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