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Investigating the Impact of X-Ray Computed Tomography Imaging on Soluble Organic Matter in the Murchison Meteorite: Implications for Bennu Sample AnalysesX-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.
Document ID
20230018340
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Daniel P Glavin ORCID
(Goddard Space Flight Center Greenbelt, United States)
Scott A Eckley ORCID
(Jacobs (United States) Dallas, Texas, United States)
José C Aponte ORCID
(Goddard Space Flight Center Greenbelt, United States)
Eve L Berger
(Johnson Space Center Houston, United States)
Aaron S Burton
(Johnson Space Center Houston, United States)
Jason P Dworkin ORCID
(Goddard Space Flight Center Greenbelt, United States)
Jamie E Elsila
(Goddard Space Flight Center Greenbelt, United States)
Frank T Ferguson
(Catholic University of America Washington D.C., District of Columbia, United States)
Yoshihiro Furukawa ORCID
(Tohoku University Sendai, Japan)
Heather V Graham
(Goddard Space Flight Center Greenbelt, United States)
Toshiki Koga ORCID
(Kyushu University Fukuoka, Japan)
Michael Liss
(Research Unit Analytical BioGeoChemistry Saint-Louis, France)
Hannah L McLain
(Catholic University of America Washington D.C., District of Columbia, United States)
Hiroshi Naraoka ORCID
(Kyushu University Fukuoka, Japan)
Yasuhiro Oba ORCID
(Hokkaido University Sapporo, Hokkaidô, Japan)
Eric T Parker ORCID
(Goddard Space Flight Center Greenbelt, United States)
Kevin Righter ORCID
(Johnson Space Center Houston, United States)
Philippe Schmitt-Kopplin ORCID
(Research Unit Analytical BioGeoChemistry Munich, Germany)
Danielle N Simkus ORCID
(Catholic University of America Washington D.C., District of Columbia, United States)
Yoshinori Takano ORCID
(Japan Agency for Marine-Earth Science and Technology Yokosuka, Japan)
Harold C Connolly Jr. ORCID
(University of Arizona Tucson, United States)
Dante S Lauretta
(University of Arizona Tucson, United States)
Date Acquired
December 18, 2023
Publication Date
December 15, 2023
Publication Information
Publication: Meteoritics and Planetary Science
Publisher: Wiley
Volume: 59
Issue: 1
Issue Publication Date: January 1, 2024
ISSN: 1086-9379
e-ISSN: 1945-5100
Subject Category
Space Sciences (General)
Astronomy
Funding Number(s)
WBS: 828928.04.02.02.01
CONTRACT_GRANT: 80JSC022DA035
CONTRACT_GRANT: 80GSFC21M0002
CONTRACT_GRANT: NNM10AA11C
CONTRACT_GRANT: NNH09ZDA007O
CONTRACT_GRANT: Simons Foundation SCOL 302497
PROJECT: 364653263—TRR 235 (CRC 235)
CONTRACT_GRANT: KAKENHI JP20H00202
CONTRACT_GRANT: KAKENHI JP20H05846
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
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