The ESO 3.6-metre Telescope

The ESO 3.6-metre telescope started operations in 1977 and set Europe the exciting engineering challenge of constructing and operating a telescope in the 3–4-metre class in the Southern Hemisphere.

Over the years, the ESO 3.6-metre telescope has been constantly upgraded, including the installation of a new secondary mirror that has kept the telescope in its place as one of the most efficient and productive engines of astronomical research.

The telescope hosts HARPS, the High Accuracy Radial velocity Planet Searcher, the world’s foremost exoplanet hunter. HARPS is a spectrograph with unrivalled precision and is the most successful finder of low-mass exoplanets to date.

More details can be found on the telescope page.

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, Chile
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