The first image of a new gaseous component in a planetary nebula.
False color image of the planetary nebula NGC 6778. In blue, the emission associated with weak lines of ion O++ recombination, taken with the OSIRIS tunable filter blue instrument in the GTC. In green, emission of the same ion in the excited lines by coll
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Jorge García Rojas: jogarcia_ext [at] iac.es (jogarcia_ext[at]iac[dot]es)
The PLATO (PLAnetary Transits and Oscillations of Stars) space mission, led by the European Space Agency (ESA), has recently completed one of the most delicate phases of its development: the integration of its main components, the 26 scientific cameras and the service module that houses all the instrument's acquisition, processing, and control electronics. This stage, carried out at the facilities of the aerospace company OHB in Germany, marks a fundamental step toward the launch scheduled for December 2026 from French Guiana aboard an Ariane 6 rocket. “Almost eight years after ESA gave the
El Instituto de Astrofísica de Canarias (IAC), a través de su departamento IACTEC-Espacio, celebra hoy la System Requirements Review (SRR) de la misión IACSAT-1, un hito clave que marca la finalización de la fase B1 del proyecto y consolida todos los requisitos técnicos, científicos y programáticos necesarios para avanzar hacia el diseño preliminar del satélite. IACSAT-1 es la primera misión liderada íntegramente por el IAC dedicada a la observación astronómica desde el espacio. Se trata de un proyecto desarrollado por IACTEC-Espacio, con un equipo científico dirigido por el Prof. Rafael
The new infrared spectrograph NIRPS, built with the participation of the Instituto de Astrofísica de Canarias (IAC) and installed on the 3.6-metre telescope at ESO’s La Silla Observatory in Chile, has achieved its first scientific results, with four articles published today in the journal Astronomy & Astrophysics and one more accepted for publication. The data confirm its ability to detect Earth-like planets in the infrared for the first time with a precision better than one metre per second. One of the papers, led by IAC researcher Alejandro Suárez Mascareño, confirms the presence of a