Jupiter's Moon: Europa

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This liquid water, in combination with a rocky silicate sea floor and radiolytically produce surface oxidants, may provide for a chemically rich ocean that would be considered habitable. While the surface of Europa may contain clues about the composition of an interior ocean, debate still continues about the surface’s chemistry and how exogenous radiation processing and endogenous oceanic emplacement play a role on this moon. One way of understanding Europa is determining if the external composition reflects the internal ocean chemistry. Results from the NIMS (Near Infrared Mapping Spectrograph) instrument on Galileo inferred that the surface of Europa was dominated by hydrated sulfate salts that would be probable in evaporates from an internal ocean. In finding that these spectral signatures are more predominant in what seems to be younger terrains, it strengthens the hypothesis that these are more newly sited evaporates. Further Study of the spectra, however, showed that these same NIMS surface spectra could be explained just as well by a surface dominated by hydrated sulfuric acid. Sulfuric acid is a probable outcome of bombardment of a frozen surface by sulfur ions. These sulfur ions are ultimately come from volcanoes located on Io, and then dissociated, ionized, and accelerated by Jupiter’s quickly spinning magnetic field until they hit Europa. Such radiolysis could also clarify the sulfur dioxide and sulfur allotropes seen on the surface of Europa and their favored appearance on the more heavily bombarded trailing hemisphere. The existence of sulfuric acid and other sulfur products appears to be nearly unavoidable, but the salt hypothesis is still convincing (Brown 1).
If there were to be a mission to Europa, it could possi...

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