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The resonance overlap and Hill stability criteria revisited

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Abstract

We review the orbital stability of the planar circular restricted three-body problem in the case of massless particles initially located between both massive bodies. We present new estimates of the resonance overlap criterion and the Hill stability limit and compare their predictions with detailed dynamical maps constructed with N-body simulations. We show that the boundary between (Hill) stable and unstable orbits is not smooth but characterized by a rich structure generated by the superposition of different mean-motion resonances, which does not allow for a simple global expression for stability. We propose that, for a given perturbing mass \(m_1\) and initial eccentricity e, there are actually two critical values of the semimajor axis. All values \(a < a_\mathrm{Hill}\) are Hill-stable, while all values \(a > a_\mathrm{unstable}\) are unstable in the Hill sense. The first limit is given by the Hill-stability criterion and is a function of the eccentricity. The second limit is virtually insensitive to the initial eccentricity and closely resembles a new resonance overlap condition (for circular orbits) developed in terms of the intersection between first- and second-order mean-motion resonances.

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References

  • Beaugé, C.: Asymmetric librations in exterior resonances. Celest. Mech. Dyn. Astron. 60, 225–248 (1994)

    Article  MATH  ADS  Google Scholar 

  • Bodman, E.H.L., Quillen, A.C.: Stability boundaries for resonant migrating planet pairs. Mon. Not. R. Astron. Soc. Icarus Nature 440, 1753–1762 (2014)

    Article  ADS  Google Scholar 

  • Brouwer, D., Clemence, G.M.: Methods of Celestial Mechanics. Academic Press, New York (1961)

    Google Scholar 

  • Chirikov, B.V.: A universal instability of many-dimensional oscillator systems. Phys. Rep. 52, 263–379 (1979)

    Article  MathSciNet  ADS  Google Scholar 

  • Deck, K.M., Payne, M., Holman, M.J.: First-order resonance overlap and the stability of close two-planet systems. Astrophys. J. 774, 129–141 (2013)

    Article  ADS  Google Scholar 

  • Duncan, M., Quinn, T., Tremaine, S.: The long-term evolution of orbits in the solar system. A mapping approach. Icarus 82, 402–418 (1989)

    Article  ADS  Google Scholar 

  • Dvorak, R., Pilat-Lohinger, E., Schwarz, R., Freistetter, F.: Extrasolar Trojan planets close to habitable zones. Astron. Astrophys. 426, L37–L40 (2004)

    Article  ADS  Google Scholar 

  • Ferraz-Mello, S.: Expansion of the disturbing force-function for the study of high-eccentricity librations. Astron. Astrophys. 183, 208 (1987)

    Google Scholar 

  • Ferraz-Mello, S.: The high-eccentricity libration of the Hildas. Astron. J 96, 400–408 (1988)

    Article  ADS  Google Scholar 

  • Ferraz-Mello, S.: Canonical Perturbation Theories: Degenerate Systems and Resonance. Springer, New York (2007)

    Book  Google Scholar 

  • Gladman, B.: Dynamics of systems of two close planets. Icarus 106, 247–263 (1993)

    Article  ADS  Google Scholar 

  • Henrard, J., Lemaître, A.: A second fundamental model for resonance. Celest. Mech. Dyn. Astron. 30, 197–218 (1983)

    Article  MATH  Google Scholar 

  • Hori, G.: Theory of general perturbations with unspecified canonical variables. Publ. Astron. Soc. Jpn. 18, 287–295 (1966)

    ADS  Google Scholar 

  • Malhotra, R.: Orbital resonances and chaos in the solar system. In ASP Conf. Ser. 149, Solar System Formation and Evolution, ed. D. Lazzaro, R. Vieira Martins, S. Ferraz-Mello, J. Fernandez, ans C. Beaugé (San Francisco, CA: ASP), 37 (1998)

  • Moons, M., Morbidelli, A.: The main mean motion commensurabilities in the planar circular and elliptic problem. Celest. Mech. Dyn. Astron 57, 99–108 (1993)

    Article  MATH  MathSciNet  ADS  Google Scholar 

  • Morbidelli, A.: Modern Celestial Mechanics. Cambridge University Press, UK (1999)

  • Murray, C.D., Dermott, S.F.: Solar Systems Dynamics. Cambridge University Press, Cambridge (1999)

    Google Scholar 

  • Mustill, A.J., Wyatt, M.C.: Dependence of a planets’ chaotic zone on particle eccentricity: the shape of debris disc inner edges. Mon. Not. R. Astron. Soc. Icarus Nature 419, 3074–3070 (2012)

    Article  ADS  Google Scholar 

  • Quillem, A.C., Faber, P.: Chaotic zone boundary for low free eccentricity particles near an eccentric planet. Mon. Not. R. Astron. Soc. Icarus Nature 373, 1245–1250 (2006)

    Article  ADS  Google Scholar 

  • Seidov, Z.F.: The Roche problem: some analytics. Astrophys. J. 603, 283–284 (2004)

    Article  ADS  Google Scholar 

  • Walker, G.H., Ford, J.: Amplitude instability and ergodic behavior for conservative nonlinear oscillator systems. Phys. Rev. 188, 416 (1969)

    Article  MathSciNet  ADS  Google Scholar 

  • Wisdom, J.: The resonance overlap criterion and the onset of stochastic behavior in the restricted three-body problem. Astron. J 85, 1122–1133 (1980)

    Article  ADS  Google Scholar 

Download references

Acknowledgments

This work was supported by research grants from Secretaría de Ciencia y Tecnología/Universidad Nacional de Córdoba (Secyt/UNC), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), and Fondo para la Investigación Científica y Tecnológica (FONCyT). in full. The authors wish to thank Instituto de Astronomía Teórica y Experimental (IATE) and the UNC for extensive use of their computing facilities and to Pablo Benitez-Llambay for his assistance in developing the graphical routines. Finally, we would also like to express our gratitude to an anonymous referee for stimulating discussions that helped improve this paper.

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Ramos, X.S., Correa-Otto, J.A. & Beaugé, C. The resonance overlap and Hill stability criteria revisited. Celest Mech Dyn Astr 123, 453–479 (2015). https://doi.org/10.1007/s10569-015-9646-z

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  • DOI: https://doi.org/10.1007/s10569-015-9646-z

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