Fakultät für Physik und Astronomie
STEPHEN PHILLIPS hostreviews.co.uk / UNSPLASH

How the formation of multiple giant planets can impact their own growth and the structure of their protoplanetary disk

Camille Bergez , MPIA

Giant planets are partly formed by accretion of the gas present in the protoplanetary disk surrounding them. This process influences the shape of the protoplanetary disk as well as the growth of the giants themselves when considering more than one giant forming at the same time. I will present the results of my hydrodynamical simulations which investigate the evolution of the masses of the planets as a function of time as well as the evolution of the structures present in the protoplanetary disk. I will link these two quantities to observations of protoplanetary disks as well as the distributions of characteristics of the observed exoplanets.

Königstuhl Colloquium
9 Sep 2022, 11:00
Max-Planck-Institut für Astronomie, Level 3 Lecture Hall (301)

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