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
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Czech description
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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
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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
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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