Orbital resonances in the solar nebula - Strengths and weaknesses

Details Orbital resonances in the solar nebula - Strengths and weaknesses Orbital resonances in the solar nebula - Strengths and weaknesses

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106..264m&link_type=abstract

Icarus, vol. 106, p. 264

Physics

32

Solar Corona, Orbital Resonances (Celestial Mechanics), Protoplanets, Aerodynamic Drag, Eccentricity, Digital Simulation

Scientific paper

Because resonant perturbations from a protoplanet interior to a planetesimal's orbit can counteract both orbital decay and eccentricity damping, the planetesimal can undergo capture in an orbital resonance and its eccentricity can be enhanced to a modestly high equilibrium value. The characteristics of the phenomenon of resonance capture by gas drag are here established in the circular restricted three-body approximation, leading to determinations of the strengths of the equilibrium resonant orbits relative to impulse velocity perturbations.

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