Seafloor hydrothermal control over ocean dynamics in Enceladus
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10508376" target="_blank" >RIV/00216208:11320/25:10508376 - isvavai.cz</a>
Result on the web
<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=LE4ybL1l3B" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=LE4ybL1l3B</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1038/s41550-025-02490-1" target="_blank" >10.1038/s41550-025-02490-1</a>
Alternative languages
Result language
angličtina
Original language name
Seafloor hydrothermal control over ocean dynamics in Enceladus
Original language description
Cassini observations imply that there is a global ocean underneath Enceladus's ice shell with hydrothermal seafloor activity. Previous numerical simulations showed that convection in Enceladus's unconsolidated core may produce a heterogeneous seafloor heat flux and hydrothermal activity, potentially explaining the South Polar ice thinning and plume activity. How the ocean transports heat and hydrothermal products is the missing piece of the Enceladus puzzle. Here we perform three-dimensional numerical simulations of the ocean dynamics using a very heterogeneous bottom boundary condition from three-dimensional hydrothermal core simulations. We gradually increase the heterogeneity amplitude of the bottom heat flux until its peak-to-peak value reaches 60 times its mean. We show that a strong zonal flow diminishes low-latitude heat transfer, whereas the heat flux remains efficient in polar regions, which explains the ice shell variations derived from gravity and topography observations. Using passive tracers, we predict rising times of hours to weeks, which are compatible with previous predictions. Our simulations confirm that a strong heterogeneous seafloor heat flux concentrates upwellings at the South Pole, thus efficiently transporting organic matter from hydrothermal vents to erupting plumes.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10500 - Earth and related environmental sciences
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Nature Astronomy
ISSN
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e-ISSN
2397-3366
Volume of the periodical
9
Issue of the periodical within the volume
5
Country of publishing house
GB - UNITED KINGDOM
Number of pages
8
Pages from-to
650-657
UT code for WoS article
001443012700001
EID of the result in the Scopus database
2-s2.0-105000040232