Formation of Gaseous and Rocky Exoplanets

Formation of Gaseous and Rocky Exoplanets

Planetary population synthesis modells are a potentially powerful tool to produce planetary Initial-Mass-Functions, if the underlying physics is well understood. A part of our group aims at using and improving those modells and comparing them to the known planetary populations.

A picture with the one true color-scale.

Members working on this project

PhD project

Accretion shock influence on initial entropy for gaseous planets (PhD project)

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