Equivalence between simple multilayered and homogeneous laboratory-based rheological models in planetary science
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2023-05-17
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Oxford University PressCitation
Yeva Gevorgyan, Isamu Matsuyama, Clodoaldo Ragazzo, Equivalence between simple multilayered and homogeneous laboratory-based rheological models in planetary science, Monthly Notices of the Royal Astronomical Society, Volume 523, Issue 2, August 2023, Pages 1822–1831, https://doi.org/10.1093/mnras/stad1496Rights
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The goal of this work is to investigate under which circumstances the tidal response of a stratified body can be approximated by that of a homogeneous body. We show that any multilayered planet model can be approximated by a homogeneous body, with the same dissipation of tidal energy as a function of the excitation frequency, as long as the rheology of the homogeneous model is sufficiently complex. Moreover we provide two straightforward methods for finding the parameters of the homogeneous rheology that would exhibit the same tidal response as the layered body. These results highlight the fact that the two models cannot be distinguished from each other only by the measurement of the second degree tidal Love number and quality factor, and that we do not need the complexity of the multilayer planet model in order to estimate its tidal dissipation. The methodology promises a great simplification of the treatment of multilayered bodies in numerical simulations because the treatment of a homogeneous body – even with a complex rheological model – can be computationally better handled than that of a multilayered planet. © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.Note
Immediate accessISSN
0035-8711Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1093/mnras/stad1496