The positions of secular resonance surfaces

Details The positions of secular resonance surfaces The positions of secular resonance surfaces

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...46..390w&link_type=abstract

Icarus, vol. 46, June 1981, p. 390-399.

Physics

69

Orbital Elements, Planetary Surfaces, Resonance, Secular Variations, Solar Orbits, Solar System, Asteroids, Graphs (Charts), Mars (Planet), Asteroids, Surface, Resonance, Axis, Eccentricity, Inclination, Planets, Secular Variations, Perturbations, Procedure, Orbits, Data, Distribution, Asteroid Belt, Mars Crossers, Earth Crossers, Motion, Planetesimals, Mapping

Scientific paper

The surfaces for the three strongest secular resonances have been located as a function of proper semimajor axis, eccentricity, and inclination for semimajor axes between 1.25 and 3.5 AU. The results are presented graphically. The nu5 resonance only occurs at high inclinations (approximately greater than 23 deg). The nu6 resonance passes through both the main belt and Mars-crossing space. The nu16 resonance starts near the inner edge of the belt and, at low inclinations at least, folds around a portion of the Mars-crossing space until it runs nearly parallel with the earth-crossing boundary.

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