A Potůčky fragment of the Steinbach IVA-an meteorite: Implications from the trace-element composition of the constituent phases

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Alexandre V. Andronikov, Irina E. Andronikova, Ondrej Pour, Petr Bohdalek
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引用次数: 0

Abstract

We have analyzed in situ mineral phases in a Potůčky fragment of the stony-iron IVA-an meteorite Steinbach for trace-element compositions. The studied fragment contains silicate grains (pyroxene and tridymite) interspersed with grains of metal (kamacite, plessite, and taenite) displaying Widmanstätten pattern and troilite. Multiple inclusions of chromite, troilite, and bi-mineral troilite + taenite assemblages were observed within some pyroxene grains. The data on variations in trace-element compositions in different meteorite phases are consistent with a number of models, suggesting the involvement of several processes in the generation of the lithologies presently observed in the Potůčky meteorite. These processes might have involved fractional crystallization of silicate liquid, collision, impact, shock melting, and cooling. As a result of such processes, specific trace-element composition of different mineral phases was formed. Trace-element compositions of metals and sulfides from the Potůčky meteorite are very similar to those for minerals from the LL ordinary chondrite, suggesting LL-like asteroid as a parent body for the Potůčky (IVA-an) precursor material.

Steinbach IVA-an陨石的Potůčky碎片:组成相的微量元素组成的含义
我们在Steinbach石铁IVA-an陨石Potůčky碎片中原位分析了微量元素组成。所研究的碎片含有硅酸盐颗粒(辉石和钇铝石),点缀着金属颗粒(卡玛石、硅镁石和带长石),显示Widmanstätten模式和三辉石。在一些辉石颗粒中观察到铬铁矿、三黄铁矿和双矿物三黄铁矿+带长石组合的多个包裹体。关于不同陨石阶段微量元素组成变化的数据与许多模型一致,表明目前在Potůčky陨石中观察到的岩性的形成涉及几个过程。这些过程可能包括硅酸盐液体的分步结晶、碰撞、冲击、冲击熔化和冷却。这些过程形成了不同矿物相的特定微量元素组成。Potůčky陨石中金属和硫化物的微量元素组成与LL普通球粒陨石中矿物的微量元素组成非常相似,表明类似LL的小行星是Potůčky (IVA-an)前体物质的母体。
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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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