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The Onset of Chaos in Permanently Deformed Binaries from Spin–Orbit and Spin–Spin Coupling

Seligman, Darryl and Batygin, Konstantin (2021) The Onset of Chaos in Permanently Deformed Binaries from Spin–Orbit and Spin–Spin Coupling. Astrophysical Journal, 913 (1). Art. No. 31. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20210524-164633973

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Abstract

Permanently deformed objects in binary systems can experience complex rotation evolution, arising from the extensively studied effect of spin–orbit coupling as well as more nuanced dynamics arising from spin–spin interactions. The ability of an object to sustain an aspheroidal shape largely determines whether or not it will exhibit nontrivial rotational behavior. In this work, we adopt a simplified model of a gravitationally interacting primary and satellite pair, where each body's quadrupole moment is approximated by two diametrically opposed point masses. After calculating the net gravitational torque on the satellite from the primary, as well as the associated equations of motion, we employ a Hamiltonian formalism that allows for a perturbative treatment of the spin–orbit and retrograde and prograde spin–spin coupling states. By analyzing the resonances individually and collectively, we determine the criteria for resonance overlap and the onset of chaos, as a function of orbital and geometric properties of the binary. We extend the 2D planar geometry to calculate the obliquity evolution. This calculation indicates that satellites in spin–spin resonances undergo precession when inclined out of the plane, but they do not tumble. We apply our resonance overlap criteria to the contact binary system (216) Kleopatra, and find that its satellites, Cleoselene and Alexhelios, may plausibly be exhibiting chaotic rotational dynamics from the overlap of the spin–orbit and retrograde spin–spin resonances. While this model is, by construction, generalizable to any binary system, it will be particularly useful for studies of small bodies in the Solar System, whose irregular shapes make them ideal candidates for exotic rotational states.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/abf248DOIArticle
https://arxiv.org/abs/2103.12484arXivDiscussion Paper
https://github.com/DSeligman/Onset_Chaos_SpinSpinOrbitRelated Itemcode & Mathematica notebook
ORCID:
AuthorORCID
Seligman, Darryl0000-0002-0726-6480
Batygin, Konstantin0000-0002-7094-7908
Additional Information:© 2021. The American Astronomical Society. Received 2020 September 16; revised 2021 March 22; accepted 2021 March 24; published 2021 May 21. We thank Kaitlin Kratter, Michele Bannister, Robert Jedicke, Edwin Kite, Cristobal Petrovich, and Mahdi Jafari Nadoushan for useful conversations. We also thank the anonymous referee for a constructive and insightful report, and for encouraging us to explore the effects of obliquity, which greatly strengthened our manuscript. K.B. is grateful to Caltech, and the David and Lucile Packard Foundation for their generous support. All of the code that generated the figures in this paper, as well as a mathematica notebook containing the derivations of the relevant equations, may be found at https://github.com/DSeligman/Onset_Chaos_SpinSpinOrbit.
Funders:
Funding AgencyGrant Number
CaltechUNSPECIFIED
David and Lucile Packard FoundationUNSPECIFIED
Subject Keywords:Asteroids; Astrodynamics; Trans-Neptunian objects
Issue or Number:1
Classification Code:Unified Astronomy Thesaurus concepts: Asteroids (72); Astrodynamics (76); Trans-Neptunian objects (1705)
Record Number:CaltechAUTHORS:20210524-164633973
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210524-164633973
Official Citation:Darryl Seligman and Konstantin Batygin 2021 ApJ 913 31
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:109245
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:25 May 2021 15:18
Last Modified:25 May 2021 15:18

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