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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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An international team of scientists, with participation by researchers at the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL) have found a barred spiral galaxy, similar to the Milky Way, in the early universe, when it was only 15% as old as it is now. The galaxy, ceers-2112, is the most distant barred spiral observed, and its existence poses a challege to the current model of formation and evolution of galaxies. The discovery, made with the James Webb Space Telescope (JWST) is published in the journal Nature. In astrophysics studying the structure of galaxiesAdvertised on
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Tras cuatro años de actividades, el proyecto Interreg EELabs llega a su fin y, como broche final, la noche del 14 de diciembre, a partir de las 22:30 UT (hora local en Canarias), retransmitirá la lluvia de meteoros de las Gemínidas a través del canal sky-live.tv desde el Observatorio del Teide (Tenerife) y El Anillo (Extremadura). Las llamadas “estrellas fugaces” son en realidad pequeñas partículas de polvo de distintos tamaños (entre fracciones de milímetros hasta centímetros de diámetro) que van dejando los cometas -o asteroides- a lo largo de sus órbitas alrededor del Sol. La nube deAdvertised on