Detection and quantification of organosulfur species in the Tagish Lake Meteorite by highly sensitive LC‐MS

Abstract We analyzed the methanol extracts of six pristine specimens of the Tagish Lake meteorite (TL1, TL4, TL5A, TL6, TL7, and TL10a) and heated and unheated samples of Allende using high‐performance liquid chromatography coupled with high‐resolution, accurate mass–mass spectrometry (HPLC‐HRAM‐MS)...

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Bibliographic Details
Published in:Meteoritics & Planetary Science
Main Authors: Randazzo, N., Hilts, R. W., Holt, M. C., Herd, C. D. K., Reiz, B., Whittal, R. M.
Other Authors: Natural Sciences and Engineering Research Council of Canada, University of Alberta, Government of Alberta, Canada Foundation for Innovation
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2024
Subjects:
Tagish
Tagish Lake
Online Access:http://dx.doi.org/10.1111/maps.14189
https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.14189
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Summary:Abstract We analyzed the methanol extracts of six pristine specimens of the Tagish Lake meteorite (TL1, TL4, TL5A, TL6, TL7, and TL10a) and heated and unheated samples of Allende using high‐performance liquid chromatography coupled with high‐resolution, accurate mass–mass spectrometry (HPLC‐HRAM‐MS). All samples contained ppm levels of sulfate and methyl sulfate. The most abundant organosulfur compound in the methanol extracts of the Tagish Lake and Allende samples was methyl sulfate, which was likely formed primarily via an esterification reaction between intrinsic sources of methanol and sulfate. A homologous series of polythionic acids was also observed in the extracts of the Tagish Lake specimens and Allende. The polythionic acids were the most abundant soluble inorganic sulfur species found in the meteorites. Our results were confirmed using retention time, accurate mass, isotope matching, and tandem mass spectrometry (MS/MS). Hydroxymethanesulfonic acid, previously reported in Tagish Lake, was found only in an unheated Allende sample and in low abundance. Here, we propose possible sulfate formation pathways that begin with interstellar dimethyl sulfide, dimethyl disulfide, methyl sulfide, or methanethiol via cold, nebular processes within the interstellar medium and continue via MSA as an intermediary compound ending within planetary bodies with sulfate and methyl sulfate as the final products.

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