Terrestrial planets form best in simulations with an inner planetesimal ring near 0.5 au plus an outer source near 1.5 to 2 au, with outward Type-I migration.
E., & Betts, H.\ 2012, , Instability-driven Dynamical Evolution Model of a Primordially Five-planet Outer Solar System, 744, 1, L3
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Terrestrial Planet Formation from Two Source Reservoirs
Terrestrial planets form best in simulations with an inner planetesimal ring near 0.5 au plus an outer source near 1.5 to 2 au, with outward Type-I migration.