The stability of the solar system

Details The stability of the solar system The stability of the solar system

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mmsai..52..505r&link_type=abstract

(NATO, Advanced Study Institute on Comparative Study of the Planets, Vulcano, Italy, Sept. 14-25, 1981.) Società Astronomica Ita

Astronomy and Astrophysics

Astronomy

Celestial Mechanics, Dynamic Stability, Many Body Problem, Solar System, Elliptical Orbits, Natural Satellites, Orbit Perturbation, Three Body Problem

Scientific paper

Empirical criteria are presented for the stability of a hierarchical dynamical n-body system and applied to the problem of the long-term stability of hierarchical planetary and satellite systems in the solar system. The criterion of Zare (1976, 1977) for the stability of a three-body system consisting of a binary around which a third body orbits is introduced, and a statistical empirical approach to the question of the stability of hierarchical dynamic systems of three or more bodies is presented which is based on Zare's criterion and involves the establishment of a set of parameters expressing the disturbances to elliptical orbits. When applied to hierarchical three-body subsets of the solar system and satellite systems, the criterion is observed to be well satisfied, with certain exceptions including the retrograde satellites of Jupiter.

Affiliated with

Also associated with

No associations

Rating

The stability of the solar system 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 The stability of the solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stability of the solar system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1515508