A search for temporal variability in the surface chemistry of the icy Galilean satellites

Details A search for temporal variability in the surface chemistry of the icy Galilean satellites A search for temporal variability in the surface chemistry of the icy Galilean satellites

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005icar..173...50d&link_type=abstract

Icarus, Volume 173, Issue 1, p. 50-65.

Physics

2

Spectroscopy, Europa, Ganymede, Callisto, Satellite

Scientific paper

The purpose of this study was to determine if any temporal variability in the broadband UV spectral properties of the icy Galilean satellites exists, and if so, to characterize its spatial distribution as a function of longitude in order to attempt to correlate any temporal changes with satellite surface interactions with the space environment. The temporal time period examined is between 1978-1984 (referred to as the 1980s data) and those from 1995-1996 (referred to as the 1990s data). The plausible temporal characteristics detected appear to vary from one satellite to the next. For Europa possible temporal variations are concentrated on the leading, anti-jovian quadrant. Example broadband UV spectra show Europa's spectral slope decreases (and darkens) with time on the leading and anti-jovian hemispheres, but remains essentially constant with time on the trailing hemisphere. The data quality does not support any definitive temporal changes for Ganymede. Possible temporal changes seen in the Callisto data set are concentrated on the jovian hemisphere. Example broadband UV spectra for Callisto show no definitive change in slope with time. The hypothesis is that these temporal differences in UV spectral properties are caused by variations in the surface ice chemistry due to temporal variability in the space environment. It is postulated that the UV spectral changes suggested for Europa may be linked to changes in H2O2 concentrations, whereas the changes on Callisto may be linked to variability in SO2 concentration.

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