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- W3100834467 endingPage "11" @default.
- W3100834467 startingPage "11" @default.
- W3100834467 abstract "Super-Earths with orbital periods less than 100 days are extremely abundant around Sun-like stars. It is unlikely that these planets formed at their current locations. Rather, they likely formed at large distances from the star and subsequently migrated inward. Here we use N-body simulations to study the effect of super-Earths on the accretion of rocky planets. In our simulations, one or more super-Earths migrates inward through a disk of planetary embryos and planetesimals embedded in a gaseous disk. We tested a wide range of migration speeds and configurations. Fast-migrating super-Earths ($tau_{mig} sim$0.01-0.1 Myr) only have a modest effect on the protoplanetary embryos and planetesimals. Sufficient material survives to form rocky, Earth-like planets on orbits exterior to the super-Earths'. In contrast, slowly migrating super-Earths shepherd rocky material interior to their orbits and strongly deplete the terrestrial planet-forming zone. In this situation any Earth-sized planets in the habitable zone are extremely volatile-rich and are therefore probably not Earth-like." @default.
- W3100834467 created "2020-11-23" @default.
- W3100834467 creator A5036459292 @default.
- W3100834467 creator A5045650283 @default.
- W3100834467 creator A5047892872 @default.
- W3100834467 date "2014-09-18" @default.
- W3100834467 modified "2023-10-05" @default.
- W3100834467 title "TERRESTRIAL PLANET FORMATION IN THE PRESENCE OF MIGRATING SUPER-EARTHS" @default.
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