Literature DB >> 32921836

Simulations of wobble damping in viscoelastic rotators.

Alice C Quillen1, Katelyn J Wagner1,2, Paul Sánchez3.   

Abstract

Using a damped mass-spring model, we simulate wobble of spinning homogeneous viscoelastic ellipsoids undergoing non-principal axis rotation. Energy damping rates are measured for oblate and prolate bodies with different spin rates, spin states, viscoelastic relaxation timescales, axis ratios, and strengths. Analytical models using a quality factor by Breiter et al. (2012) and for the Maxwell rheology by Frouard & Efroimsky (2018) match our numerical measurements of the energy dissipation rate after we modify their predictions for the numerically simulated Kelvin-Voigt rheology. Simulations of nearly spherical but wobbling bodies with hard and soft cores show that the energy dissipation rate is more sensitive to the material properties in the core than near the surface.

Entities:  

Keywords:  asteroids; dynamical evolution and stability; general planets and satellites; minor planets

Year:  2019        PMID: 32921836      PMCID: PMC7485121          DOI: 10.1093/mnras/stz422

Source DB:  PubMed          Journal:  Mon Not R Astron Soc        ISSN: 0035-8711            Impact factor:   5.287


  2 in total

1.  Pressure wave propagation in a shaken granular bed.

Authors:  Stephen R Hostler; Christopher E Brennen
Journal:  Phys Rev E Stat Nonlin Soft Matter Phys       Date:  2005-09-21

2.  A brief visit from a red and extremely elongated interstellar asteroid.

Authors:  Karen J Meech; Robert Weryk; Marco Micheli; Jan T Kleyna; Olivier R Hainaut; Robert Jedicke; Richard J Wainscoat; Kenneth C Chambers; Jacqueline V Keane; Andreea Petric; Larry Denneau; Eugene Magnier; Travis Berger; Mark E Huber; Heather Flewelling; Chris Waters; Eva Schunova-Lilly; Serge Chastel
Journal:  Nature       Date:  2017-11-20       Impact factor: 49.962

  2 in total

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