Molecular and isotopic analyses of Tagish Lake alkyl dicarboxylic acids

Abstract— The Tagish Lake meteorite soluble organic suite has a general composition that differs from those of both CI and CM chondrites. These differences suggest that distinct processes may have been involved in the formation of different groups of organics in meteorites. Tagish Lake alkyl dicarbo...

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Bibliographic Details
Published in:Meteoritics & Planetary Science
Main Authors: Pizzarello, Sandra, Huang, Yongsong
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2002
Subjects:
Online Access:http://dx.doi.org/10.1111/j.1945-5100.2002.tb00848.x
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2002.tb00848.x
https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2002.tb00848.x
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Summary:Abstract— The Tagish Lake meteorite soluble organic suite has a general composition that differs from those of both CI and CM chondrites. These differences suggest that distinct processes may have been involved in the formation of different groups of organics in meteorites. Tagish Lake alkyl dicarboxylic acids have a varied, abundant distribution and are, with carboxylated pyridines, the only compounds to have an occurrence comparable to that of the Murchison meteorite. This study has undertaken their molecular and isotopic characterization, with the aim to understand their origin and to gain insights into the evolutionary history of the meteorite parent body. Tagish Lake alkyl dicarboxylic acids are present as a homologous series of saturated and unsaturated species with three‐ through ten‐carbon atom chain length. Linear saturated acids are predominant and show decreasing amounts with increasing chain length. A total of 44 of these compounds were detected with the most abundant, succinic acid, present at ˜40 nmol/g meteorite. Overall the molecular distribution of Tagish Lake dicarboxylic acids shows a remarkable compound‐to‐compound correspondence with those observed in the Murchison and Murray meteorites. In both Tagish Lake and Murchison, the imides of the more abundant dicarboxylic acids were also observed. The hydrogen and carbon isotopic compositions of individual Tagish Lake dicarboxylic acids were determined and compared to those of the corresponding acids in the Murchison meteorite. All δD and δ 13 C values for Tagish Lake acids are positive and show a substantial isotopic enrichment. δD values vary from, approximately, +1120% o for succinic acid to +1530% o for methyl glutaric acid. δ 13 C values ranged from +12.6% o for methyl glutaric acid to +22.9% o for glutaric acid, with adipic acid having a significantly lower value (+5.5% o ). Murchison dicarboxylic acid showed similar isotopic values: their δ5 13 C values were generally higher by an average 17% and δD values were lower for succinic and ...