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An international team has just discovered a wide variety of carbonaceous gases in the disc surrounding a young very low-mass star, hence constraining the building blocks for planets forming therein.

This study, in which scientists from the PSILab at ULiège took part, opens up a new path for studying exoplanets that can be observed by direct imaging. 

This is an essential discovery in which ULiège researchers played a key role, and which offers clues as to the habitability of rocky planets around other stars.

Located 374 light years away from Earth, HD169142 b has been confirmed as a protoplanet by a team of researchers from the University of Liège and Monash University.

ULiège researchers are involved in the analysis and comparison of data obtained by the James Webb Space Telescope (JWST) and ground-based telescopes.

New capabilities developed by an international team of astronomers make it possible to directly image planets that could potentially harbour life in the habitable zone of a nearby system.

The instrument that will equip ESO's Extremely Large Telescope and for which ULiège will supply a series of coronographs has successfully passed its preliminary design review.