Computer Science
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phdt.........5t&link_type=abstract
Ph.D. Thesis Texas Univ., Austin.
Computer Science
Deposition, Jupiter (Planet), Orbital Resonances (Celestial Mechanics), Solar System, Stellar Evolution, Celestial Mechanics, Excitation, Resonance
Scientific paper
The solar system, in its early evolution, is thought to have consisted of an accretion disk around a growing central protostar. The accretion disk from which the planets ultimately formed can play a significant role in the processes of planetary and solar formation. As well as leading, by thermalization of orbital motions in the disk, to bipolar flows in the T Tauri stage of stellar evolution, the disk can influence the course of planetary accumulation. By virtue of its essentially solar composition, Jupiter was formed before the accretion disk was removed. This first formed planet then gravitationally imposed a harmonic structure on the planetesimal swarm through its commensurability resonances. Accelerated growth of planetesimals in orbital resonance with Jupiter resulted in runaway growth producing planetary embryos. These embryos accelerated growth at their own resonances in a process that propagation inward and outward forming a resonant configuration of embryos.
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