Incompatible trace element geochemistry of the anorthositic achondrite Northwest Africa (NWA) 15118: Relation to diogenites and the Vestan magma ocean

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
A. I. Sheen, K. T. Tait, V. E. Di Cecco, B. R. Joy, C. J. Bray
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引用次数: 0

Abstract

Petrogenetic models for the howardite–eucrite–diogenite (HED) clan of achondrites have been challenged by the lack of substantial plagioclase in the HED record, which is at odds with the chemical composition of diogenites. Northwest Africa (NWA) 15118, an anorthositic achondrite, displays strong isotopic affinities with HEDs and has been proposed as a lunar-style primary flotation crust of the Vestan magma ocean. Nevertheless, a geochemical link with known HEDs, particularly diogenites, remains to be demonstrated. We present major, minor, and trace element data for plagioclase and orthopyroxene in NWA 15118. Despite textural evidence for post-crystallization shock and thermal metamorphism, transect major and minor element data reveal that igneous crystallization trends are preserved. Normalized trace element data reveal depletion in Ti, Nb, Hf, Zr in plagioclase and corresponding enrichment in orthopyroxene. Orthopyroxene in NWA 15118 does not plot on the Y versus Ti array formed by diogenite orthopyroxenes, which have a higher Ti/Y ratio. The calculated melt composition in equilibrium with NWA 15118 plagioclase has lower Ti/Y, Ti/Yb, and La/Sm ratios than melts in equilibrium with diogenite orthopyroxenes; differences in the melt compositions cannot be accounted for by the choice of partition coefficients or by single-stage magmatic processes. Therefore, we argue that NWA 15118 and diogenites are not complementary cumulates that crystallized simultaneously from a global Vestan magma ocean. Furthermore, the modeled evolution curve of such a magma ocean does not produce the composition of NWA 15118 plagioclase equilibrium melts in Ti-Y-Yb space, indicating that NWA 15118 is unlikely to have been a primary flotation crust of a global magma ocean. Our findings suggest that the incompatible trace element composition of NWA 15118 likely reflects more complex, multistage magmatic processes and/or source heterogeneities than envisioned in geochemistry-based HED petrogenetic models proposed to date.

Abstract Image

西北非洲斜长无球粒岩(NWA) 15118的不相容微量元素地球化学:与Vestan岩浆海和闪长岩的关系
非球粒陨石howardite - eucite - diogenite (HED)族的岩石成因模式受到了挑战,因为HED记录中缺乏大量斜长石,这与diogenites的化学成分不一致。西北非洲(NWA) 15118是一种与HEDs具有较强同位素亲和力的斜长无球粒岩,被认为是Vestan岩浆海的月球型原生浮壳。然而,地球化学上与已知的HEDs,特别是diogenites的联系仍有待证明。我们给出了NWA 15118中斜长石和正辉石的主、次和微量元素数据。尽管存在结晶后冲击和热变质作用的结构证据,但样条主微量元素数据显示火成岩结晶趋势得到保留。归一化微量元素数据显示,斜长石中Ti、Nb、Hf、Zr富集,正辉石中Ti、Nb、Hf、Zr富集。NWA 15118中的正辉石没有绘制在由具有较高Ti/Y比值的闪长岩正辉石组成的Y / Ti阵列上。计算得到的NWA 15118斜长石平衡熔体的Ti/Y、Ti/Yb和La/Sm比值低于与闪长岩正辉石平衡熔体;熔体成分的差异不能用分割系数的选择或单阶段岩浆作用来解释。因此,我们认为NWA 15118和深成岩并不是在全球Vestan岩浆海洋中同时结晶的互补堆积。此外,该岩浆海的模拟演化曲线并没有得到NWA 15118斜长石平衡熔体在Ti-Y-Yb空间的组成,表明NWA 15118不太可能是全球岩浆海的初级浮选壳。我们的研究结果表明,NWA 15118的不相容微量元素组成可能反映了比迄今为止基于地球化学的HED岩石成因模型所设想的更复杂、多阶段的岩浆过程和/或源非均质性。
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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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