The Secular Variations in the Restricted Problem's Sixth-Order Theory and Stability - an Explicit Numerical Approach
Abstract
In this paper, we develop and implement an explicit numerical technique for studying equilibrium solutions concerning the secular variations in the restricted problem of three bodies, and their stability. In this implementation, we employ a sixth-order theory for the secular terms.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- May 1990
- DOI:
- 10.1007/BF00642069
- Bibcode:
- 1990Ap&SS.167..139F
- Keywords:
-
- Computational Astrophysics;
- Numerical Stability;
- Secular Variations;
- Three Body Problem;
- Dynamic Stability;
- Equations Of Motion;
- Astrophysics