![Diseño artístico de la súper-Tierra GJ 625 b y su estrella, GJ625 (Gliese 625). Crédito: Gabriel Pérez, SMM (IAC). Diseño artístico de la súper-Tierra GJ 625 b y su estrella, GJ625 (Gliese 625). Crédito: Gabriel Pérez, SMM (IAC).](/sites/default/files/styles/crop_square_2_2_to_320px/public/images/gallery/news/prensa1207_2610.jpg?itok=QCb-VTQ-)
An international team led by researchers from the IAC, using the radial velocity method, have discovered a possibly rocky planet at the edge of the habitable zone of a red dwarf star. Only a few dozen planets of this kind are known and its detection was made possible with the HARPS-N spectrograph on the Telescopio Nazionale Galileo (TNG) at the Roque de Los Muchachos Observatory, La Palma.
Advertised on