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Sizes Matter: The Dust Size Distribution during Planet Formation

CORDIS · observation · Publication date unknown

tions of protoplanetary discs as well as the composition of Solar system bodies. We will use a novel numerical method that allows us to perform these computationally expensive simulations, and employ machine learning to speed up the calculations. This way, we will for the first time be able to build up a complete picture of how dust particles grow into planets and construct a comprehensive model of planet formation.

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recordType
award
status
SIGNED
region
EU
value
2314680
unit
EUR

Evidence & attribution

European Commission, CORDIS Horizon Europe project dataset. Metadata adapted.

License: CORDIS reuse policy

First collected: 2026-09-20T00:21:03.701Z. This is not the publication date.