JUICE and planet Jupiter
Contributions to MAJIS with ASIMUT-ALVL
BIRA-IASB is assessing the capabilities of MAJIS’ visible and near-infrared (VIS-NIR) channel for the study of Jupiter’s atmosphere.
Snapshot of a GEM-Mars simulation of ozone
GEM-Mars model explores fundamental Mars chemistry problem
Using BIRA-IASB's Mars climate model GEM-Mars, a wide range of processes were explored that can contribute to solving the puzzle.
Surface Venus
Spectacular increase in the D/H ratio in Venus’ atmosphere
Unanticipated increase in the abundances of two variants of water molecules – H2O and HDO – along with their ratio in the Venus mesosphere.