Chaotic motion and the Graziani-Black criterion

Details Chaotic motion and the Graziani-Black criterion Chaotic motion and the Graziani-Black criterion

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cemda..54..357s&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 54, no. 4, p. 357-362.

Astronomy and Astrophysics

Astronomy

Chaos, Hill Method, Laplace Equation, Liapunov Functions, Three Body Problem, Gravitational Effects, Planetary Evolution, Poincare Problem, Star Clusters

Scientific paper

Chaotic motion is presented as a fundamental cause for the development of the Laplacian instability described by the Graziani-Black (GB) criterion. While the GB criterion is valid for different sets of finite masses in a general three-body system, a circular planar restricted three-body system is studied here. Poincare surfaces of section and Liapunov characteristic numbers are used to test for the chaotic motion in this system. A simple description of the chaos detection techniques and the GB criterion is provided.

Affiliated with

Also associated with

No associations

Rating

Chaotic motion and the Graziani-Black criterion 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 Chaotic motion and the Graziani-Black criterion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chaotic motion and the Graziani-Black criterion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1113879