Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-28T06:31:43.357Z Has data issue: false hasContentIssue false

A Dynamical Survey of Inner Solar System Asteroids

Published online by Cambridge University Press:  12 April 2016

Marc A. Murison*
Affiliation:
Astronomical Applications Dept., U.S. Naval Observatory, 3450 Massachusetts Ave NW, Washington DCUSA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Results from a numerical integration survey of all 179 currently-known inner solar system asteroids with a ≤ aMars, qaMercury are presented. A surprising number of asteroids are currently in, or very near, mean-motion resonances with Mercury, Venus, Earth, or Mars. Some of the resonance associations are of high order. Most of the resonance associations are relatively short-lived, with the asteroids wandering in and out of resonance on timescales of hundreds to several thousand years.

Type
Extended Abstracts
Copyright
Copyright © Kluwer 1999