Stability VS inclination of motions in E3

Details Stability VS inclination of motions in E3 Stability VS inclination of motions in E3

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..41..417h&link_type=abstract

Astrophysics and Space Science, vol. 41, June 1976, p. 417-422.

Astronomy and Astrophysics

Astrophysics

Dynamic Stability, Orbit Calculation, Three Body Problem, Graphs (Charts), Inclination, Tables (Data)

Scientific paper

Five families of three-dimensional doubly symmetric motions are computed after establishing their existence by means of a grid-search technique. It is confirmed that within the same family, orbits of lower inclination with respect to the plane of motion of the primaries are stable, while the critical inclination at which instability occurs varies between families. The maximum inclination at which stable motions of the type presented were found is about 52 deg.

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