CM chondrite Reckling Peak 17085中的早期流体迁移和蚀变前沿

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Meteoritics & Planetary Science Pub Date : 2024-09-02 DOI:10.1111/maps.14261
A. Musolino, M. D. Suttle, L. Folco, A. J. King, G. Poggiali, H. C. Bates, J. R. Brucato, A. Brearley
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摘要

Reckling Peak(RKP)17085 是一块新分类的南极 CM 陨石,它保存了复杂的蚀变历史,其特征是轻度水蚀变(CM2.7),被短暂的热变质事件(加热阶段 III [<750°C])所覆盖,并受到低级陆地风化的影响。这块陨石的细粒基质中含有丰富的富铁带,由微米级的铁氧氢氧化物矿物组成。它们被解释为 "蚀变前沿",是由于铁(通常为 500 μm)在突然沉积前的溶解和迁移而产生的。这种蚀变纹理在水合碳质软玉中较为罕见,迄今为止仅有五例报道(默奇森、默里、艾伦山81002、米勒山脉07687和西北非5958)。来自 RKP 17085 的证据表明,早期的水蚀变是作为多个地球化学上孤立的微环境运作的,这些微环境从基质内的局部点源向外移动。软玉上的低渗透性细粒边缘似乎是流体流动的障碍,控制着流体在母体中的迁移。此外,蚀变细粒基质中孔隙率较高的区域要么是水化后变质过程中水合矿物脱水产生的空隙空间,要么是保留在轻度蚀变原始基质中的冰吸积点(水冰或含C冰)。
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Early fluid migration and alteration fronts in the CM chondrite Reckling Peak 17085

Reckling Peak (RKP) 17085 is a newly classified Antarctic CM chondrite that preserves a complex alteration history characterized by mild aqueous alteration (CM2.7), overprinted by a short-lived thermal metamorphic event (heating stage III [<750°C]), and affected by low-grade terrestrial weathering. This meteorite contains abundant Fe-rich bands within the fine-grained matrix, composed of micron-scale Fe-oxyhydroxide minerals. They are interpreted as “alteration fronts” arising due to the dissolution and transport of Fe (typically <500 μm) before being abruptly deposited. This alteration texture is relatively rare among hydrated carbonaceous chondrites, with only five reported instances to date (Murchison, Murray, Allan Hills 81002, Miller Range 07687, and Northwest Africa 5958). Evidence from RKP 17085 suggests that early aqueous alteration operated as multiple geochemically isolated microenvironments, which moved outwards from local point sources within the matrix. Low permeability fine-grained rims on chondrules appear to have acted as barriers to fluid flow, controlling the migration of fluid across the parent body. Furthermore, the higher porosity regions within the altered fine-grained matrix represent either void space generated by the dehydration of hydrated minerals during post-hydration metamorphism and/or sites of ice accretion (water-ice or C-bearing ices) preserved within a mildly altered primitive matrix.

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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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Issue Information Cover Constraints on the impact history of the Apollo 16 landing site: Implications of soil-like breccia noble gas records Issue Information Cover
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