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2020AJ....160..139T - Astron. J., 160, 139-139 (2020/September-0)

Secular resonances in nonrestricted hierarchical triple systems.

TAN P., HOU X., LIAO X., WANG W. and TANG J.

Abstract (from CDS):

In this paper, the averaged Hamiltonian of a nonrestricted hierarchical triple system truncated at the third order is investigated. First, each secular resonant term is studied. For the well-studied secular quadrupole theory, it is analytically reformulated in a different manner in our work. The resonance width is numerically determined and displayed on the sqrt(1-e12)-sqrt(1-e22) plane (also denoted as the ∼e1-∼e2 plane). In terms of the octupole terms, we show that for a near-planar configuration of the system, considerable variations of both the eccentricities of the inner and outer orbits can be generated by a single resonant term. The resonance width for every secular resonant angle from the octupole terms is also numerically determined and displayed on the ∼e1-∼e2 plane. The results show that an orbit flip with a near-perpendicular initial mutual inclination is possible for each secular resonance. By displaying the resonance widths of different resonant terms on the same ∼e1-∼e2 plane, we intuitively show the overlap of different secular resonances. Then, the full averaged Hamiltonian with both quadrupole and octupole terms is investigated using the Poincare surface of section, with a special focus on the orbit flip. For the cases we exploited, we find that the near-planar flip of the inner orbit can be either regular or chaotic while the outer orbit flip is generally chaotic.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Orbital resonances - Three-body problem - Exoplanet dynamics - Celestial mechanics

Simbad objects: 4

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