On the formation of terrestrial planets in hot-Jupiter systems

@article{Fogg2007OnTF,
  title={On the formation of terrestrial planets in hot-Jupiter systems},
  author={M. Fogg and R. Nelson},
  journal={Astronomy and Astrophysics},
  year={2007},
  volume={461},
  pages={1195-1208}
}
  • M. Fogg, R. Nelson
  • Published 2007
  • Physics
  • Astronomy and Astrophysics
  • Context. There are numerous extrasolar giant planets which orbit close to their central stars. These “hot-Jupiters” probably formed in the outer, cooler regions of their protoplanetary disks, and migrated inward to ∼ 0.1 AU. Since these giant planets must have migrated through their inner systems at an early time, it is uncertain whether they could have formed or retained terrestrial planets. Aims. We present a series of calculations aimed at examining how an inner system of planetesimals… CONTINUE READING
    Debris disks as signposts of terrestrial planet formation
    • 118
    • Open Access
    TOWARD CHEMICAL CONSTRAINTS ON HOT JUPITER MIGRATION
    • 97
    • Open Access
    A Decreased Probability of Habitable Planet Formation around Low-Mass Stars
    • 137
    • Open Access
    Observable consequences of planet formation models in systems with close-in terrestrial planets
    • 111
    • Open Access
    WASP-47: A Hot Jupiter System with Two Additional Planets Discovered by K2
    • 131
    • Open Access
    The effect of type I migration on the formation of terrestrial planets in hot-Jupiter systems
    • 48
    • Open Access

    References

    Publications referenced by this paper.
    SHOWING 1-10 OF 54 REFERENCES