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Modeling Triatomic Biosignatures: Ozone and Isotopomers

Cross, Thomas M.; Benoit, David M.; Pignatari, Marco

Authors

Thomas M. Cross

Profile image of David Benoit

Dr David Benoit D.Benoit@hull.ac.uk
Senior Lecturer in Molecular Physics and Astrochemistry

Marco Pignatari



Abstract

In this work, we present a new approach to produce spectroscopic constants and model first-principles synthetic spectra for all molecules of astrophysical interest. We have generalized our previous diatomic molecule simulation framework, employing transition-optimized shifted Hermite (TOSH) theory, thereby enabling the modeling of polyatomic rotational constants for molecules with three or more atoms. These capabilities are now provided by our new code Epimetheus. As a first validation of our approach, we confront our predictions and assess their accuracy against the well-studied triatomic molecule ozone 666 (16O3), in addition to eight of its potential isotopomers: ozone 668 (16O16O18O), 686 (16O18O16O), 667 (16O16O17O), 676 (16O17O16O), 688 (16O18O18O), 868 (18O16O18O), 888 (18O3), and 777 (17O3). We then assess the accuracy of these rotational constants using the Epimetheus data in our code Pandora, and generate synthetic molecular spectra. The ozone spectra presented here are purely infrared and not Raman. Epimetheus builds upon the work from our previous code Prometheus, which used the TOSH theory to account for anharmonicity for the fundamental ν = 0 → ν = 1 band, going further to now account for triatomic molecules. This is combined with thermal profile modeling for the rotational transitions. We have found that this extended method performs well, typically approximating the spectroscopic constants with errors of less than 2%. Some issues do arise depending on the symmetry group of the ozone isotopomer. From these spectroscopic constants and using our own spectral modeling code, we show that we can provide the data to produce appreciable molecular spectra, which are good approximations until high-resolution studies can be done.

Citation

Cross, T. M., Benoit, D. M., & Pignatari, M. (2025). Modeling Triatomic Biosignatures: Ozone and Isotopomers. The Astrophysical journal, 985(1), Article 110. https://doi.org/10.3847/1538-4357/adbc61

Journal Article Type Article
Acceptance Date Mar 1, 2025
Online Publication Date May 16, 2025
Publication Date May 20, 2025
Deposit Date Jun 2, 2025
Publicly Available Date Jun 19, 2025
Journal Astrophysical Journal
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 985
Issue 1
Article Number 110
DOI https://doi.org/10.3847/1538-4357/adbc61
Keywords Biosignatures; Astrochemistry
Public URL https://hull-repository.worktribe.com/output/5185247

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Copyright Statement
© 2025. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.




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