Heat flows through the ice lithosphere of Europa

Some of the geological features on the surface of Europa's ice shell suggest the existence of a brittle lithosphere that in some regions is no more than 2 km thick. The surface heat flow needed to put the brittle‐ductile transition in ice at a depth of 2 km is at least ∼100 mW m−2, much higher...

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Veröffentlicht in:Journal of Geophysical Research: Planets 2000-12, Vol.105 (E12), p.29283-29289
Hauptverfasser: Ruiz, Javier, Tejero, Rosa
Format: Artikel
Sprache:eng
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Zusammenfassung:Some of the geological features on the surface of Europa's ice shell suggest the existence of a brittle lithosphere that in some regions is no more than 2 km thick. The surface heat flow needed to put the brittle‐ductile transition in ice at a depth of 2 km is at least ∼100 mW m−2, much higher than predicted by tidal heating models for a purely conductive ice shell. A possible explanation lies in the probable existence of a convective layer beneath the brittle lithosphere, which, owing to tidal dissipation in warm ice, could contribute to higher heat flows. If a convective subsurface layer and grain size dependent flow behavior of ice are admitted, the grain size at brittle‐ductile transition depth cannot be >1 mm, which is consistent with the required value for the onset of convection in an ice shell thinner than 20 km.
ISSN:0148-0227
2156-2202
DOI:10.1029/1999JE001228