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Thanks to a stellar occultation, astronomers were able to observe and determine the characteristics of 2002 GZ32, a centaur with a diameter of almost 400 kilometers on its major axis. Known for more than forty years, we have little information about this group of icy objects orbiting the Sun between the orbits of Jupiter and Neptune

Although similar studies have been carried out in other countries, this is the only one that has obtained results thanks to the combination of observations from the satellite and from the ground

 

 

Researchers from the Institute of Astrophysics of Andalusia (IAA-CSIC) are leading an ambitious radio observation project that shows that extrasolar planets can be detected with radio telescopes

 

This December, due to the alignment of the Earth, Jupiter and Saturn, we will be able to see the giant planets of the Solar System very close in the sky. Many activities are being organized to enjoy the event

 

 

As part of the European Horizon 2020 program, the RoadMap project (Role and impact of dust and clouds in the Martian atmosphere) has just started

 

 

Observations with the Hubble Space Telescope show how this young nebula has lost its brightness and changed shape in just two decades

 

 

MHONGOOSE, a legacy project of the MeerKAT radiointerferometer, South African precursor to the Square Kilometer Array, produces its first results. They have been obtained in its preparatory phase, thus anticipating the window that will open to the understanding of the formation and evolution of galaxies

 

The mission, developed by the European Space Agency (ESA) and scheduled for launch in 2029, has moved from the study phase to the implementation phase, which involves selecting an industrial contractor to build the spacecraft. The Institute de Astrophysics of Andalusia (IAA-CSIC) participates in Ariel through two of its scientific working groups

The Institute of Astrophysics of Andalusia (IAA-CSIC) participates in the project, coordinated by the Center for the Study of Physics of the Cosmos of Aragon (CEFCA)

 

 

The identification of a source producing very short duration radio bursts in our own galaxy, the Milky Way, is presented in three articles in the journal Nature. Studies suggest that a magnetar, a neutron star with a very intense magnetic field, would be behind this phenomenon

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