The Distribution in Eccentricity and Inclination, as a Function of the Semi-major Axis of Asteroids

Details The Distribution in Eccentricity and Inclination, as a Function of the Semi-major Axis of Asteroids The Distribution in Eccentricity and Inclination, as a Function of the Semi-major Axis of Asteroids

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003dda....34.0616v&link_type=abstract

American Astronomical Society, DDA meeting #34, #06.16; Bulletin of the American Astronomical Society, Vol. 35, p.1040

Astronomy and Astrophysics

Astronomy

Scientific paper

We use a running window on the AsDys catalogue of asteroids and create groups of varying proper semi-major axis values. We calculate, for each such group, the distribution of asteroids with respect to proper eccentricity and inclination. We plot the distribution parameters as a function of the semi-major. We see that the graphs are related to the resonant structure in the region of the main Kirkwood gaps.

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