Hill Stability and Distance Curves for the General Three-Body Problem

Details Hill Stability and Distance Curves for the General Three-Body Problem Hill Stability and Distance Curves for the General Three-Body Problem

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982cemec..26..311m&link_type=abstract

Celestial Mechanics, Volume 26, Issue 3, pp.311-333

Physics

60

Scientific paper

The notion of Hill stability is extended from the circular restricted 3-body problem to the general three-body problem; it is even extended to systems of positive energy and the Hill's curves with their corresponding forbidden zones are generalized. Hill stable systems of negative energy present a hierarchy: they have a close binary that can be neither approached nor disrupted by the third body. This phenomenon becomes particularly clear with the distance curves presentation. The three limiting cases, restricted, planetary and lunar are analysed as well as some real stellar cases.

Affiliated with

Also associated with

No associations

Rating

Hill Stability and Distance Curves for the General 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 Hill Stability and Distance Curves for the General Three-Body Problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hill Stability and Distance Curves for the General Three-Body Problem will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1017279