西北非洲(NWA) 7059和Nova 018的橄榄石结构和微观结构:对榴辉石变形的洞察

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
A. I. Sheen, C. K. F. Tirona, K. T. Tait, L. F. White, B. C. Hyde, S. Korchinos
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引用次数: 0

摘要

橄榄石是uilites的主要成分,通常通过细长晶粒的形状偏好取向来定义宏观结构。本研究利用电子背散射衍射(EBSD)分析了西北非洲(NWA) 7059和Nova 018中未角砾石橄榄鸽石的橄榄石结构(晶体优选取向,CPO)和微观结构。NWA 7059的逐晶取向数据显示出与晶粒伸长近似平行的<;010>;线理。NWA 7059中两个颗粒的定向失位数据表明,(010)[100]、(001)[100]、(100)[001]和{hk0}[001]滑移体系的活动占优势。Nova 018显示轴向[010]织物,方向错误表示(010)[001],{hk0}[001]滑移,以及(010)捻度边界的形成。Nova 018的轴向-[010]织物与熔体萃取过程中残余橄榄石的压实一致。NWA 7059中的<;010>;线理与典型的uilite织物不同,需要[010]Burgers向量,这在陆地样品中并不常见。橄榄石中2°-10°取向的旋转轴分析表明,两种球粒陨石中[001]滑移和[100]滑移的相对比例与在亚固相温度下变形的普通热冲击球粒陨石相似。然而,两种铀矿的亚固体变形温度与铀矿母体(UPB)的“热破坏”模型不一致。2°-10°取向偏差指标与橄榄石岩心Fo含量之间缺乏相关性,这表明变形温度并不是橄榄石滑移系统的主要控制因素。我们的研究结果强调了利用橄榄石岩石组构来深入了解榴辉石的变形,以及根据UPB的历史解释橄榄石变形数据的复杂性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Olivine fabric and microstructure in Northwest Africa (NWA) 7059 and Nova 018: Insights into ureilite deformation

Olivine fabric and microstructure in Northwest Africa (NWA) 7059 and Nova 018: Insights into ureilite deformation

Olivine is a major constituent in ureilites and commonly defines macroscopic fabric via shape-preferred orientation of elongate grains. In this study, we examined olivine fabric (crystallographic preferred orientation, or CPO) and microstructures in the unbrecciated olivine-pigeonite ureilites Northwest Africa (NWA) 7059 and Nova 018 using electron backscatter diffraction (EBSD) analysis. Point-per-grain orientation data of NWA 7059 indicate a <010> lineation subparallel to grain elongation. Misorientation data of two grains in NWA 7059 indicate dominant activity of (010) [100], (001) [100], (100) [001], and {hk0} [001] slip systems. Nova 018 displays an axial-[010] fabric, with misorientations indicating (010) [001], {hk0} [001] slips, and formation of (010) twist boundaries. Axial-[010] fabric in Nova 018 is consistent with compaction of residual olivine during melt extraction. The <010> lineation in NWA 7059 is unlike typical ureilite fabric and requires a [010] Burgers vector, uncommon in terrestrial samples. Rotational axis analysis of 2°–10° misorientations in olivine shows that the relative proportion of [001] slips and [100] slips in both ureilites are similar to warm-shocked ordinary chondrites, which were deformed at subsolidus temperatures. However, subsolidus deformation temperatures for both studied ureilites are inconsistent with a “hot disruption” model for the ureilite parent body (UPB). The further lack of correlation between 2°–10° misorientation metrics and olivine core Fo content argues against deformation temperature as the main control on olivine slip systems in ureilites. Our findings highlight the use of olivine petrofabric to gain insights into ureilite deformation, as well as complexities in interpreting olivine deformation data with respect to the history of the UPB.

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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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