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.

  • Attendees at the Spanish ALMA Day 2025
    The Instituto de Astrofísica de Canarias (IAC) has been host to the Spanish ALMA Days 2025, which was held from 18th to 20th February in the IACTEC building in the Science and Technology Park at Las Mantecas (Tenerife). The aim of this event was to give information about the coming observation cycle of ALMA ( Atacama Large Millimetre/Submillimetre Array ) and to provide an overview of the data base of the telescope and its observing tools. In addition the scientific results of more than 10 years of observations were presented, and the future perspectives offered with the implementation of
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  • Gran Telescopio Canarias (GTC or Grantecan) at the Roque de los Muchachos Observatory on La Palma
    The Solar System research group at the Instituto de Astrofísica de Canarias (IAC) is participating in the international programme to keep a closet track of asteroid 2024 YR4. The aim is to determine its orbit with the highest possible precision before it stops being observable by ground based and satellite telescopes in April, and so improving our value of the probability that it will impact the Earth in 2032. In this context several telescopes of the Canary Observatories of the IAC are playing an outstanding role in this observing campaign: The Gran Telescopio Canarias (GTC) at the Roque de
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  • El equipo de IACTEC Espacio presenta sus proyectos en el foro internacional SSSIF
    El equipo de IACTEC-Espacio , la división del Instituto de Astrofísica de Canarias (IAC) dedicada al desarrollo de tecnología espacial, participa esta semana como expositor en el Small Satellites & Services International Forum (SSSIF) 2025, celebrado en Málaga, consolidando su posición como referente en el sector espacial español. El evento, clave para la industria de pequeños satélites, está sirviendo de plataforma para presentar proyectos innovadores y establecer colaboraciones estratégicas en especial sobre los proyectos DRAGO, los instrumentos canarios con capacidad de detectar imágenes
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  • Este año se celebra el Año Internacional de la Ciencia y Tecnología Cuántica
    El Instituto de Astrofísica de Canarias (IAC) colabora con la Real Sociedad de Amigos del País de Tenerife para celebrar los 100 años de Progreso Cuántico con un ciclo de conferencias que se inauguran este jueves 20 de febrero a las 19:00 horas con la charla ‘Cuando el Universo deje de fabricar estrellas’, impartida por la astrofísica y subdirectora del IAC Eva Villaver Sobrino. Este ciclo se enmarca dentro de las actividades organizadas con motivo del Año Internacional de la Ciencia y Tecnología Cuántica dentro del Seminario Permanente de Ciencias y Humanidades Blas Cabrera que cuenta con
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  • The 3D structure of the atmosphere of the exoplanet Tylos. Credit: ESO/M. Kornmesser
    An international team, in which the Instituto de Astrofísica de Canarias participates, has succeeded in mapping for the first time the three-dimensional structure of the atmosphere of an exoplanet, that is a planet beyond the Solar System. This research, published today in Nature , has been able to discover very strong winds that carry chemical elements such as iron and titanium, which create certain weather patterns through the planet's atmosphere. This mapping opens the door to more comprehensive and detailed studies of the chemical composition and climate of other planets. Enric Pallé
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  • figura_afm_press
    Ultra-diffuse galaxies, an extreme type of dwarf galaxy, have been the focus of extensive observational and theoretical studies over the past decade. With stellar masses comparable to dwarf galaxies (between 10 7 and 10 9 solar masses) but much larger in size (as defined by their effective radius), they exhibit an extremely low surface brightness. These galaxies display highly diverse properties: some have large dark matter halos, others lack them, and their number of globular clusters varies widely. Studies of their kinematics and stellar populations have shown that these extreme galaxies
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