Stationary solutions in simplified resonance cases of the restricted three-body problem

Details Stationary solutions in simplified resonance cases of the restricted three-body problem Stationary solutions in simplified resonance cases of the restricted three-body problem

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cemec..21..157b&link_type=abstract

(Conference on Mathematical Methods in Celestial Mechanics, 6th, Oberwolfach, West Germany, Aug. 14-19, 1978.) Celestial Mechani

Astronomy and Astrophysics

Astronomy

6

Asteroids, Jupiter (Planet), Resonance, Solar System, Three Body Problem, Astrodynamics, Motion Stability, Orbital Mechanics, Periodic Functions

Scientific paper

In the planar elliptic problem sun-Jupiter-massless body the resonances of mean motion 3/2, 2/1, 7/3, and 1/3 are considered. Short-period effects are eliminated by Schubart's averaging method. Applying a minimization technique, stationary solutions can be found in the given resonance cases. Some of these solutions are well-known as periodic solutions in the rigorous (i.e., unaveraged) restricted problem. The construction in a numerical way of a linearized theory of motion around a stationary solution is illustrated, and results are presented.

Affiliated with

Also associated with

No associations

Rating

Stationary solutions in simplified resonance cases of the restricted three-body problem 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 Stationary solutions in simplified resonance cases of the restricted three-body problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stationary solutions in simplified resonance cases of the restricted three-body problem will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620831