Zusammenfassung
1 Evidence for an ocean beneath the icy crust of Europa includes
reflectance spectra of disrupted surface regions indicating hydrated
materials such as salts. We simulated exposure of salty brine on
the cold surface of Europa by flash-freezing sulfate and carbonate
solutions. This produces materials that have near-infrared reflectance
spectra distinct from those for crystalline minerals and more similar
to those for Europa's non-ice regions. These new spectroscopic data,
along with geophysical evidence, geochemical models, and meteorite
studies, strongly suggest that the non-ice materials in the disrupted
regions on Europa's surface contain large amounts of disordered and
heavily hydrated MgSO4 and perhaps Na2SO4 that are endogenic in origin.
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