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The mission, which will observe the Sun from an unprecedented perspective, will study both solar physics and the influence of the Sun on the interplanetary environment. The Institute de Astrophysics of Andalusia (IAA-CSIC) co-leads SO/PHI, the largest of the ten instruments on board the mission

With a minimum mass of about six times that of the Earth, the planet would revolve around the star at 1.5 times the distance between the Earth and the Sun. This study adds to previous work that points to the existence of a complex planetary system around Proxima Centauri

A survey with an unprecedented resolution of the central regions of our galaxy reveals its full history of star formation, which presents steep ups and downs in star formation. There are indications of a burst of star formation so intense that it caused more than one hundred thousand supernova explosions

The system is composed of two white dwarf stars that revolve around the common centre of mass every twenty minutes, and which are gradually approaching. The work, in which the Institute of Astrophysics of Andalusia (IAA-CSIC) participates, shows that the stars have “flattened out” and have an ellipsoidal shape due to the tidal forces

IAA collaborates in the development of four of the nine instruments on board the mission

Observations with the Kepler satellite allow surface activity to be found in stars where, according to theoretical models, it should not occur. In the sample highlights the star KIC 9716385, which presents, hidden between its pulsations, flares millions of times more intense than the solar ones

MAGIC telescopes, on the island of La Palma, detect photons in the range of teraelectronvolts in a gamma ray explosion (GRB), the product of the death of a very massive star. The detection, which requires contemplating new mechanisms in the energy production of GRBs, provides a fundamental perspective to complete our understanding of these events

Calar Alto Observatory opens a call for new instrumentation projects

An international group of astronomers led by the Instituto de Astrofísica de Andalucía finds a periodic variation in the X-ray emission of the central star of the Eskimo Nebula.

This finding could confirm the hypothesis that there is a multiple system at the centre of the planetary nebula.

The Dark Energy Spectroscopic Instrument (DESI) sees first light. DESI, a project with the participation of the IAA-CSIC, will improve the understanding of the role of dark energy in the history of the expansion of the universe

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