Investigating the Impact of X-Ray Computed Tomography Imaging on Soluble Organic Matter in the Murchison Meteorite: Implications for Bennu Sample Analyses

• Published in: Meteoritics & planetary science Vol. 59; no. 1; pp. 105 - 133
• Main Authors: Glavin, Daniel P, Eckley, Scott A, Aponte, José C, Berger, Eve L, Burton, Aaron S, Dworkin, Jason P, Elsila, Jamie E, Ferguson, Frank T, Furukawa, Yoshihiro, Graham, Heather V, Koga, Toshiki, Liss, Michael, McLain, Hannah L, Naraoka, Hiroshi, Oba, Yasuhiro, Parker, Eric T, Righter, Kevin, Schmitt-Kopplin, Philippe, Simkus, Danielle N, Takano, Yoshinori, Jr, Harold C Connolly, Lauretta, Dante S
• Format: Journal Article
• Language: English
• Published: Goddard Space Flight Center Wiley 01.01.2024; Wiley Subscription Services, Inc
• Subjects: Abundance; Alcohols; Amines; Amino acids; Apollo asteroids; Aromatic compounds; Asteroids; Astronomy; Carbonaceous chondrites; Carbonyl compounds; Carbonyls; Carboxylic acids; Chondrites; Composition; Computed tomography; Heterogeneity; Hydroxy acids; Imaging; Meteorites; Meteors & meteorites; Murchison meteorite; Organic chemistry; Organic compounds; Organic matter; Polycyclic aromatic hydrocarbons; Regolith; Space Sciences (General); Tomography
• ISSN: 1086-9379; 1945-5100
• DOI: 10.1111/maps.14111

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.