet in a habitable zone, outside the Solar System (ESO 22/07). Several telescopes at La Silla played a crucial role in linking gamma-ray bursts — the most energetic explosions in the Universe since the Big Bang — with the explosions of massive stars. Since 1987, the ESO La Silla Observatory has also played an important role in the study and follow-up of the nearest recent supernova, SN 1987A.

The La Silla Observatory is located at the outskirts of the Chilean Atacama Desert, one of the driest and loneliest areas of the world. Like other observatories in this geographical area, La Silla is located far from sources of light pollution and, like the Paranal Observatory, home to the Very Large Telescope, it has one of the darkest night skies on the Earth.

 

Some more details about the operational instruments on La Silla is available on a separate page and via the Science Instrumentation page.

More images and videos are available in the ESO multimedia archive.

Read more
Read more on about this observatory on the ESO Handout in PDF format.

 

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La Silla on Google Map

 

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