At the end of September, the International Astronomical Union officially approved the naming of two asteroids after our two emeritus colleagues, Mária Kun and Géza Kovács.
An international research team used the ALMA antenna array to capture the most detailed image ever of 24 debris disks, which may help better understand the turbulent adolescence of planetary systems.
A Hungarian-led international research team has discovered that the birthplace of Tattoine-like planetary systems is undergoing unprecedented variability.
An international research team including Ágnes Kóspál from Konkoly Observatory has created the first detailed map of the molecular layers within a planet-forming disk – the flattened cloud of gas and dust surrounding a young star, where planets are born.
The Ritchey-Chrétien-Coudé (RCC) telescope at the Piszkéstető Mountain Station, with a 102 cm primary mirror and an effective focal length of 13.5 meters, is currently the largest telescope in Hungary.
The Mauve small satellite has been recently successfully launched and will study the activity of stars across the Milky Way. Hungarian space-industry partners played a key role in building the spacecraft, while Hungarian astronomers will be deeply involve
Researchers have for the first time identified possible radio signatures of a coronal mass ejection (CME) originating from another star with the LOFAR array, helping us to understand the interaction between stellar activity and exoplanetary environments.
More than a hundred astronomers and astrophysicists gathered at the Assembly of Hungarian Astronomers, held at the Academy headquarters, for a one-day conference.