News

This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • Antonin Bouchez (GMT). Crédito: Elena Mora (IAC).
    En el Observatorio de las Campanas, en el desierto de Atacama, en Chile, se está construyendo uno de los llamados “Telescopios Extremadamente Grandes”: el Telescopio Gigante de Magallanes (GMT, de sus siglas en inglés), de 24,5 m de diámetro y que, en principio, estará disponible en 2022. Su nombre recuerda al navegante y explorador portugués cuya expedición descubriría el paso entre el Océano Atlántico y el Pacífico y acabaría dando por primera vez la vuelta al mundo. El GMT, perteneciente a un consorcio internacional liderado por Estados Unidos - Giant Magellan Telescope Organization (GMTO
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  • Norbert Hubin. Credit: Elena Mora (IAC)
    “Although giant telescopes are under construction, astronomical images with good resolution cannot be obtained unless they use Adaptive Optics”, warns Norbert Hubin, head of instrumentation at the Very Large Telescope (VLT), a system of four 8.2 m telescopes installed at the European Southern Observatory (ESO) Observatory in La Silla, Chile. It was on the telescope of 3.6 m of that observatory where the first system of Adaptive Optics in the history of the Astronomy (called "COME-ON") was tried. This engineer was in Tenerife this week attending the conference on "Adaptive Optics for
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  • Participantes en el congreso sobre “Óptica Adaptativa para Telescopios Extremadamente Grandes” (AO4ELT5). Crédito: Elena Mora (IAC).
    The conference on "Adaptive Optics for Extremely Large Telescopes" (AO4ELT5) which brought together in Tenerife almost 300 international specialists in this astronomical technique, was brought to a close this afternoon. This meeting, organized by the Instituto de Astrofísica de Canarias (IAC), has explored the common ground between astronomy and engineering which will improve the quality of the five projected future extremely large telescopes -the solar telescopes DKIST and EST, and the night-time telescopes GMT, TMT and E-ELT-, as well as for the present large telescopes, among them the
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