Heat flows through the ice lithosphere of Europa

Authors
Citation
J. Ruiz et R. Tejero, Heat flows through the ice lithosphere of Europa, J GEO R-PLA, 105(E12), 2000, pp. 29283-29289
Citations number
30
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
ISSN journal
21699097 → ACNP
Volume
105
Issue
E12
Year of publication
2000
Pages
29283 - 29289
Database
ISI
SICI code
0148-0227(200012)105:E12<29283:HFTTIL>2.0.ZU;2-Y
Abstract
Some of the gec,logical features on the surface of Europa's ice shell sugge st the existence of a brittle lithosphere that in some regions is no more t han 2 km thick. The surface heat flow needed to put the brittle-ductile tra nsition in ice at a depth of 2 km is at least similar to 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 convectiv e layer beneath the brittle lithosphere, which, owing to tidal dissipation in warm ice, could contribute to higher heat flows. If a convective subsurf ace layer and grain size dependent flow behavior of ice are admitted, the g rain size at brittle-ductile transition depth cannot be >1 mm, which is con sistent with the required value for the onset of convection in an ice shell thinner than 20 km.