High-resolution cathodoluminescence of calcites from the Cold Bokkeveld chondrite: New insights on carbonatation processes in CM parent bodies

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Meteoritics & Planetary Science Pub Date : 2024-06-11 DOI:10.1111/maps.14225
Vincent Guigoz, Anthony Seret, Marc Portail, Ludovic Ferrière, Guy Libourel, Harold C. Connolly Jr, Dante S. Lauretta
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Abstract

Carbonates, as secondary minerals found in CM chondrites, have been widely employed for reconstructing the composition of the fluids from which they precipitated. They also offer valuable insights into the hydrothermal evolution of their parent bodies. In this study, we demonstrate that high-resolution cathodoluminescence (HR-CL) analyses of calcites derived from the brecciated Cold Bokkeveld CM2 chondrite can effectively reveal subtle compositional features and intricate zoning patterns. We have identified two distinct types of cathodoluminescence (CL) centers: a blue emission band (approximately 375–425 nm), associated with intrinsic structural defects, and a lower energy orange extrinsic emission (around 620 ± 10 nm), indicating the presence of Mn cations. These compositional variations enable discrimination between the calcite grain types previously designated as T1 and T2 in studies of CM chondrites. T1 calcites exhibit variable CL and peripheral Mn enrichments, consistently surrounded by a rim composed of Fe-S-rich serpentine–tochilinite assemblage. Conversely, T2 calcites display homogeneous CL and more abundant lattice defects. These polycrystalline aggregates of calcite grains, devoid of serpentine, contain Fe-Ni sulfide inclusions and directly interface with the matrix. We propose that changes in the Mn content of calcite (indicated by the intensity of orange CL emission) are influenced by variations in redox potential (Eh) and pH of the fluid phase. This proposed hydrothermal evolution establishes a parallel between terrestrial serpentinization followed by carbonation processes and the aqueous alteration of CM chondrites, warranting further exploration and investigation of this intriguing similarity.

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Cold Bokkeveld软玉中方解石的高分辨率阴极发光:CM 母体碳化过程的新见解
碳酸盐作为在 CM 软骨岩中发现的次生矿物,已被广泛用于重建析出碳酸盐的流体成分。它们还为了解母体的热液演化提供了宝贵的信息。在这项研究中,我们证明了对来自角砾化Cold Bokkeveld CM2软玉的方解石进行高分辨率阴极发光(HR-CL)分析,可以有效地揭示微妙的成分特征和复杂的分带模式。我们发现了两种不同类型的阴极发光(CL)中心:一种是蓝色发射带(约 375-425 纳米),与内在结构缺陷有关;另一种是能量较低的橙色外发射(约 620±10 纳米),表明存在锰阳离子。通过这些成分变化,可以区分以前在 CM 软骨岩研究中被指定为 T1 和 T2 的方解石晶粒类型。T1 方解石显示出不同的 CL 和外围富锰矿,周围始终围绕着富含 Fe-S 的蛇纹石-蛭石集合体。相反,T2钙钛矿显示出均匀的CL和更丰富的晶格缺陷。这些方解石颗粒的多晶聚集体不含蛇纹石,含有铁-镍硫化物包裹体,并直接与基质相接。我们提出,方解石中锰含量的变化(以橙色 CL 发射强度表示)受流体相氧化还原电位(Eh)和 pH 值变化的影响。这种拟议的热液演化过程在陆地蛇纹石化和碳化过程与 CM 软骨的水蚀变之间建立了平行关系,值得进一步探索和研究这种有趣的相似性。
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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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