Mass Distribution and Planet Formation in the Solar Nebula

  title={Mass Distribution and Planet Formation in the Solar Nebula},
  author={Steven J. Desch},
  journal={The Astrophysical Journal},
  pages={878 - 893}
  • S. Desch
  • Published 10 December 2007
  • Physics, Geology
  • The Astrophysical Journal
The surface density profile Σ(r) of the solar nebula protoplanetary disk is a fundamental input to all models of disk processes and evolution. Traditionally it is estimated by spreading out the augmented masses of the planets over the annuli in which the planets orbit today, the so-called minimum-mass solar nebula. Doing so implicitly assumes that the planets completely accreted all planetesimals in their feeding zones, but this assumption has not been tested. Indeed, models of the growth of… 


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  • A. Boss
  • Physics, Geology
    The Astrophysical journal
  • 2000
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New numerical simulations of the formation of the giant of the second phase. planets are presented, in which for the first time both the gas and The actual rates at which the giant planets accreted

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Radial Flow of Dust Particles in Accretion Disks

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