Mass-Independent Sulfur Isotope Fractionation in the Photochemical SO2 Processes under the UV Radiation of Different Wave Length

A series of photochemical experiments with sulfur dioxide were carried out using a xenon lamp (λ > 200 nm), a low-pressure mercury lamp (λ = 184.9 and 253.7 nm), and an UP-213 laser system (λ = 213 nm) as light sources. Based on the isotope data obtained for elemental sulfur (the end product of S...

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Bibliographic Details
Published inGeochemistry international Vol. 58; no. 11; pp. 1228 - 1238
Main Authors Velivetskaya, T. A., Ignatiev, A. V., Yakovenko, V. V.
Format Journal Article
LanguageEnglish
Published Moscow Pleiades Publishing 01.11.2020
Springer Nature B.V
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Summary:A series of photochemical experiments with sulfur dioxide were carried out using a xenon lamp (λ > 200 nm), a low-pressure mercury lamp (λ = 184.9 and 253.7 nm), and an UP-213 laser system (λ = 213 nm) as light sources. Based on the isotope data obtained for elemental sulfur (the end product of SO 2 photolysis), we revealed specifics in correlations between δ 34 S, ∆ 33 S, and ∆ 36 S values depending on the spectral characteristics of the incident radiation. Our studies showed that the Archean Δ 33 S/δ 34 S and Δ 36 S/Δ 33 S ratios could be reproduced in the SO 2 photolysis experiments by combining spectral composition of the radiation, the intensity of the spectral components, and the partial pressure of SO 2 . The results of the experiments suggest that the UV radiation with wavelengths less than 200 nm was a determining factor in the production of sulfur isotopic anomalies in the Archean atmosphere.
ISSN:0016-7029
1556-1968
DOI:10.1134/S0016702920110105