Computer Science
Scientific paper
May 1968
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968saosr.278.....g&link_type=abstract
SAO Special Report #278 (1968)
Computer Science
3
Scientific paper
The secular characteristics of the motion of asteroids in resonance with Jupiter are analyzed. The Trojan group is given special attention by a description of these characteristics in a complete qualitative and quantitative manner. Except for collision orbits, the eccentricity and inclination of the asteroid can take any value. The shortperiod perturbations caused by Jupiter are averaged by a nonlinear numerical application of von Zeipel's method. Elimination of the resonant argument is carried, in a semianalytical way, to an approximation of the order of the mass of Jupiter. The final system, with one degree of freedom, is represented by isoenergetic curves in the phase plane (ω, e). The various steps of solution allow a description of the general features of motion for a very long time.
No associations
LandOfFree
Secular Motion of Resonant Asteroids 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 Secular Motion of Resonant Asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Secular Motion of Resonant Asteroids will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-835053