Investigating the impact of x‐ray computed tomography imaging on soluble organic matter in the Murchison meteorite: Implications for Bennu sample analyses
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- Daniel P. Glavin
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Scott A. Eckley
- Jacobs Technology NASA Johnson Space Center Houston Texas USA
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- José C. Aponte
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Eve L. Berger
- Astromaterials Research and Exploration Science Division NASA Johnson Space Center Houston Texas USA
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- Aaron S. Burton
- Astromaterials Research and Exploration Science Division NASA Johnson Space Center Houston Texas USA
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- Jason P. Dworkin
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Jamie E. Elsila
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Frank T. Ferguson
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Yoshihiro Furukawa
- Department of Earth Science Tohoku University Sendai Japan
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- Heather V. Graham
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Toshiki Koga
- Biogeochemistry Research Center Japan Agency for Marine‐Earth Science and Technology Yokosuka Japan
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- Michael Liss
- Research Unit Analytical Biogeochemistry Helmholtz Munich Neuherberg Germany
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- Hannah L. McLain
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Hiroshi Naraoka
- Department of Earth and Planetary Sciences Kyushu University Fukuoka Japan
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- Yasuhiro Oba
- Institute of Low Temperature Science Hokkaido University Sapporo Japan
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- Eric T. Parker
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Kevin Righter
- Astromaterials Research and Exploration Science Division NASA Johnson Space Center Houston Texas USA
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- Philippe Schmitt‐Kopplin
- Research Unit Analytical Biogeochemistry Helmholtz Munich Neuherberg Germany
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- Danielle N. Simkus
- Solar System Exploration Division NASA Goddard Space Flight Center Greenbelt Maryland USA
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- Yoshinori Takano
- Biogeochemistry Research Center Japan Agency for Marine‐Earth Science and Technology Yokosuka Japan
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- Harold C. Connolly
- Department of Geology, School of Earth and Environment Rowan University Glassboro New Jersey USA
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- Dante S. Lauretta
- Lunar and Planetary Laboratory University of Arizona Tucson Arizona USA
説明
<jats:title>Abstract</jats:title><jats:p>X‐ray computed tomography (XCT) is a valuable reconnaissance tool for three‐dimensional imaging and identification of distinct lithologies in extraterrestrial samples. It will be used as part of the preliminary examination of samples returned from asteroid (101955) Bennu by the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS‐REx) mission. However, it must first be established whether x‐rays generated during XCT could degrade or alter the organic composition of the returned samples by radiolysis. To test this, we split a crushed sample of the Murchison CM2 meteorite, kept one portion as a control, and irradiated the other portion up to the maximum x‐ray dosage (~180 Gy) that a Bennu sample would experience during an XCT imaging experiment. We then extracted organic compounds from both splits and conducted (i) nontargeted soluble organic analyses to compare the chemical distributions of C‐, H‐, O‐, N‐, and S‐bearing species and (ii) targeted measurements to quantify the abundances of 96 individual soluble organic molecules that included protein amino acids, amines, carboxylic acids, hydroxy acids, carbonyl compounds, polycyclic aromatic hydrocarbons, alcohols, sugars, and N‐heterocycles. We found that XCT imaging of the Murchison meteorite had no measurable impact on the relative abundances or enantiomeric compositions of most of the soluble organic compounds targeted in this study. Elevated total abundances of several soluble organic compound classes were observed in the XCT‐scanned Murchison sample relative to the control. This is likely related to particle size heterogeneity and specific surface area differences between the sample aliquots used for the extractions, rather than a result of the x‐ray exposure. Assuming the samples returned from asteroid Bennu by OSIRIS‐REx have a similar composition to carbonaceous chondrites, these data provide confidence that XCT will not significantly alter their soluble organic compositions.</jats:p>
収録刊行物
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- Meteoritics & Planetary Science
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Meteoritics & Planetary Science 59 (1), 105-133, 2023-12-15
Wiley
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詳細情報 詳細情報について
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- CRID
- 1360865815688507648
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- ISSN
- 19455100
- 10869379
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE