Secular Resonance Sweeping in a Self-gravitating Planetesimal Disk, with Application to the Kuiper Belt

Details Secular Resonance Sweeping in a Self-gravitating Planetesimal Disk, with Application to the Kuiper Belt Secular Resonance Sweeping in a Self-gravitating Planetesimal Disk, with Application to the Kuiper Belt

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1930h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1930

Physics

2

Scientific paper

Nagasawa and Ida (2000) have shown that scanning secular resonances can
excite large eccentricities and inclinations. We reexamine this
phenomena for a planetesimal disk having mass, and it is shown that such
excitation is muted by wave propagation.

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