Orbits of real and fictitious asteroids studied by numerical integration

Details Orbits of real and fictitious asteroids studied by numerical integration Orbits of real and fictitious asteroids studied by numerical integration

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..104..391s&link_type=abstract

Astronomy and Astrophysics, Suppl. Ser. 104, 391-399

Astronomy and Astrophysics

Astrophysics

Scientific paper

The paper starts with a review of the author's various numerical studies on asteroid orbits, ruled by the violent evolution of the computer technique, and continues with a collection of starting values of orbital elements. This collection supplements the author's numerous papers on orbits at resonances of mean motion with respect to Jupiter. Especially, it refers to work on Trojan-type motion, mainly done together with R. Bien, and to the Hilda and Hecuba cases of resonance. It will allow the extension of intervals covered by numerical integration in interesting cases. The collection contains hitherto unpublished examples of orbits and additional comments. In particular, special remarks and some new results refer to low-eccentricity motion of Hecuba type.

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