The "Fundación Galileo Galilei - INAF, Fundación Canaria" (FGG) is a Spanish no-profit institution constituted by "INAF", the Italian Institute of Astrophysics.
The FGG's aim is to promote the astrophysical research, as foreseen in the international agreement of May 26, 1979 ("Acuerdo de Cooperación en Materia de Astrofísica, B.O.E. Núm.161, 6 Jul 1979"), by managing and running the Telescopio Nazionale Galileo (TNG), a 3.58m optical/infrared telescope located in the Island of San Miguel de La Palma, together with its scientific, technical and administrative facilities.
Latest news

Young Astronomers at the Telescopio Nazionale Galileo: III Edition
The Ministry of Education and Merit (MIM), in collaboration with Società Astronomica Italiana (SAIt), Istituto Nazionale di Astrofisica (INAF), and Telescopio Nazionale Galileo (TNG), announced the Third Edition of the National Competition “Giovani Astronomi al Telescopio Nazionale Galileo”. The competition aims to promote and enhance students scientific and technological skills by offering opportunities for growth, teamwork, and exploration of the wonders of the Universe.

Characterization of the outer substellar companion around HD 72659 using HARPS-N and Gaia
An Italian research team has precisely characterized the mass and orbital parameters of HD 72659 c, an exoplanet located in the so-called “brown dwarf desert”, by combining data from HARPS-N (High Accuracy Radial velocity Planet Searcher – Northern Hemisphere) installed at the Telescopio Nazionale Galileo (TNG), astrometric measurements from Gaia (ESA), direct imaging from SPHERE on the Very Large Telescope in Chile and data from literature.

The Telescopio Nazionale Galileo observes with NICS the new interstellar visitor, 3I/ATLAS
The Telescopio Nazionale Galileo (TNG), at the Roque de los Muchachos Observatory (La Palma), did not miss the opportunity to observe the new interstellar object whose discovery was announced on July 1, 2025. This visitor, named 3I/ATLAS, follows in the footsteps of its predecessors, 1I/‘Oumuamua and 2I/Borisov, discovered in 2017 and 2019. Like them, it was detected on its journey toward the Sun, on a hyperbolic orbit at high speed (about 60 km/s) when it was still 3.3 AU from our star (about 495 million km). Shortly after the announcement of its discovery by the ATLAS telescopes, its cometary nature was confirmed thanks to the coma surrounding its bright nucleus.