Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.182..313r&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 182, no. 2, Aug. 1991, p. 313-336.
Astronomy and Astrophysics
Astrophysics
7
Lagrangian Equilibrium Points, Orbital Mechanics, Three Body Problem, Equations Of Motion, Gravitational Effects, Orbit Calculation
Scientific paper
In a binary system with both bodies being luminous, the inner collinear equilibrium point L1 becomes stable for values of the mass ratio and radiation pressure parameters in a certain region. The kind of periodic motions around L1 is examined in this case. Second-order parametric expansions are given and the families of periodic orbits generated from L1 are numerically determined for several sets of values of the parameters. Short- and long-period solutions are identified showing a similarity in the character of periodicity with that around L4. It is also found that the finite periodic solutions in the vicinity of L1 are stable.
Perdios E.
Ragos Omiros
Zagouras C. G.
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