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Retrograde resonance in the planar three-body problem

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Abstract

We continue the investigation of the dynamics of retrograde resonances initiated in Morais and Giuppone (Mon Notices R Astron Soc 424:52–64, doi:10.1111/j.1365-2966.2012.21151.x, 2012). After deriving a procedure to deduce the retrograde resonance terms from the standard expansion of the three-dimensional disturbing function, we concentrate on the planar problem and construct surfaces of section that explore phase-space in the vicinity of the main retrograde resonances (2/-1, 1/-1 and 1/-2). In the case of the 1/-1 resonance for which the standard expansion is not adequate to describe the dynamics, we develop a semi-analytic model based on numerical averaging of the unexpanded disturbing function, and show that the predicted libration modes are in agreement with the behavior seen in the surfaces of section.


Publication:

Celestial Mechanics and Dynamical Astronomy

Pub Date:
December 2013
DOI:

10.1007/s10569-013-9519-2

10.48550/arXiv.1305.0016

arXiv:
arXiv:1305.0016
Bibcode:
2013CeMDA.117..405M
Keywords:
  • Resonance;
  • Three-body problem;
  • Surface of section;
  • Co-orbital resonance;
  • Astrophysics - Earth and Planetary Astrophysics
E-Print:
Celestial Mechanics and Dynamical Astronomy, in press