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How drifting and evaporating pebbles shape giant planets II: Volatiles and refractories in atmospheres
Aaron David Schneider, Bertram Bitsch
Upcoming studies of extrasolar gas giants will give precise insights into the composition of planetary atmospheres with the ultimate goal to link it to the formation history of the…
Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line
Bertram Bitsch, Sean N. Raymond, Lars A. Buchhave +3
In the pebble accretion scenario, the pebbles that form planets drift inward from the outer disk regions, carrying water ice with them. At the water ice line, the water ice on the…
How drifting and evaporating pebbles shape giant planets I: Heavy element content and atmospheric C/O
Aaron David Schneider, Bertram Bitsch
Recent observations of extrasolar gas giants suggest super-stellar C/O ratios in planetary atmospheres, while interior models of observed extrasolar giant planets additionally sugg…