Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..56..153s&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 56, no. 1-2, p. 153-162.
Astronomy and Astrophysics
Astronomy
1
Asteroids, Four Body Problem, Libration, Orbital Resonances (Celestial Mechanics), Solar Orbits, Jupiter (Planet), Saturn (Planet), Sun
Scientific paper
(903) 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 110,000 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.
No associations
LandOfFree
Low-eccentricity motion of asteroids near the 2/1 Jovian resonance does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Low-eccentricity motion of asteroids near the 2/1 Jovian resonance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-eccentricity motion of asteroids near the 2/1 Jovian resonance will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1739549