Computation of weak stability boundaries: Sun-Jupiter system

Details Computation of weak stability boundaries: Sun-Jupiter system Computation of weak stability boundaries: Sun-Jupiter system

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cemda.105....3t&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, Volume 105, Issue 1-3, pp. 3-17

Astronomy and Astrophysics

Astronomy

5

Restricted Three-Body Problem, Weak Stability Boundary, Ballistic Capture, Invariant Manifolds, Lyapunov Orbits, Stable Sets

Scientific paper

We compute the weak stability boundary in the planar circular restricted three-body problem starting from the algorithmic definition, and its generalization by García and Gómez. In addition, we consider a new set of primaries, Sun-Jupiter, to replace the case of Earth-Moon considered in previous studies. Numerical enhancements are described and compared to previous methods. This includes defining the equations of motion in polar coordinates and a modified numerical scheme for the derivation of both stable sets and their boundaries. These enhancements decrease the computational time. New results are obtained by considering the Sun-Jupiter case which we compare to the Earth-Moon case.

Affiliated with

Also associated with

No associations

Rating

Computation of weak stability boundaries: Sun-Jupiter 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 Computation of weak stability boundaries: Sun-Jupiter system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Computation of weak stability boundaries: Sun-Jupiter system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1263281