CORDIS Project
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This project investigates the formation of planets around young stars by studying the properties of dust in protoplanetary disks. It aims to provide direct observational data on the midplane pebble layer and understand dust growth mechanisms, which are crucial for planet formation.
Exoplanets are frequent around Solar-like stars, as shown by Large Surveys.
They are formed by the growth of dust and accumulation of gas contained in protoplanetary disks surrounding young stars.
To form planets, the classic Core-Accretion scenario is the main framework today, but it appears to be too slow given the short lifetimes of disks.
Theoretical additions to Core-Accretion exist to speed it up.
They all hypothesize that disks contain a massive, dense, and flat layer of pebbles in the mi…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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