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24 papers · 2 filters
Formation of moon systems around giant planets: Capture and ablation of planetesimals as foundation for a pebble accretion scenario
Thomas Ronnet, Anders Johansen
The four major satellites of Jupiter, known as the Galilean moons, and Saturn's most massive satellite, Titan, are believed to have formed in a predominantly gaseous circum-planeta…
Resilient habitability of nearby exoplanet systems
Giorgi Kokaia, Melvyn B. Davies, Alexander J. Mustill
We investigate the possibility of finding Earth-like planets in the habitable zone of 34 nearby FGK-dwarfs, each known to host one giant planet exterior to their habitable zone det…
The Kepler-11 system: evolution of the stellar high-energy emission and {initial planetary} atmospheric mass fractions
D. Kubyshkina, L. Fossati, A. J. Mustill +8
The atmospheres of close-in planets are strongly influenced by mass loss driven by the high-energy (X-ray and extreme ultraviolet, EUV) irradiation of the host star, particularly d…
Exploring the conditions for forming cold gas giants through planetesimal accretion
Anders Johansen, Bertram Bitsch
The formation of cold gas giants similar to Jupiter and Saturn in orbit and mass is a great challenge for planetesimal-driven core accretion models because the core growth rates fa…
On the inclinations of the Jupiter Trojans
Simona Pirani, Anders Johansen, Alexander J. Mustill
Jupiter Trojans are are characterized by dark photometric colors, high inclinations and an asymmetry in number of bodies between the two swarms. Different models have been proposed…
A giant exoplanet orbiting a very low-mass star challenges planet formation models
J. C. Morales, A. J. Mustill, I. Ribas +179
Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreeme…