Hydrate sulfuric acid after sulfur implantation in water ice |
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| Authors: | G Strazzulla GA Baratta G Leto O Gomis |
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| Institution: | aINAF – Osservatorio Astrofisico, via S. Sofia 78, I-95123 Catania, Italy;bDepartamento de Fisica Aplicada, Escuela Politecnica Superior Alcoy, Universidad Politecnica de Valencia, Spain |
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| Abstract: | For many years an ongoing research program performed at our laboratory has had the aim to investigate the implantation of reactive ions in ices relevant to planetology by using IR spectroscopy. We present new results obtained by implanting 200 keV sulfur ions into water ice at 80 K. We have looked at the formation of sulfur-bearing molecules such as sulfuric acid, sulfur dioxide and hydrogen sulfide. We find that hydrated sulfuric acid is formed with high yield (0.65±0.1 molecules/ion). An upper limit to the production yield of SO2 (Y 0.025 molecules/ion) has been estimated; no hydrogen sulfide has been detected. The formation of hydrogen peroxide is confirmed. Ozone is not detected. The results are discussed relevant to the inquiry on the radiolytic sulfur cycle considered responsible for the formation of sulfur-bearing molecules on the surfaces of the Galilean satellites. We demonstrate that sulfur implantation efficiently forms hydrated sulfuric acid whose observed abundance is explained as caused by an exogenic process. It is more difficult to say if the observed sulfur dioxide is quantitatively supported by only sulfur implantation; additional experimental studies are necessary along with direct observations, especially at UV wavelengths such as those that could be performed by instruments on board Hubble Space Telescope or by the forthcoming World Space Observatory (WSO/UV). |
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| Keywords: | Satellites surfaces |
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