NASA NTRS · 19810044223
Non-linear stability around the triangular libration points
Abstract
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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Mckenzie, R., Szebehely, V.. 1981-03-01. Non-linear stability around the triangular libration points. https://ntrs.nasa.gov/citations/19810044223
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