Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...456..384t&link_type=abstract
Astrophysical Journal v.456, p.384
Astronomy and Astrophysics
Astronomy
29
Molecular Processes, Planets And Satellites: Individual Io, Ultraviolet: Solar System
Scientific paper
We report ultraviolet HST/GHRS observations of Io's spectrum at opposite orbital elongations in the wavelength band 2095-2135 Å smoothed to an effective resolution of 3.7-4.1 Å. Gaseous SO2 absorption over Io's trailing sunlit hemisphere was found to be 37% stronger than over the leading sunlight hemisphere. The effective two-way path of SO_{2 }gas averaged over the disk is 4.4 × 1016 and 3.2 × 1016 SO2 molecules cm-2, respectively. This is in qualitative agreement with the millimeter-wave observations and is opposite to the case for Io's SO2 frost absorption, which is stronger over the leading hemisphere. The corresponding disk-averaged column abundances are 0.7 × 1016 and 0.5 × 1016 SO2 molecules cm-2, respectively, with a 5% uncertainty. Lower limits to the fractional disk coverage of gaseous SO2 are found to be 0.40 and 0.35, respectively. The extreme case where the gas is restricted to a circular region centered at the subsolar point implies minimum fractional hemispherical coverages of 0.23 and 0.20, respectively, and a maximum SO2 column abundance of 9.6 × 1016 cm-2 for each hemisphere (12% fitting uncertainty), substantially more diluted than the millimeter-wave results. Unidentified absorptions appear near 2114 Å and greater than 2128 Å which are unlikely to be SO2 frost because they are not periodic, like the SO2 gas manifolds, and are stronger over the trailing hemisphere.
Barnet Chris
Caldwell J. Jr. J.
Cunningham Colin
Trafton Larry M.
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