The secular variations in the restricted problem's sixth-order theory and stability - an explicit numerical approach

Details The secular variations in the restricted problem's sixth-order theory and stability - an explicit numerical approach The secular variations in the restricted problem's sixth-order theory and stability - an explicit numerical approach

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.167..139f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 167, no. 1, May 1990, p. 139-158.

Statistics

Computation

2

Computational Astrophysics, Numerical Stability, Secular Variations, Three Body Problem, Dynamic Stability, Equations Of Motion

Scientific paper

An explicit numerical technique for studying equilibrium solutions
concerning the secular variations in the restricted problem of three
bodies and their stability is developed and implemented. In this
implementation, a sixth-order theory for the secular terms is employed.

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