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Large tides alert on Saturn

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.

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Fig. 1: Titan is receding from Saturn at 11 cm yr–1.

NASA/JPL-Caltech/Space Science Institute.


  1. 1.

    Lainey, V. et al. Nat. Astron. (2020).

  2. 2.

    Fuller, J., Luan, J. & Quataert, E. Mon. Not. R. Astron. Soc. 458, 3867–3879 (2016).

    ADS  Article  Google Scholar 

  3. 3.

    Lainey, V. et al. Astrophys. J. 752, 14 (2012).

    ADS  Article  Google Scholar 

  4. 4.

    Charnoz, S. et al. Icarus 212, 535–550 (2011).

    ADS  Article  Google Scholar 

  5. 5.

    Ćuk, M., Dones, L. & Nesvorny, D. Astrophys. J. 820, 97 (2016).

    ADS  Article  Google Scholar 

  6. 6.

    Crida, A. & Charnoz, S. Science 338, 1196–1199 (2012).

    ADS  Article  Google Scholar 

Download references

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Correspondence to Aurélien Crida.

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Crida, A. Large tides alert on Saturn. Nat Astron 4, 1024–1025 (2020).

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