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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&apos;s ice shell with hydrothermal seafloor activity. Previous numerical simulations showed that convection in Enceladus&apos;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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10500 - Earth and related environmental sciences

Result continuities

  • Project

  • 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

  • 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