Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration

Details Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mvsfa..29...71g&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 29, Sept.-Oct. 1988, p. 71-75. In Russian

Astronomy and Astrophysics

Astronomy

Asteroids, Celestial Mechanics, Orbit Perturbation, Solar Orbits, Jupiter (Planet), Numerical Integration, Orbit Calculation, Three Body Problem

Scientific paper

Results of a previous qualitative analysis of the motion of asteroids near the 2:1 commensurability with Jupiter are compared with results of the numerical integration of the equations of the plane version of the circular restricted three-body problem. Steady-state solutions are examined. It is concluded that the comparison demonstrates the correctness of the analytical model chosen.

Affiliated with

Also associated with

No associations

Rating

Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration 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 Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Motion of asteroids near 2:1 commensurability - Comparison of an analytical model with results of numerical integration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1599872