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Dynamical friction in spherical systems

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Tremaine, S., Weinberg, M. D.·1984·Monthly Notices of the Royal Astronomical Society

Abstract

We investigate dynamical friction on a test object (such as a bar or satellite) which rotates or revolves through a spherical stellar system. We find that frictional effects arise entirely from near-resonant stars and we derive an analog to Chandrasekhar's dynamical friction formula which applies to spherical systems. We show that a formula of this type is valid so long as the angular speed of the test object changes sufficiently rapidly. If the angular speed is slowly changing two new effects appear: a reversible dynamical feedback which can stabilize or destabilize the rotation speed, and permanent capture of near-resonant stars into librating orbits. We discuss orbital decay of satellites in the light of these results.

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Metadata

Authors
Tremaine, S., & Weinberg, M. D.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1984-08-01
Volume
209
Issue
4
Pages
729-757
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2052986856
Cited by
313
References
0
FWCI
2.61
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Dynamical friction in spherical systems. https://app.cochat.ai/papers/10.1093/mnras/209.4.729
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Tremaine, S., & Weinberg, M. D. (1984). Dynamical friction in spherical systems. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/209.4.729

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