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Research led by the Instituto de Astrofísica de Canarias (IAC) has discovered that, in binary systems, stars that evolve into red giants change the way they rotate with their companions, making their orbits more circular. The result was achieved after studying nearly 1000 solar-like oscillating stars in binary systems, the greatest yield to date of such objects. For their identification, the third Gaia Data Release (Gaia-DR3) and NASA Kepler and TESS catalogs have been explored. The study has been published in the journal Astronomy and Astrophysics and has been selected as the most recentAdvertised on -
The President of the Cabildo of La Palma, Sergio Rodríguez inaugurated this morning the International Conference LSST@Europe 6 which has brought together over 140 people from over twenty countries in the field of astrophysical research. In the oficial inauguration there was also participation by the Director of the Instituto de Astrofísica de Canarias (IAC), Valentín Martínez Pillet, the director of the LSST constructive project Zeljko Ivezic and the president of the international organizing committee Mireia Montes Quiles. Sergio Rodríguez noted the importance of this type of scientificAdvertised on -
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