Early terrestrial planet formation by torque-driven convergent migration of planetary embryos

@article{Bro2021EarlyTP,
  title={Early terrestrial planet formation by torque-driven convergent migration of planetary embryos},
  author={Miroslav Bro{\vz} and Ondřej Chrenko and David Nesvorn{\'y} and Nicolas Dauphas},
  journal={Nature Astronomy},
  year={2021}
}
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 is that the terrestrial planet system formed later (30–200 Myr after the dispersal of the gas disk) by giant collisions of tens of lunar- to Mars-sized protoplanets3,4. Here we propose, instead, that the terrestrial planets of the Solar System formed earlier by the gas-driven… Expand
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