The measure of Titan’s incredibly large migration speed away from Saturn reveals that tidal dissipation depends on the orbital frequency. This new paradigm has many implications for the internal structure of Saturn and the history of its satellite system.
References
Lainey, V. et al. Nat. Astron. https://doi.org/10.1038/s41550-020-1120-5 (2020).
Fuller, J., Luan, J. & Quataert, E. Mon. Not. R. Astron. Soc. 458, 3867–3879 (2016).
Lainey, V. et al. Astrophys. J. 752, 14 (2012).
Charnoz, S. et al. Icarus 212, 535–550 (2011).
Ćuk, M., Dones, L. & Nesvorny, D. Astrophys. J. 820, 97 (2016).
Crida, A. & Charnoz, S. Science 338, 1196–1199 (2012).
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Crida, A. Large tides alert on Saturn. Nat Astron 4, 1024–1025 (2020). https://doi.org/10.1038/s41550-020-1109-0
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DOI: https://doi.org/10.1038/s41550-020-1109-0
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