Secular resonances in the primitive solar nebula

Details Secular resonances in the primitive solar nebula Secular resonances in the primitive solar nebula

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cemda..52...57l&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 52, no. 1, 1991, p. 57-78.

Astronomy and Astrophysics

Astronomy

10

Asteroid Belts, Orbital Elements, Orbital Resonances (Celestial Mechanics), Secular Variations, Solar Orbits, Solar System Evolution, Equations Of Motion, Gravitational Effects, Long Term Effects, Solar Planetary Interactions

Scientific paper

The objective of the study was to investigate whether the secular resonances nu6 and nu16 could explain the relatively high eccentricities and inclinations of the asteroid belt. A simple model of secular resonance, eccentricity dependent for nu6 and inclination-dependent for nu16, is written. The effect of the dissipation of the primitive solar nebula is considered, and nebula models are presented and used in the eccentricity dependent and inclination-dependent cases. The dissipation process is then analyzed, starting with an initial moderate surface density up to the actual situation corresponding to a zero density in the nebula.

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