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Quantitative determination of the shock stage of L6 ordinary chondrites using X-ray diffraction

  • Naoya Imae ORCID logo and Makoto Kimura
Published/Copyright: September 4, 2021
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Abstract

The shock stages of 14 L6 ordinary chondrites are estimated using the random X‑ray diffraction patterns of polished thin section samples and the in-plane rotation method. The mean lattice strains and grain size factors for olivine and orthopyroxene are determined from the analyses based on the Williamson–Hall plots, which depict the tangent Bragg angle and integral breadth β. The lattice strain in olivine, εOl, is distributed from ~0.05% to ~0.25%, while that in orthopyroxene, εOpx, is distributed from ~0.1 to ~0.4%, where we selected the isolated peaks of olivine and orthopyroxene. The olivine peaks have Miller indices of (130), (211), (222), and (322), while the orthopyroxene peaks have Miller indices of (610), (511), (421), (631), and (12.1.2). The intercept for integral breadth β 0 O1  and β 0 O p x for the Williamson–Hall plots correlates with the grain size of the constituent minerals. The grain size is proportional to the inverse of β0 since the β intercept increases with the shock stage. Introducing a new parameter, –ε/log β0 for olivine (0.04–0.16) and orthopyroxene (0.07–0.32) reveals a clear relationship between them: –εOpx/log β 0 O p x = –0.01+ 2.0 ε 01 / log β 0 O 1 (R > 0.9). In addition, the isolated peak of plagioclase (2̅01) systematically changes as the shock stage increases, suggesting the progress of amorphization (maskelynitization). Another parameter, (I/FWHM)Pl(2̅01) reveals additional relationships: ε O l / log β 0 O l = 0.14(±0.01) − 5.2 × 10−5 (±5.7 × 10−6) × (I/FWHM)Pl(2̅01), and ε O p x / log β 0 O p x = 0.25(±0.04) − 8.9 × 10−5 (±2.6 × 10−5) × 10–5 × (I/FWHM)Pl(2̅01). These three parameters systematically change with the shock stage, suggesting that they are suitable shock barometers. The present method is useful to evaluate the shock stage of L6 chondrites and potentially enables quantitative shock stage classification for stony meteorites.

Funding statement: The study is partly supported by KAKENHI 17K05721 and NIPR Research Project KP-307. The polished thin sections of the Antarctic meteorites and Tenham were on loan from NIPR.

Acknowledgments and Funding

We are grateful to Anner Peslier, Associate Editor, for the handling of our manuscript and the constructive review, and Roberta L. Flemming, Jörg Fritz, and Jacob A. Tielke for their constructive and thoughtful reviews. We are grateful to Yoshihiro Nakamuta, Naotaka Tomioka, Masahiro Yasutake, and Rei Kanemaru for the discussions and to Sen Hu for supplying and permission to use of the Mangui L6 chondrite fell in 1 June 2018 on Yunnan, China.

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Received: 2020-04-09
Accepted: 2020-10-24
Published Online: 2021-09-04
Published in Print: 2021-09-27

© 2021 Mineralogical Society of America

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