Interstellar Ice Chemistry Yields Elusive Sulfinothioic Acid (HS(O)SH)

M Mason McAnally (Department of Chemistry, University of Hawaii at Mānoa) Z Zesen Wang (W. M. Keck Research Laboratory in Astrochemistry) C Chaojiang Zhang (W. M. Keck Research Laboratory in Astrochemistry) J Jia Wang R Ryan Fortenberry (Department of Chemistry & Biochemistry University of Mississippi University Oxford MS USA) R Ralf I. Kaiser (Department of Chemistry)

Abstract

ABSTRACT Low‐oxidation‐state sulfur oxyacids are key yet experimentally elusive intermediates in interstellar sulfur chemistry; even the simplest member, sulfinothioic acid (HS(O)SH), has neither been detected in space nor isolated terrestrially. The S–S(O) motif, also present in biological systems, can be reduced to form disulfide bridges (RSSR’), suggesting potential astrobiological relevance. Here, we report the first formation of sulfinothioic acid in astrophysically relevant sulfur dioxide (SO 2 )–water (H 2 O) ices and its identification via isomer‐selective photoionization reflectron time‐of‐flight mass spectrometry combined with isotopic labeling. Irradiation of these ices at 5 K under ultrahigh vacuum with galactic cosmic‐ray proxies yields sulfinothioic acid. These results establish a missing link in interstellar sulfur chemistry and reveal a previously unrecognized class of astrochemically accessible sulfur oxyacids formed via radical‐mediated, non‐equilibrium processes driven by energetic particles in cold interstellar environments.

Article Details

Volume / Issue Vol. 1, Issue 1
Published July 10, 2026
ISSN 1433-7851
Publisher Wiley

Journal Info

Angewandte Chemie International Edition

Wiley

ISSN: 1433-7851 Physical Sciences

Authors (6)

M

Mason McAnally

Department of Chemistry, University of Hawaii at Mānoa

Z

Zesen Wang

W. M. Keck Research Laboratory in Astrochemistry

C

Chaojiang Zhang

W. M. Keck Research Laboratory in Astrochemistry

J

Jia Wang

R

Ryan Fortenberry

Department of Chemistry & Biochemistry University of Mississippi University Oxford MS USA

R

Ralf I. Kaiser

Department of Chemistry