*** Welcome to piglix ***

European Southern Observatory

European Southern Observatory (ESO)
European Southern Observatory (ESO) logo.svgESO member states.svg
ESO logo and map of participating countries
Formation 1962
Type Intergovernmental organization
Purpose Research organization for astronomy
Headquarters Garching, Germany
Membership
16 (15 European countries and Brazil)
Official language
Czech, Danish, Dutch, English, Finnish, French, German, Italian, Norwegian, Polish, Portuguese, Spanish, Swedish
Director General
Tim de Zeeuw
Slogan Reaching New Heights in Astronomy
Website ESO.org

The European Southern Observatory (ESO, formally: European Organization for Astronomical Research in the Southern Hemisphere; French: Organisation Européenne pour des Recherches Astronomiques dans l'Hémisphere Austral) is a 16-nation intergovernmental research organization for ground-based astronomy. Created in 1962, ESO has provided astronomers with state-of-the-art research facilities and access to the southern sky. The organisation employs about 730 staff members and receives annual member state contributions of approximately €131 million. Its observatories are located in northern Chile.

ESO has built and operated some of the largest and most technologically advanced telescopes. These include the New Technology Telescope, an early pioneer in the use of active optics, and the Very Large Telescope (VLT), which consists of four individual telescopes, each with a primary mirror 8.2 metre across, and four smaller auxiliary telescopes. The Atacama Large Millimeter Array observes the universe in the millimetre and submillimetre wavelength ranges, and is the world's largest ground-based astronomy project to date. It was completed in March 2013 in an international collaboration by Europe (represented by ESO), North America, East Asia and Chile.

Currently under construction is the European Extremely Large Telescope. It will use a 39.3-metre-diameter segmented mirror, and become the world's largest optical reflecting telescope when operational in 2024. Its light-gathering power will allow detailed studies of planets around other stars, the first objects in the universe, supermassive black holes, and the nature and distribution of the dark matter and dark energy which dominate the universe.


...
Wikipedia

...