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An international team, led by a researcher from the University of Liège (Belgium) affiliated to the Instituto de Astrofísica de Canarias (IAC), has discovered an extraordinarily light planet orbiting a distant star in our galaxy. This discovery, reported today in the journal Nature Astronomy, is a promising key to solving the mystery of how such giant, super-light planets form. The new planet, named WASP-193b, appears to dwarf Jupiter in size, yet it is a fraction of its density. The scientists found that the gas giant is 50 percent bigger than Jupiter, and about a tenth as dense — anAdvertised on
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Research led by the Instituto de Astrofísica de Canarias (IAC) has used an innovative technique based on artificial intelligence to study how stars form in galaxies. By analysing 10 000 nearby galaxies, the team have discovered that most stars are born within their own galaxy. Galactic mergers, while important, are not the main source of new stars. Furthermore, the study reveals that more massive galaxies are more affected by these mergers. These results, published in Nature Astronomy, provide new clues about the complex history of galaxies and their evolution over time. Most galaxies do notAdvertised on
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El embajador de Japón en España, Takahiro Nakamae , visitó esta semana la sede central del Instituto de Astrofísica de Canarias (IAC) y el Observatorio del Teide, junto con Shinji Yamada, cónsul de Japón en Las Palmas de Gran Canaria, junto a personal de su equipo. En la sede central fueron recibidos por Valentín Martínez Pillet, director del IAC; y por el responsable de Instrumentación, Marcos Reyes; y por la jefa de la Unidad de Comunicación y Cultura Científica (UC3), Verónica Martín. En la sede central del IAC conocieron las instalaciones y las principales líneas de investigación delAdvertised on