Astrochemistry

Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH2DSH)

By Keith Cowing
Status Report
astro-ph.GA
February 2, 2025
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Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH2DSH)
The experimental far-infrared spectrum (top) of CH2DSH showing the Q-branch of three intrastate (∆νt=0) torsional subbands, near 27.2 cm−1 , and two interstate (∆νt=±1) torsional subbands near 26.75 cm−1 and 27.6 cm−1 . The calculated spectrum (bottom) emphasizes the strong overlap between bands, especially near 27.2 cm−1 . Calculated transitions are colour coded with red, blue, and green indicating that their lower torsional state is e0, o1, and e1, respectively. — astro-ph.GA

We report an extensive rotational spectroscopic analysis of singly deuterated methyl mercaptan (CH2DSH) using both millimeter and far-infrared synchrotron spectra to achieve a global torsional analysis of the three lowest torsional substates (e0, e1, and o1) of this non-rigid species.

A fit including 3419 millimeter wave transitions along with 43 infrared torsional subband centers was performed with root mean square deviations of 0.233 MHz and 0.270 cm−1, respectively, resulting in 68 fit parameters.

A spectroscopic catalogue built from this analysis for a temperature of 125 K has led to the first interstellar detection of CH2DSH towards the Solar-like protostar IRAS 16293-2422 B. We report the identification of 46 transitions, including eight relatively unblended lines, resulting in a derived column density of (3.0±0.3)×1014 cm−2. The column density ratio for HDCS/CH2DSH compared to HDCO/CH2DOH suggests a difference in the interstellar chemistry between the sulphur and oxygen complex organics, in particular a different link between H2CO and CH3OH and between H2CS and CH3SH.

This is the first interstellar detection of a deuterated sulphur-bearing COM and therefore an important step into understanding the chemical origin of sulphur-based prebiotics.

Hayley A. Bunn, Silvia Spezzano, Laurent H. Coudert, Jean-Claude Guillemin, Yuxin Lin, Christian P. Endres, Brant Billinghurst, Olivier Pirali, Jes Jørgensen, Valerio Lattanzi, Paola Caselli

Comments: Accepted for publication in Astrophysical Journal Letters (ApJL)
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2501.15944 [astro-ph.GA] (or arXiv:2501.15944v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2501.15944
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Submission history
From: Hayley Bunn
[v1] Mon, 27 Jan 2025 10:44:15 UTC (573 KB)
https://arxiv.org/abs/2501.15944
Astrobiology, Astrochemistry

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻