Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion

Details Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion Mass ratios of three bodies for stable low-inclination three-dimensional periodic motion

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.192..291p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 192, no. 2, June 1992, p. 291-297.

Statistics

Computation

3

Celestial Mechanics, Computational Astrophysics, Mass Ratios, Three Body Problem, Three Dimensional Motion, Orbital Mechanics, Periodic Variations

Scientific paper

In Markellos et al. (1981) 21 basic vertical critical periodic orbits of the restricted three-body problem were computed for the entire range of the mass parameter mu = m2/(m1 + m2), and 12 intervals on the mu-axis were determined for which the 120 vertical critical orbits are horizontally stable. In the present paper, these intervals are extended into regions of the mu - m3 (m3 = 1 - m1 - m2) parameter space of the general three-body problem.

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