Hill stability in a restricted three-body problem

Details Hill stability in a restricted three-body problem Hill stability in a restricted three-body problem

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pazh....2..311k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 2, June 1976, p. 311-314. In Russian.

Astronomy and Astrophysics

Astronomy

Elliptical Orbits, Hill Method, Motion Stability, Three Body Problem, Trajectory Analysis, Circular Orbits, Existence Theorems

Scientific paper

Sufficient conditions are determined for Hill stability and instability
of an isoenergetic family of trajectories in the simplified semiaveraged
elliptical restricted three-body problem proposed by Rein (1938) for
small eccentricities. The existence of motions that are stable in the
circular problem but unstable in Rein's problem is proven.

Affiliated with

Also associated with

No associations

Rating

Hill stability in a 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 Hill stability in a restricted three-body problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hill stability in a restricted three-body problem will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1784988