How drifting and evaporating pebbles shape giant planets – i. heavy element content and atmospheric c/o

HIGHLIGHTS

  • who: Schneider Aaron David and Bitsch Bertram from the Max-Planck-Institut für Astronomie, Königstuhl, Heidelberg, Germany have published the research: How drifting and evaporating pebbles shape giant planets - I. Heavy element content and atmospheric C/O, in the Journal: (JOURNAL)
  • what: The authors investigate in this work the inward drift and evaporation of volatile-rich pebbles influences the atmospheric C/O ratio and heavy element content of giant planets growing by pebble and gas accretion. The authors focus thus on a disk model that includes the growth and drift of pebbles (Birnstiel . . .

     

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