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OBrien_2007_Icarus_191_434_Primordial_Excitation_Clearing_Asteroid_Belt.pdf
Preview of "The primordial excitation and clearing of the asteroid belt—Revisited"
🔗 Source: boulder.swri.edu
📊 Size: 926 KB
📄 Pages: 19 pages
⬇️ Downloads: 86

Summary

The asteroid belt's primordial excitation and clearing are revisited, assuming Jupiter and Saturn had initially circular orbits as predicted by the Nice Model. Simulations of two scenarios are performed: sweeping secular resonances driven by solar nebula depletion, and planetary embryos embedded in the asteroid belt. The first scenario is found to be insufficient for dynamical excitation and mass depletion, while the second scenario can lead to comparable excitation and radial mixing, but requires a secondary depletion event to explain the current mass of the main belt.

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Description

The asteroid belt's primordial excitation and clearing are revisited, assuming Jupiter and Saturn had initially circular orbits as predicted by the Nice Model.

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  • File Format: PDF
  • File Size: 926 KB
  • Pages: 19
  • Language: EN
  • Total Downloads: 86
  • Last Updated: 1 week ago

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