A high-resolution in situ X-ray diffraction study of mineral transitions due to post-hydration heating in CM chondrite meteorites.

IF 3 3区 地球科学 Earth, Planets and Space Pub Date : 2024-01-01 Epub Date: 2024-12-26 DOI:10.1186/s40623-024-02116-2
Laura E Jenkins, Ashley J King, Martin R Lee, Luke Daly, Stephen P Thompson, Sarah J Day, Lucy Saunders, Pierre-Etienne Martin, Fahkri Bintang
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Abstract

Abstract: The effects of post-hydration heating over a broad range of temperatures are evident in many Mighei-like carbonaceous (CM) chondrites as a variety of mineral transitions. To better understand these processes and how a CM chondrite's starting composition may have affected them, we experimentally heated two meteorites with different degrees of aqueous alteration, Allan Hills 83100 and Murchison, at 25 °C temperature steps from 200 °C to 950 °C and 300 °C to 750 °C, respectively. During heating, synchrotron in situ X-ray diffraction patterns were collected. With the exception of calcite decomposition and its products, most mineral transitions were unaffected by starting composition. Key observations include: (1) partial decomposition of tochilinite at 200 °C, which indicates that tochilinite breakdown might be a two-stage process due to its intergrown layers of brucite/amakinite and mackinawite; (2) the breakdown of serpentine occurring at 300 °C with transitional phases appearing at 525 °C and 575-600 °C, while secondary olivine formed at 600 °C; (3) cronstedtite decomposing faster than lizardite, (4) the formation of secondary enstatite at 750 °C, and (5) calcite decomposition temperature differing significantly between meteorites, occurring at 725 °C and 575 °C in ALH 83100 and Murchison, respectively. The results for calcite are likely controlled by differences in its microstructure and chemical composition, related to the meteorite's impact history and degree of aqueous alteration. The difference in calcite decomposition temperature also explains the contrasts in the observed breakdown products, with clinopyroxene occurring in both meteorites, and oldhamite only in ALH 83100. Mineral transitions due to post-hydration heating have been characterized with a high resolution XRD method, enabling a better understanding of processes occurring on the parent asteroids of CM chondrites.

Graphical abstract:

Supplementary information: The online version contains supplementary material available at 10.1186/s40623-024-02116-2.

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CM球粒陨石水化加热后矿物转变的高分辨率原位x射线衍射研究。
摘要/ Abstract摘要:在许多类梅伊碳质球粒陨石中,在广泛的温度范围内水化后加热的影响是很明显的,因为它是多种矿物转变的产物。为了更好地了解这些过程以及CM球粒陨石的起始成分如何影响它们,我们实验加热了两个具有不同程度水蚀变的陨石,Allan Hills 83100和Murchison,分别在25°C的温度下从200°C到950°C和300°C到750°C。在加热过程中,收集了同步加速器原位x射线衍射图。除了方解石分解及其产物外,大多数矿物转变不受起始成分的影响。主要观测结果包括:(1)在200°C时tochilinite的部分分解,表明tochilinite的分解可能是一个两阶段的过程,这是由于其水镁石/马镁石和mackinaite的交错层;(2)蛇纹石在300℃发生分解,在525℃和575 ~ 600℃出现过渡相,次生橄榄石在600℃形成;(4)在750℃时形成次生辉长辉石;(5)方解石分解温度在陨石间差异显著,ALH 83100和Murchison分别发生在725℃和575℃。方解石的结果可能受其微观结构和化学成分的差异所控制,这些差异与陨石的撞击历史和水蚀变程度有关。方解石分解温度的差异也解释了观察到的分解产物的差异,两种陨石中都有斜辉石,而只有在ALH 83100中才有老辉石。利用高分辨率的XRD方法表征了水化加热后的矿物转变,从而更好地理解CM球粒陨石母小行星上发生的过程。图片摘要:补充资料:在线版本包含补充资料,网址为10.1186/s40623-024-02116-2。
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来源期刊
Earth, Planets and Space
Earth, Planets and Space 地学天文-地球科学综合
CiteScore
5.80
自引率
16.70%
发文量
167
期刊介绍: Earth, Planets and Space (EPS) covers scientific articles in Earth and Planetary Sciences, particularly geomagnetism, aeronomy, space science, seismology, volcanology, geodesy, and planetary science. EPS also welcomes articles in new and interdisciplinary subjects, including instrumentations. Only new and original contents will be accepted for publication.
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