Chemical pathways of SO2 with hydrogen atoms on interstellar ice analogues
Thanh Nguyen, Yasuhiro Oba, W. M. C. Sameera, Kenji Furuya, and Naoki, Watanabe

TL;DR
This study investigates the surface reactions of solid SO2 with hydrogen atoms on interstellar ice analogues, revealing partial hydrogenation, formation of sulfur-bearing species, and possible chemical desorption processes relevant to interstellar chemistry.
Contribution
It combines laboratory experiments and computational analyses to elucidate the reaction pathways of SO2 with H atoms on icy surfaces, highlighting new reaction products and desorption mechanisms.
Findings
Approximately 80% of SO2 was lost after H exposure at 10-40 K.
Formation of sulfur-bearing species such as HSO2, H2S, and HS(O)OH was observed.
Some reaction products likely desorb into the gas phase, explaining SO2 loss.
Abstract
Sulfur dioxide (SO2) is a sulfur-containing molecule expected to exist as a solid in the interstellar medium (ISM). In this study, we performed laboratory experiments and computational analyses on the surface reactions of solid SO2 with hydrogen atoms on amorphous solid water (ASW) at low temperatures. After 40 min of exposure of SO2 deposited on ASW to H atoms, approximately 80% of the solid SO2 was lost from the substrate at 10-40 K, and approximately 50% even at 60 K, without any definite detection of reaction products. Quantum chemical calculations suggest that H atoms preferentially add to the S atom of solid SO2, forming the HSO2 radical. Further reactions of the HSO2 radical with H atoms result in the formation of several S-bearing species, including HS(O)OH, the S(O)OH radical, HO-S-OH, HS-OH, and H2S. In codeposition experiments involving H and SO2, we confirmed the formation…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Atmospheric Ozone and Climate · Molecular Spectroscopy and Structure
