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Timing of water plume eruptions on Enceladus explained by interior viscosity structure

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10314657" target="_blank" >RIV/00216208:11320/15:10314657 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1038/NGEO2475" target="_blank" >http://dx.doi.org/10.1038/NGEO2475</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1038/NGEO2475" target="_blank" >10.1038/NGEO2475</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Timing of water plume eruptions on Enceladus explained by interior viscosity structure

  • Original language description

    At the south pole of Saturn's icy moon Enceladus, eruptions of water vapour and ice emanate from warm tectonic ridges(1-4). Observations in the infrared(5) and visible(6) spectra have shown an orbital modulation of the plume brightness, which suggests that the eruption activity is influenced by tidal forces. However, the observed activity seems to be delayed by several hours with respect to predictions based on simple tidal models(6,7). Here we simulate the viscoelastic tidal response of Enceladus witha full three-dimensional numerical model(8,9) and show that the delay in eruption activity may be a natural consequence of the viscosity structure in the south-polar region and the size of the putative subsurface ocean. By systematically comparing simulations of variations in normal stress along faults with plume brightness data, we show that the observed activity is reproduced for two classes of interior models with contrasting thermal histories: a low-viscosity convective region above

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    DE - Earth magnetism, geodesy, geography

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA14-04145S" target="_blank" >GA14-04145S: Internal evolution of close-in terrestrial exoplanets</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2015

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Nature Geoscience

  • ISSN

    1752-0894

  • e-ISSN

  • Volume of the periodical

    8

  • Issue of the periodical within the volume

    8

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    4

  • Pages from-to

    601-604

  • UT code for WoS article

    000358735500011

  • EID of the result in the Scopus database

    2-s2.0-84938587376