来自CK3碳质球粒陨石的CAIs中的次生刚玉确定了CK球粒陨石交代变化的年代

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
A. N. Krot, K. Nagashima, S. Ebert, M. I. Petaev, C. Ma, J. Han, T. L. Dunn
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引用次数: 0

摘要

本文报道了CK3 (karoonda型)碳质球粒陨石NWA(西北非洲)4964-#1和- homer, NWA 5343-#1和LAR (Larkman Nunatak) 12002-#1中含刚玉的Ca, al富包裹体(CAIs)的矿物学、岩石学、氧和铝镁同位素系统。这些CAIs经历了广泛的交代蚀变:千英石(可能还有钙长石和铝透辉石)几乎完全被次生刚玉、粗晶、cana斜长石、铁透辉石和富feo尖晶石所取代;钙钛矿大部分被钛铁矿取代。NWA 4964 CAIs中出现了两种类型的刚玉颗粒:(1)致密,阴极发光(CL)图像中显示FeO贫颗粒;(2)含FeO(高达1.5 wt% FeO),多孔颗粒,未检测到CL;多孔刚玉晶粒比致密刚玉晶粒长得多。LAR 12002和NWA 5343的CAIs中刚玉晶粒分别属于第一类和第二类。尖晶石中的Hibonite、原生尖晶石和稀有钙钛矿包裹体保留了原始的富含16o的成分(Δ17O ~−24±2‰),而melilite、大多数钙钛矿颗粒、次生刚玉和尖晶石则缺乏16o (Δ17O ~−5±2‰)。Hibonite和melilite具有过量的放射性成因26Mg (26Mg*),大约对应于典型的初始26Al/27Al比值[(26Al/27Al)0]为~5 × 10−5,这表明所研究的含刚玉的CAIs属于典型包裹体群体,在大多数球粒陨石群中占主导地位。在LAR 12002-#1、NWA 4964-#1、NWA 4964- homer和NWA 5343-#1中,刚玉晶粒的26Mg*与27Al/24Mg比值的相关性远低于规范的(26Al/27Al)0:(3.10±0.48)× 10−6、(3.03±0.23)× 10−6、(2.72±0.19)× 10−6和(3.5±1.2)× 10−7。NWA 4964 CAIs Homer和#1的多孔含铁刚玉颗粒26Mg*较低,与27Al/24Mg比值无关。我们认为,CK3 CAIs致密刚玉颗粒是在结晶后3 ~ 5 Ma的热液作用下,寄主包裹体发生交代蚀变的次生母体产物。多孔刚玉颗粒可能是由一水硬铝石[AlO(OH)]在随后的热变质过程中脱水形成的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Secondary corundum in CAIs from CK3 carbonaceous chondrites dates metasomatic alteration of CK chondrites

Secondary corundum in CAIs from CK3 carbonaceous chondrites dates metasomatic alteration of CK chondrites

We report on the mineralogy, petrography, and oxygen and aluminum-magnesium isotopic systematics of the corundum-bearing Ca,Al-rich inclusions (CAIs) from the CK3 (Karoonda-type) carbonaceous chondrites NWA (Northwest Africa) 4964-#1 and -Homer, NWA 5343-#1, and LAR (Larkman Nunatak) 12002-#1. These CAIs experienced extensive metasomatic alteration: melilite and possibly anorthite and AlTi-diopside are nearly completely replaced by secondary corundum, grossular, CaNa-plagioclase, FeAl-diopside, and FeO-rich spinel; perovskite is largely replaced by ilmenite. Two types of corundum grains occur in the NWA 4964 CAIs: (1) compact, FeO-poor grains zoned in cathodoluminescent (CL) images and (2) FeO-bearing (up to 1.5 wt% FeO), porous grains showing no detectable CL; the porous corundum grains overgrow the compact ones. Corundum grains in CAIs from LAR 12002 and NWA 5343 belong to the first and second types, respectively. Hibonite, primary spinel, and rare perovskite inclusions in spinel retained the original, 16O-rich compositions (Δ17O ~ −24 ± 2‰), whereas melilite, most perovskite grains, and secondary corundum and spinel are 16O-depleted (Δ17O ~ −5 ± 2‰). Hibonite and melilite have excesses of radiogenic 26Mg (26Mg*) corresponding to approximately the canonical initial 26Al/27Al ratio [(26Al/27Al)0] of ~5 × 10−5 suggesting that corundum-bearing CAIs studied belong to a population of the canonical inclusions, dominant in most chondrite groups. Corundum grains in LAR 12002-#1, NWA 4964-#1, NWA 4964-Homer, and NWA 5343-#1 show resolvable 26Mg* correlated with 27Al/24Mg ratio which corresponds to much lower than the canonical (26Al/27Al)0: (3.10 ± 0.48) × 10−6, (3.03 ± 0.23) × 10−6, (2.72 ± 0.19) × 10−6, and (3.5 ± 1.2) × 10−7, respectively. Porous Fe-bearing corundum grains in NWA 4964 CAIs Homer and #1 have low 26Mg* not correlated with 27Al/24Mg ratio. We conclude that compact corundum grains in the CK3 CAIs studied are secondary parent body products that resulted from metasomatic alteration of the host inclusions by hydrothermal fluid ~3−5 Ma after their crystallization. Porous corundum grains may have formed by dehydration of diaspore [AlO(OH)] during subsequent thermal metamorphism.

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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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