Cited by 31Astro and Planetary ScienceStellar, planetary, and galactic studiesSpace Satellite Systems and Control

CARE AND FEEDING OF FROGS

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Pan, Margaret, Chiang, Eugene·2012·The Astronomical Journal

Abstract

"Propellers" are features in Saturn's A ring associated with moonlets that open partial gaps. They exhibit non-Keplerian motion (Tiscareno et al.); the longitude residuals of the best-observed propeller, "Blériot," appear consistent with a sinusoid of period ∼4 years. Pan & Chiang proposed that propeller moonlets librate in "frog resonances" with co-orbiting ring material. By analogy with the restricted three-body problem, they treated the co-orbital material as stationary in the rotating frame and neglected non-co-orbital material. Here we use simple numerical experiments to extend the frog model, including feedback due to the gap's motion, and drag associated with the Lindblad disk torques that cause Type I migration. Because the moonlet creates the gap, we expect the gap centroid to track the moonlet, but only after a time delay t delay , the time for a ring particle to travel from conjunction with the moonlet to the end of the gap. We find that frog librations can persist only if t delay exceeds the frog libration period P lib , and if damping from Lindblad torques balances driving from co-orbital torques. If t delay ≪ P lib , then the libration amplitude damps to zero. In the case of Blériot, the frog resonance model can reproduce the observed libration period P lib ≃ 4 yr. However, our simple feedback prescription suggests that Blériot's t delay ∼ 0.01 P lib , which is inconsistent with the observed libration amplitude of 260 km. We urge more accurate treatments of feedback to test the assumptions of our toy models.

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  • The observed non-Keplerian radial motions of propeller moonlets may result from interactions between moonlets and stochastic density fluctuations in the disk or between moonlets and ring particles on loosely bound frog orbits.

    “These motions may result from interactions between moonlets and stochastic density fluctuations in the disk (Crida et al. 2010;Rein & Papaloizou 2010;Pan et al. 2012) or between moonlets and ring particles on loosely bound”

    From MIGRATION OF SMALL MOONS IN SATURN's RINGS (2013) · cites this paper as Pan et al. 2012

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  1. Colwell, J. E., Nicholson, P. D., Tiscareno, M. S., et al. 2009, in Saturn from Cassini-Huygens, ed. M. Dougherty, L. Esposito, & T. Krimigis (Heidelberg: Springer), 375
  2. Cuzzi, J., Clark, R., Filacchione, G., et al. 2009, in Saturn from Cassini-Huygens, ed. M. K. Dougherty, L. W. Esposito, & S. M. Krimigis (Heidelberg: Springer), 459

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Authors
Pan, M., & Chiang, E.
Affiliations
University of California, Berkeley (US)
Corresponding author
Pan, Margaret
Venue
The Astronomical Journal
Published
2011-12-08
Volume
143
Issue
1
Pages
9
ISSN
  • 0004-6256 (ISSN-L)
  • 1538-3881
OpenAlex
W2002945171
Cited by
31
References
13
Citations by year
2019: 1 · 2018: 21 · 2017: 1 · 2013: 2 · 2012: 3
FWCI
1.36
Type
journal article
Language
en
Open access
Locations
  • The Astronomical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Engineering › Aerospace Engineering › Space Satellite Systems and Control
Keywords
ring gaps, Lindblad torque, type I migration, restricted three-body problem

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