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Published September 1, 2024 | Published
Journal Article Open

Oxygen isotope equilibria of O-bearing organic compounds based on first principle quantum mechanical models, and implications for their use in the study of extraterrestrial organics

  • 1. ROR icon California Institute of Technology

Abstract

We report theoretically calculated equilibrium oxygen isotopic fractionation factors (17O/16O, 18O/16O) between a set of representative O-bearing organic molecules and water, as well as site specific 13C, 15N and 13C—18O equilibrium clumped isotopic anomalies in these compounds, all computed using density functional theory (DFT) methods combined with Urey-Bigeleisen-Mayer (UBM) calculations of reduced partition function ratios. We performed density functional theory (DFT) calculations with the B3LYP exchange correlation functional, and explored different basis sets, and treatments of solvation. After benchmarking results against prior theoretical and empirical studies, we conclude that B3LYP level of theory and aug-cc-pVTZ basis set with cluster solvation provides the most accurate treatment of this problem within the constraints of our approach. A representative set of O bearing organic compounds including aldehyde, ketones, amino acid and aromatic alcohol are predicted to be ∼24–41 ‰ higher in 18O/16O relative to water with θcompound – water varying in the range 0.522–0.526; and ∼ 23–41 ‰ lower in 13C/12C and ∼ 11 ‰ higher in 15N/14N relative to CO2 and N2, respectively (all presuming equilibrium partitioning) at 273 K.

This study is motivated by the study of soluble organic molecules found in carbonaceous chondrite meteorites, a significant fraction of which contain oxygen in their structure in the form of functional groups such as carbonyl, carboxylic acid, ester, ethers, and alcohol. These samples also contain oxygen-bearing macromolecular organic matter. We use the fractionation factors presented here to predict the triple oxygen isotope compositions of these organics, assuming equilibration with previously proposed early solar system volatile reservoirs and environments of organic synthesis.

Copyright and License

© 2024 Elsevier Ltd. All rights are reserved, including those for text and data mining, AI training, and similar technologies.

Acknowledgement

SB acknowledges Roman Korol, Ojashvi Rautela, Hao Xie for help with computational issues and Simon Andren Alexander Meshoulam, Sarah Zeichner, Amy Hofmann, Laura Chimiak, Noam Lotem for helpful discussions. We thank Jeffrey Catalano and Yoko Kebukawa for prompt editorial handling of the manuscript and considering this work for publication. We sincerely thank three unknown reviewers for constructive and helpful reviews. This study is supported by Caltech Center for Comparative Planetary EvolutionUnited States Department of Energy (grant no.: DE-SC0016561) and Simons Foundation funding awarded to JME.

Funding

This study is supported by Caltech Center for Comparative Planetary EvolutionUnited States Department of Energy (grant no.: DE-SC0016561) and Simons Foundation funding awarded to JME.

Contributions

Surjyendu Bhattacharjee: Writing – review & editing, Writing – original draft, Visualization, Validation, Software, Methodology, Investigation. John M. Eiler: Writing – review & editing, Writing – original draft, Supervision, Resources, Methodology, Funding acquisition, Conceptualization.

Data Availability

Data are available through CaltechDATA at https://doi.org/10.22002/5za3h-ckp07.

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Additional details

Created:
September 24, 2024
Modified:
September 25, 2024