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 1 - 6 of 479
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  • Dark galaxies in the Local Group
    The Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna are leading an international study on dark galaxies. ULL PhD student Guacimara García Bethencourt, together with her thesis supervisors Arianna Di Cintio and Sébastien Comerón, both lecturers in the Department of Astrophysics at the ULL and researchers at the IAC, presents a pioneering study in Astronomy & Astrophysics on one of the most intriguing objects in modern astrophysics: dark galaxies, systems rich in gas and dark matter but incapable of forming stars, and therefore invisible to traditional telescopes
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  • Día de Nuestra de Ciencia 2026
    El Instituto de Astrofísica de Canarias reúne a su personal investigador y técnico para presentar los resultados más destacados del último año y abordar los retos científicos de la próxima década El Instituto de Astrofísica de Canarias (IAC) ha celebrado hoy la XVII edición del “Día de Nuestra Ciencia”, un encuentro anual de carácter interno que ha reunido a personal investigador, técnico y de apoyo a la investigación en la sede de IACTEC, en La Laguna. La jornada se ha consolidado como un espacio para compartir los avances científicos y tecnológicos más relevantes desarrollados en el último
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  • Roberta Zanin, responsable científica del CTAO; Valentín Martínez Pillet, director del IAC; y Juan Ramón Felipe San Antonio, vicepresidente del Cabildo de La Palma.
    El Cherenkov Telescope Array Observatory (CTAO) , el futuro observatorio de astronomía de rayos gamma más grande y potente del mundo, continúa su avance constante hacia su fase de operaciones iniciales. En una rueda de prensa conjunta celebrada en Santa Cruz de La Palma, Islas Canarias (España), representantes de la Organización Central del CTAO (CTAO ERIC), la Colaboración LST del CTAO , el Cabildo de La Palma y el Instituto de Astrofísica de Canarias (IAC) se reunieron para destacar el avance del proyecto hacia una ciencia pionera. Este progreso está marcado por la próxima inauguración de
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  • Milky Way-like galaxies from the BEARD project
    The international BEARD project, led from the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL), has used data from several telescopes at the Roque de los Muchachos Observatory, and computer simulations to explain how galaxies similar to the Milky Way have managed to survive the most violent stages of the history of the Universe. The present model for the evolution of the universe predicts an epoch dominated by important mergers of galaxies some ten thousand million years ago. “It’s a case of violent interactions, in which it is foreseeable that weak structures
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  • Artist's impression of the HD 114082 planetary system
    An international collaboration of astronomers led by the Universidad de La Laguna (ULL) and Instituto de Astrofísica de Canarias (IAC) has identified two intriguing, humongous but light planets orbit ing HD 114082. This star is only 15 million years old, this is, much younger than the Sun (4.6 billion years old) , spin s 15 times faster , has 28% more mass , and is about one thousand degrees hotter and almost four times more luminous. Its planets receive about 200 times more light and heat than Jupiter. The study, which involved separating the faint planetary signal from the stellar one
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  • galaxy_overdensity
    The Universe is not distributed uniformly. Galaxies are arranged in a gigantic cosmic web made of voids, filaments, and galaxy clusters. These filaments act as enormous “cosmic highways” through which matter and galaxies flow toward the densest regions of the Universe. Understanding how these structures influence galaxy evolution is one of the major goals of modern astrophysics. In this work, we analyzed hundreds of thousands of galaxies from the Sloan Digital Sky Survey (SDSS) to study how galaxy density changes around cosmic filaments in the nearby Universe. Our main goal was to determine
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