Non-linear stability around the triangular libration points

Details Non-linear stability around the triangular libration points Non-linear stability around the triangular libration points

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cemec..23..223m&link_type=abstract

Celestial Mechanics, vol. 23, Mar. 1981, p. 223-229. Research supported by the University of Texas, NASA, and NATO.

Mathematics

15

Earth-Moon System, Lagrangian Equilibrium Points, Librational Motion, Motion Stability, Three Body Problem, Celestial Mechanics, Nonlinear Systems, Partitions (Mathematics)

Scientific paper

The configuration space around the triangular libration points in the
Earth-Moon system is partitioned according to the stability of the
motion. The regions around L4 and L5 are established where particles
placed with zero initial velocity will librate. The complexity of the
partitioning is revealed.

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