A Numerical Method for Determining the Elements of Circumbinary Orbits and Its Application to Circumbinary Planets and the Satellites of Pluto-Charon

Abstract

Planets and satellites orbiting a binary system exist in the solar system and extrasolar planetary systems. Their orbits can be significantly different from Keplerian orbits, if they are close to the binary and the secondary-to-primary mass ratio is high. A proper description of a circumbinary orbit is in terms of the free eccentricity $e_{\mathrm{free}}$ at the epicyclic frequency ${\kappa }_0$, forced eccentricity $e_{\mathrm{forced}}$ at the mean motion $n_0$, and oscillations at higher frequencies forced by the non-axisymmetric components of the binary's potential. We show that accurate numerical values for the amplitudes and frequencies of these terms can be extracted from numerical orbit integrations by applying fast Fourier transformation (FFT) to the cylindrical distance between the circumbinary object and the center of mass of the binary as a function of time. We apply this method to three Kepler circumbinary planets and the satellites of Pluto-Charon. For the satellite Styx of Pluto-Charon, the FFT results for ${\kappa }_0$ and $e_{\mathrm{free}}$ differ significantly from the first-order analytic value and the value reported by Showalter & Hamilton (2015), respectively. We show that the deviation in ${\kappa }_0$ is likely due to the effect of the 3:1 mean-motion resonance and discuss the implications of the lower value for $e_{\mathrm{free}}$.

17 pages, including 9 figures, accepted for publication in AJ

References in corpus (6)

• Kepler-16: A Transiting Circumbinary Planet
• The Transiting Circumbinary Planets Kepler-34 and Kepler-35
• Secular Evolution of Hierarchical Planetary Systems
• Kepler-1647b: the largest and longest-period Kepler transiting circumbinary planet
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Cited by in corpus (7)

• Past and present dynamics of the circumbinary moons in the Pluto-Charon system
• A Dynamical Systems Approach to the Theory of Circumbinary Orbits in the Circular Restricted Problem
• On the Estimation of Circumbinary Orbital Properties
• Orbit determination of the moons of the Pluto-Charon system
• Orbits of the TOI-1338 and TIC-172900988 systems
• Orbital analysis of the Pluto-Charon moon system's mutual interactions and forced frequencies
• A Pluto--Charon Sonata IV. Improved Constraints on the Dynamical Behavior and Masses of the Small Satellites