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.

Displaying 7 - 12 of 2859
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  • Carlos Blanco, director de estrategia de SENSIA en su visita al IAC junto al responsable de Instrumentación, Marcos Reyes; y el jefe de departamento de Óptica del IAC, José Luis Rasilla.
    El Instituto de Astrofísica de Canarias y la empresa tecnológica han firmado un protocolo general de actuación para el desarrollo conjunto de instrumentación avanzada en los rangos MWIR y LWIR . El Instituto de Astrofísica de Canarias (IAC) y la empresa de alta tecnología de imagen infrarroja SENSIA Solutions, S.L. (SENSIA) han formalizado este viernes, 20 de marzo de 2026, un Protocolo General de Actuación con el objetivo de establecer un marco estratégico de colaboración científica y tecnológica . La colaboración se ha formalizado con la firma de este protocolo por parte de Valentín
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  • Begoña García Lorenzo, Verónica Martín y Silvia Granja en el programa / IAC
    El Instituto de Astrofísica de Canarias (IAC) emite este jueves, 9 de abril de 2026, a las 22:30 horas, una nueva edición de su programa radiofónico “Soñando Estrellas”, que se emite a través de la radio pública, La Radio Canaria . Bajo la conducción de Verónica Martín, este espacio de 30 minutos de duración rinde homenaje en su nombre al libro del fundador del IAC, Francisco Sánchez, y busca acercar a la audiencia la labor pionera de los más de 400 profesionales que trabajan en las sedes de Tenerife y La Palma, gestionando los Observatorios de Canarias. En esta edición, el programa cuenta
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  • Javalambre Auxiliary Survey Telescope, at the Javalambre Astrophysical Observatory (Teruel, Spain)
    A team of scientists, including astrophysicist Carlos Hernández Monteagudo from the University of La Laguna (ULL) and the Canary Islands Institute of Astrophysics (IAC), has compiled one of the most comprehensive catalogues of small bodies in the Solar System, based on photometric observations made from Earth. The study, published in Monthly Notices of the Royal Astronomical Society, compiles data on 6,579 asteroids, comets and irregular satellites, mainly from the main belt located between Mars and Jupiter, opening up new possibilities for studying their composition and rotation. The
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  • Serge Haroche, winner of the 2012 Nobel Prize in Physics, and F. Duncan Haldane, winner of the 2016 Nobel Prize in Physics
    On 9 and 10 April, the Canary Islands Institute of Astrophysics (IAC) will welcome two distinguished physicists: Serge Haroche, winner of the 2012 Nobel Prize in Physics, and F. Duncan Haldane, winner of the 2016 Nobel Prize in Physics. Both scientists have been invited by the IAC to take part in the 18th Congress of Physics Students (COEFIS), organised by students from the University of La Laguna, and will each give a lecture in the IAC Lecture Hall from 10.30 am. On Thursday 9 April, the IAC will welcome Professor Haroche, and on Friday 10 April it will be Professor Haldane’s turn. In both
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  • nanojet
    An international team of researchers led by the Instituto de Astrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL), has unveiled a breakthrough explanation for the origin of tiny, jet-like plasma ejections in the solar atmosphere, known as “nanojets.” These elusive events which are recently discovered by the NASA’s solar telescopes are thought to play an important role in heating and sustaining the solar corona at temperatures above one million Kelvin. Why Study Nanojets? For decades, solar physicists have been puzzled by the so-called “coronal heating problem.” While the Sun
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  • Artistic illustration showing warm and hot ionised winds and the warm molecular gas rotating within a galaxy hosting an AGN. Credit: Gabriel Pérez Díaz (IAC).
    Astronomers have long asked: what causes galaxies to stop forming new stars? What causes them to transition from blue, star-forming systems to red and dead galaxies? One mechanism often favoured by cosmological simulations that attempt to reproduce the observed Universe is the energy released when matter falls onto the supermassive black holes at the centres of galaxies. When these black holes enter active phases – known as active galactic nuclei (AGN) – the energy they release can heat and expel gas away in the form of winds, preventing the gas from cooling and forming new stars
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