Early terrestrial planet formation by torque-driven convergent migration of planetary embryos
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DOI: 10.1038/s41550-021-01383-3
Abstract: The massive cores of the giant planets are thought to have formed in a gas disk by the accretion of pebble-sized particles whose accretional cross-section was enhanced by aerodynamic gas drag1,2. A commonly held view… read more here.
Keywords: convergent migration; terrestrial planet; gas; disk ... See more keywords