“…As regards the icy satellites of Jupiter, Europa, Ganymede, and Callisto, the Near-Infrared Mapping Spectrometer carried about the Galileo spacecraft indicated that the surfaces of these worlds are dominated by hydrate materials. Subsequent to this discovery, there emerged two premises as to the nature of these hydrate materials upon the surface of Europa–that they are brines composed within the MgSO 4 –Na 2 SO 4 –H 2 O system originating from Europa’s interior , or that they are sulfuric acid hydrates (solids in the H 2 SO 4 –H 2 O system) with the H 2 SO 4 radiolytically produced from an influx of sulfur from Io. , More recently, NaCl has been suggested as a major component of the surface of Europa, as color centers in this mineral (a result of the radiation environment of the surface) could explain the surface coloration observed by Galileo . , However, the stability of this effect over geological time scales has been questioned . As a result of these studies, models of Europa’s surface composition are divided into those that are exogenic and those that are endogenic.…”