Physics
Scientific paper
Apr 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002georl..29h..74s&link_type=abstract
Geophysical Research Letters, Volume 29, Issue 8, pp. 74-1, CiteID 1233, DOI 10.1029/2001GL013844
Physics
26
Planetology: Solar System Objects: Jovian Satellites, Tectonophysics: Dynamics, Convection Currents And Mantle Plumes, Tectonophysics: Heat Generation And Transport, Tectonophysics: Planetary Interiors (5430, 5724)
Scientific paper
Tidal heating models are linked to thermal convection models for ice having strongly temperature dependent viscosity. In the range of ice viscosity inferred from laboratory experiments, tidal forces will heat up rising diapirs on Europa. Partial melt produced in the rising diapirs is predicted to create disruption of near-surface materials and formation of lenticulae and chaos, even if the average ice layer thickness overlying an ocean is larger than 20 km.
Head James W.
Sotin Christophe
Tobie Gabriel
No associations
LandOfFree
Europa: Tidal heating of upwelling thermal plumes and the origin of lenticulae and chaos melting does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Europa: Tidal heating of upwelling thermal plumes and the origin of lenticulae and chaos melting, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Europa: Tidal heating of upwelling thermal plumes and the origin of lenticulae and chaos melting will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-842725