EPSC Abstracts
Vol. 19, EPSC2026-515, 2026, updated on 02 Jul 2026
https://doi.org/10.5194/epsc2026-515
Europlanet Science Congress 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 08 Sep, 18:00–19:30 (CEST), Display time Tuesday, 08 Sep, 08:30–19:30| Foyer 3, F3.70
Formation and evolution of the circumjovian disk
Kévin Baillié
Kévin Baillié
  • Observatoire de Paris, LTE, PARIS, France (kevin.baillie@obspm.fr)

Adapting the hydrodynamical code PHYVE (designed for protoplanetary disks) to the formation of a proto-Jupiter system, we follow the formation and evolution of the disk surrounding the proto-Jupiter.

This disk is fed by the protoplanetary disk itsself and we follow the circumJovian disk evolution based on environmental parameters inherited from the simulations of Baillié et al., 2019.

We follow the evolution of the surface mass density profile, but also the disk composition and geometry.

We investigate the question of satellite traps, similar to planet traps in protoplanetary disks.

How to cite: Baillié, K.: Formation and evolution of the circumjovian disk, Europlanet Science Congress 2026, The Hague, The Netherlands, 7–11 Sep 2026, EPSC2026-515, https://doi.org/10.5194/epsc2026-515, 2026.