Physics
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jgr...106.7567s&link_type=abstract
Journal of Geophysical Research, Volume 106, Issue E4, p. 7567-7576
Physics
15
Planetology: Solid Surface Planets, Planetology: Solid Surface Planets: Interiors, Planetology: Solid Surface Planets: Origin And Evolution, Planetology: Solar System Objects: Jovian Satellites
Scientific paper
Recent results from the Galileo Near-Infrared Mapping Spectrometer (NIMS) experiment suggest that hydrated magnesium sulfate salts may be present on the surface of Europa. We use this interpretation and a model for the chemical budget of Europa's outer water-rich layer to determine (1) how Europa's profile atop the mantle may have evolved by cooling and fractional crystallization from an initial liquid state and (2) the potential effects of this evolution on the surface geology. This model leads to predictions that the lower part is composed of layers of heavily hydrated magnesium sulfates, which effectively isolate any ocean from direct physical contact with the silicate mantle. These lower layers are overlain by an ocean which has an icy solid upper layer present at the surface; this ocean may have persisted through time. Eutectic conditions are predicted to lead to thickening of the overlying ice shell and freezing out of the ocean, although tidal heating may maintain the liquid layer. Mechanisms such as solid-state convection can further serve to thicken, thin, and/or mix the ice shell. Thermal diapirism could be induced by convection, and compositional diapirism could be driven by density instabilities within the layers. In this model, early global compression would have given way to later global expansion.
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