A Dynamical Survey of Inner Solar System Asteroids

Details A Dynamical Survey of Inner Solar System Asteroids A Dynamical Survey of Inner Solar System Asteroids

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998dda....30.0801m&link_type=abstract

American Astronomical Society, DDA meeting #30, #08.01; Bulletin of the American Astronomical Society, Vol. 30, p.1144

Astronomy and Astrophysics

Astronomy

Scientific paper

Results from a numerical integration survey of all known inner solar system asteroids (a <= aMars) are presented. A number of asteroids appear to be in or very near high order mean motion resonances with Venus, Earth, or Mars. Most of these resonance associations are short-lived, with the asteroids wandering in and out of resonance on timescales of several thousand years or less.

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