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• W2566778829 abstract "Nealley moves on an orbit of low eccentricity with a mean motion that is slightly larger than the 2/1 value of resonance. This orbit and some related fictitious orbits are studied by numerical integrations of the four-body problem Sun-Jupiter-Saturn-asteroid over an interval of 110000 yr. The author's experience on related cases of resonance allows a study of the variation of suitably defined orbital parameters. The long-term evolution of the orbits is compared with earlier predictions. Some of the librating orbits are temporarily captured in a secondary resonance that refers to three-dimensional motion and is demonstrated by a special example." @default.
• W2566778829 created "2017-01-06" @default.
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• W2566778829 date "1993-01-01" @default.
• W2566778829 modified "2023-09-23" @default.
• W2566778829 title "LOW-ECCENTRICITY MOTION OF ASTEROIDS NEAR THE 2/1" @default.
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