CORDIS Project
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This project investigates the chemical composition of gas and ice in the inner regions of protoplanetary disks around young stars using data from the James Webb Space Telescope. It aims to understand the formation of exoplanets by analyzing the relationships between chemical inventory, dust traps, and the presence of y…
The heavy elements (C, O, N) in exoplanetary atmospheres result from accretion of gas and impacts of icy pebbles and planetesimals in disks around young stars.
The gas and dust, in turn, originate from the collapsing cloud that formed the star plus disk, with icy grains growing, settling and drifting in radially to the planet-forming zones.
The inner disk (0.1-10 au) is a key region in planet formation, yet its physical and chemical structure is still poorly constrained observationally.
The next…
UNIVERSITEIT LEIDEN
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