Evidence for Abiotic Dimethyl Sulfide in Cometary Matter
Nora H\"anni, Kathrin Altwegg, Michael Combi, Stephen A. Fuselier,, Johan De Keyser, Niels F. W. Ligterink, Martin Rubin, and Susanne F. Wampfler

TL;DR
This study provides the first evidence of abiotic dimethyl sulfide (DMS) in cometary matter, suggesting complex sulfur chemistry can occur without biological processes, which has implications for understanding organic molecules in space.
Contribution
The paper demonstrates the presence of abiotic DMS in comet 67P, challenging the notion that DMS is exclusively a biosignature and revealing new insights into cometary sulfur chemistry.
Findings
DMS is compatible with observed mass spectra better than ethanethiol.
DMS abundance in comet 67P is approximately 0.13%.
First evidence of abiotic DMS formation in cometary matter.
Abstract
Technological progress related to astronomical observatories such as the recently launched James Webb Space Telescope (JWST) allows searching for signs of life beyond our Solar System, namely in the form of unambiguous biosignature gases in exoplanetary atmospheres. The tentative assignment of a spectral feature observed with JWST in the atmosphere of exoplanet K2-18b to the biosignature gas dimethyl sulfide (DMS; sum formula CHS) raised hopes that, although controversial, a second genesis had been found. Terrestrial atmospheric DMS is exclusively stemming from marine biological activity and no natural abiotic source has been identified - neither on Earth nor in space. Therefore, DMS is considered a robust biosignature. Since comets possess a pristine inventory of complex organic molecules of abiotic origin, we have searched high-resolution mass spectra collected…
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