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In Situ Formation of Icy Moons of Uranus and Neptune
J. Szulágyi, M. Cilibrasi, L. Mayer
Satellites of giant planets thought to form in gaseous circumplanetary disks (CPDs) during the late planet-formation phase, but it was unknown so far whether smaller mass planets,…
The formation of Jupiter by hybrid pebble-planetesimal accretion
Yann Alibert, Julia Venturini, Ravit Helled +8
The standard model for giant planet formation is based on the accretion of solids by a growing planetary embryo, followed by rapid gas accretion once the planet exceeds a so-called…
A sub-grid model for the growth of dust particles in hydrodynamical simulations of protoplanetary disks
Tomas Tamfal, Joanna Drazkowska, Lucio Mayer +1
We present the first 2D hydrodynamical finite volume simulations in which dust is fully coupled with the gas, including its back-reaction onto it, and at the same time the dust siz…
On the diversity in mass and orbital radius of giant planets formed via disk instability
Simon Müller, Ravit Helled, Lucio Mayer
We present a semi-analytical population synthesis model of protoplanetary clumps formed by disk instability at radial distances of 80 - 120 AU. Various clump density profiles, init…
Dust-vortex instability in the regime of well-coupled grains
Clément Surville, Lucio Mayer
We present a novel study of dust-vortex evolution in global two-fluid disk simulations to find out if evolution toward high dust-to-gas ratios can occur in a regime of well-coupled…
Satellites Form Fast & Late: a Population Synthesis for the Galilean Moons
M. Cilibrasi, J. Szulágyi, L. Mayer +3
The satellites of Jupiter are thought to form in a circumplanetary disc. Here we address their formation and orbital evolution with a population synthesis approach, by varying the…