Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.254..151p&link_type=abstract
Astrophysics and Space Science, Volume 254, Issue 1, pp.151-153
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
The intervals of the mass parameter (µ) values for possible stability of the basic families of 3D periodic orbits in the restricted three-body problem determined elsewhere are now extended into regions of theµ - q 1 parameter space of the photogravitational restricted three-body problem, where q 1 is the radiation factor of m 1 and it is assumed that m 2 does not radiate. Several 3D periodic orbits corresponding to these regions are computed and tested for stability and seven regions, corresponding to the vertical-critical orbits l1v, l'1v, l6v, m1v, m2v and i1v, survive this stability test, emerging as the regions allowing the simplest types of stable low inclination 3D motion of the infinitesimal particle.
Markellos V. V.
Papadakis K. E.
Perdios E. A.
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