An international team of astronomers, including researchers from the Instituto de Astrofísica de Canarias (IAC), the University of Liège and collaborators in UK, Chile, the USA, and Europe, has discovered a transiting giant planet orbiting the smallest known star to host such a companion — a finding that defies current theories of planet formation. The host star, TOI-6894 , is a red dwarf with only 20% the mass of the Sun , typical of the most common stars in our galaxy. Until now, such low-mass stars were not thought capable of forming or retaining giant planets. But as published today in

At the present time ground-based observatories have a wide range of instruments which can study the solar surface in the visible and infrared ranges. But it is not possible to combine these observations with those in the near ultraviolet, which cover the wavelength range from 200 to 400 nanometres, nor to maintain them for long periods due to the turbulence in the Earth’s atmosphere. In this context, the Sunrise III mission, in which the Instituto de Astrofísica de Canarias (IAC) is collaborating, “ has become the first observatory to obtain spectropolarimetric data simultaneously in the

The Instituto de Astrofísica de Canarias (IAC) has successfully completed the integration of the scientific detector into the FRIDA (inFRared Imager and Dissector for Adaptive Optics) instrument, an integra-field camera and spectrograph designed to work with the adaptive optics system of the Gran Telescopio Canarias (GTC or Grantecan), the world's largest optical and infrared telescope, located at the Roque de los Muchachos Observatory in La Palma. The integration was carried out in the laboratories of the National Autonomous University of Mexico (UNAM) in Mexico City by a team from the IAC