首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Oriented chromite-diopside symplectic inclusions in olivine from lunar regolith delivered by ' Luna-24' mission
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Oriented chromite-diopside symplectic inclusions in olivine from lunar regolith delivered by ' Luna-24' mission

机译:“ Luna-24”任务送出的月牙长石中橄榄石中的定向铬铁矿-透辉石夹杂物

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摘要

Calcium-chromium rich lamellae in olivine grain No. 1611 from the Luna-24 regolith were studied with FEG-EMPA and TEM. The lamellae consist of a worm-like intergrowth of FeCr_2O_4 chromite (Chr) and CaMgSi_2O_6 diopside (Di), with a Chr:Di modal proportion of 1:3. The linear extension of the lamellae and crystallographic orientation relationships among the symplectite phases and the olivine suggest that the lamellae nucleated at deformation defects in the olivine host. Calcium depletion haloes surrounding the lamellae amount to about 75μm and indicate that the chromite+diopside lamellae were formed by segregation of calcium and chromium from the host olivine into the lamellae without addition of calcium and/or chromium from outside the olivine. The segregation of calcium and chromium and, consequently, the growth of the symplectic lamellae were diffusion-controlled.The segregation of a calcium-chromium component from the host olivine was associated with oxidation of divalent to trivalent chromium. Oxidation was facilitated by dehydrogenation, which was driven by decompression and/or a change in redox potential. Hydrogen point defects in the original olivine with H~+ substituting for divalent cations on the M-sites provided the necessary electron acceptors for the oxidation of chromium and after electron transfer left olivine as molecular H_2. The internal microstructure of the lamellae suggests that exsolution of the calcium-chromium rich lamellae from the host olivine and formation of the chromite-diopside symplectic intergrowth occurred simultaneously. The time scale derived from diffusion modeling of the calcium depletion haloes around the lamellae indicates a thermal event on the order of several months to several hundred years at most.Symplectic inclusions found in olivine from lunar, martian and terrestrial rocks are similar with respect to their shape, crystallographic orientation relationships, and internal microstructure of the spinel-clinopyroxene intergrowth. These features are inconsistent with " dry" olivine oxidation that is by the uptake of oxygen. Dehydrogenation of OH-bearing precursor olivine is suggested as a general mechanism of oxidation accompanied by chemical segregation and phase separation resulting in symplectite formation.
机译:用FEG-EMPA和TEM研究了Luna-24块石的橄榄石1611号中富含钙铬的薄片。薄片由蠕虫状的FeCr_2O_4亚铬酸盐(Chr)和CaMgSi_2O_6透辉石(Di)共生,Chr:Di模态比例为1:3。片晶的线性延伸以及在各晶相和橄榄石之间的晶体学取向关系表明,该片晶在橄榄石宿主的形变缺陷处成核。薄片周围的钙贫化晕圈总计约75μm,表明亚铁盐+透辉石薄片是由钙和铬从主橄榄石中分离到薄片中而形成的,而没有从橄榄石外部添加钙和/或铬。钙和铬的偏析以及因此导致的辛片的生长受到扩散控制。钙铬成分从主体橄榄石中的偏析与二价铬到三价铬的氧化有关。脱氢促进了氧化,脱氢是由减压和/或氧化还原电位的变化驱动的。原始橄榄石中的氢点缺陷被H〜+取代了M位上的二价阳离子,为铬的氧化提供了必要的电子受体,并且在电子转移后,橄榄石以分子H_2的形式出现。薄片的内部微观结构表明,富含钙铬的薄片从宿主橄榄石中析出和铬铁-透辉石辛共生的形成同时发生。从片层周围贫钙晕圈的扩散模型得出的时间尺度表明,一个热事件最多长达数月至数百年。从月球,火星和陆地岩石中发现的橄榄石中的符号夹杂物在它们的方面相似尖晶石-斜茂铁共生的形状,晶体取向关系和内部微观结构。这些特征与氧气吸收引起的“干燥”橄榄石氧化不一致。含OH的前体橄榄石的脱氢被认为是氧化的一般机理,伴随着化学分离和相分离,导致了硬石膏的形成。

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