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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Published in | Geochemistry international Vol. 58; no. 11; pp. 1228 - 1238 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Moscow
Pleiades Publishing
01.11.2020
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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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. |
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ISSN: | 0016-7029 1556-1968 |
DOI: | 10.1134/S0016702920110105 |