title: The 2.5-5.0 micrometers spectra of Io:  evidence for H2S and H2O frozen in SO2.
abstract: Infrared spectra of Io in the region 2.5-5.0 micrometers, including new observational data, are analyzed using detailed laboratory studies of plausible surface ices.  Besides the absorption bands attributable to sulfur dioxide frosts, four infrared spectral features of Io are shown to be unidentified.  These unidentified features show spatial and temporal band strength variations.  One pair is centered around 3.9 micrometers (3.85 and 3.91 micrometers) and the second pair is centered around 3.0 micrometers (2.97 and 3.15 micrometers).  These absorptions fall close to the fundamental stretching modes in H2S and H2O, respectively.  The infrared absorption spectra of an extensive set of laboratory ices ranging from pure materials, to binary mixtures of H2S and H2O (either mixed at different concentrations or layered), to H2O:H2S:SO2 mixtures are discussed.  The effects of ultraviolet irradiation (120 and 160 nm) and temperature variation (from 9 to 130 K) on the infrared spectra of the ices are examined.  This comparative study of Io reflectance spectra with the laboratory mixed ice transmission data shows the following:  (1) Io's surface most likely contains H2S and H2O mixed with SO2.  The 3.85- and 3.91-micrometers bands in the Io spectra can be accounted for by the absorption of the S-H stretching vibration (nu 1) in H2S clusters and isolated molecules in an SO2-dominated ice.  The weak 2.97- and 3.15-micrometers bands which vary spatially and temporally in the Io spectra coincide with the nu 3 and nu 1 O-H stretching vibrations of clusters of H2O molecules complexed, through hydrogen bonding and charge transfer interactions, with SO2.  (2) The observations are well matched qualitatively by the transmission spectra of SO2 ices containing about 3% H2S and 0.1% H2O which have been formed by the condensation of a mixture of the gases onto a 100 K surface.  (3) No new features are produced in the region 2.5 to 5.0 micrometers in the spectrum of these ices under prolonged ultraviolet irradiation or temperature variation up to 120 K.  (4) Comparison of the Io spectra to transmission spectra of both mixed molecular ices and layered ices indicates that only the former can explain the shifts and splitting of the absorption bands seen in the Io spectrum and additionally can account for the fact that solid H2S is observed in the surface material of Io at temperature and pressure conditions above the sublimation point of pure H2S.
authors.affiliation: NASA-Ames Research Center, Space Science Division, Moffett Field, California 94035, USA.
authors.forename: F
authors.initials: F
authors.lastname: Salama
authors.forename: L J
authors.initials: LJ
authors.lastname: Allamandola
authors.forename: F C
authors.initials: FC
authors.lastname: Witteborn
authors.forename: D P
authors.initials: DP
authors.lastname: Cruikshank
authors.forename: S A
authors.initials: SA
authors.lastname: Sandford
authors.forename: J D
authors.initials: JD
authors.lastname: Bregman
mesh_terms: D055580:Astronomical Phenomena; D001256:Astronomy; D005118:Extraterrestrial Environment; D006862:Hydrogen Sulfide / Q000032:analysis*; D007053:Ice / Q000032:analysis*; D018538:Jupiter; D013057:Spectrum Analysis; D013458:Sulfur Dioxide / Q000032:analysis*; D013696:Temperature; D014867:Water / Q000032:analysis*
chemical_list: D007053:Ice; D014867:Water; D013458:Sulfur Dioxide; D006862:Hydrogen Sulfide