Quantification of Tides in Giant Planets from Observations Article Swipe
V. Lainey
,
Marco Zannoni
,
Vincent Robert
,
T. Guillot
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1007/s11214-025-01209-y
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1007/s11214-025-01209-y
Quantifying tidal effects on giant planets has recently made significant advances, thanks in particular to the Cassini space probe. During its thirteen-year orbit around Saturn, numerous measurements from different instruments made it possible to characterize fundamental parameters such as Saturn’s Love number k 2 and quality factor Q at different frequencies. In this article, we summarize the various measurements and methods that have allowed to arrive at such a result, as well as the extrapolations that can be deduced for other systems. More generally, the state of the art concerning the four giant planets of the Solar System is presented, as well as the case of exoplanets.
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- en
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- https://doi.org/10.1007/s11214-025-01209-y
- https://link.springer.com/content/pdf/10.1007/s11214-025-01209-y.pdf
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https://openalex.org/W4415106447Canonical identifier for this work in OpenAlex
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https://doi.org/10.1007/s11214-025-01209-yDigital Object Identifier
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Quantification of Tides in Giant Planets from ObservationsWork title
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2025Year of publication
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2025-10-01Full publication date if available
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V. Lainey, Marco Zannoni, Vincent Robert, T. GuillotList of authors in order
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https://doi.org/10.1007/s11214-025-01209-yPublisher landing page
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https://link.springer.com/content/pdf/10.1007/s11214-025-01209-y.pdfDirect link to full text PDF
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hybridOpen access status per OpenAlex
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0Total citation count in OpenAlex
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117Number of works referenced by this work
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