Desde la cumbre de Tenerife hasta el país del Sol naciente pasando por la capital administrativa de la Unión Europea. La exposición “100 Lunas cuadradas”, compuesta de nueve espectaculares imágenes del cielo, viaja durante el mes de abril a Tokio, donde se inaugurará el próximo día 5 en la sede del Instituto Cervantes en Japón para luego trasladarse a la Universidad Femenina de Ochanomizu. También podrá visitarse en la sede del Parlamento Europeo en Bruselas, acompañada de la maqueta del European Solar Telescope (EST), el que será el mayor telescopio solar de Europa; será inaugurada el

Researchers at the Instituto de Astrofísica de Canarias (IAC) and the University of Cambridge have detected lithium in a primitive star in our galaxy. The observations were made at the VLT, at the Paranal Observatory of ESO in Chile.

A new project from the Instituto de Astrofísica de Canarias (IAC) has been chosed to be carried out in the Science Lab in the seventh edition of the Global Azure Bootcamp. This annual event occurs simultaneously in over 100 countries, and brings together professionals and experts in Internet technology, and in the Microsoft Cloud.

Antonia Varela, Marisa Tejedor, Carolina Martínez and Teresa Giráldez are given distinctions in an institutional act commemorating Women’s Day.

The first results on the analysis of the images of Bennu obtained using OCAMS, OVIRS, and OTES instruments on-board NASA’s OSIRIS-REx spacecraft have been published today in a paper on Nature Astronomy, co-authored by four researchers of the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL).

Stars with masses between one and eight times the mass of the Sun evolve along the asymptotic giant branch (AGB) before ending their lives as white dwarfs. It is during this rapid but crucial phase when the stars expand to huge dimensions and cool down, losing a major fraction of their mass due to the strong stellar winds. The low temperature and high density of the winds provide ideal conditions for the condensation of dust grains in their circumstellar envelopes. The dust produced by the stars in their AGB phase and expelled into the interstellar medium is important for the lives of the