publication . Other literature type . Preprint . Article . 2010

Modeling the Formation of Giant Planet Cores. I. Evaluating Key Processes

Harold F. Levison; Edward Thommes; Martin J. Duncan;
  • Published: 01 Apr 2010
  • Publisher: IOP Publishing
One of the most challenging problems we face in our understanding of planet formation is how Jupiter and Saturn could have formed before the the solar nebula dispersed. The most popular model of giant planet formation is the so-called 'core accretion' model. In this model a large planetary embryo formed first, mainly by two-body accretion. This is then followed by a period of inflow of nebular gas directly onto the growing planet. The core accretion model has an Achilles heel, namely the very first step. We have undertaken the most comprehensive study of this process to date. In this study we numerically integrate the orbits of a number of planetary embryos embe...
free text keywords: Astrophysics - Earth and Planetary Astrophysics, Space and Planetary Science, Astronomy and Astrophysics, Astronomy, Fragmentation (computing), Accretion (meteorology), Physics, Primary atmosphere, Formation and evolution of the Solar System, Giant planet, Planet, Astrophysics, Planetesimal, Planetary migration
Funded by
NSF| The Formation of the Giant Planet Cores
  • Funder: National Science Foundation (NSF)
  • Project Code: 0708775
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
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