Spectral behavior of hydrated sulfate salts: implications for Europa mission spectrometer design.
Remote sensing of the surface of Europa with near-infrared instruments has suggested the presence of hydrated materials, including sulfate salts. Attention has been focused on these salts for the information they might yield regarding the evolution of a putative interior ocean, and the evaluation of its astrobiological potential. These materials exhibit distinct infrared absorption features due to bound water. The interactions of this water with the host molecules lead to fine structure that can be used to discriminate among these materials on the basis of their spectral behavior. This fine structure is even more pronounced at the low temperatures prevalent on icy satellites. Examination of hydrated sulfate salt spectra measured under cryogenic temperature conditions provides realistic constraints for future remote-sensing missions to Europa. In particular, it suggests that a spectrometer system capable of 2-5 nm spectral resolution or better, with a spatial resolution approaching 100 m, would be able to differentiate among proposed hydrated surface materials, if present, and constrain their distributions across the surface. Such information would provide valuable insights into the evolutionary history of Europa.
SETI Institute, NASA Ames Research Center, Moffett Field, California 94035-1000, USA. dalton@mail.arc.nasa.gov
James Bradley
JB
Dalton
D055580:Astronomical Phenomena; D001256:Astronomy; D003080:Cold Temperature; D004867:Equipment Design / Q000379:methods*; D019419:Evolution, Planetary; D005118:Extraterrestrial Environment; D018538:Jupiter; D008278:Magnesium Sulfate / Q000737:chemistry; D012492:Salts / Q000737:chemistry*; D018531:Spacecraft; D013055:Spectrophotometry, Infrared / Q000295:instrumentation* / Q000379:methods*; D013696:Temperature; D013997:Time Factors; D014867:Water / Q000737:chemistry
D012492:Salts; D014867:Water; D008278:Magnesium Sulfate