Experimentally induced troilite melt pervasion in chondritic analog materials: A study for FeNi-FeS darkening in chondrites

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Juulia-Gabrielle Moreau, Argo Jõeleht, Aleksandra N. Stojic, Christopher Hamann, Felix E. D. Kaufmann, Peeter Somelar, Jüri Plado, Satu Hietala, Tomas Kohout
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Abstract

Iron sulfide and metal melt veins in chondritic materials are associated with advanced stages of dynamic shock. The shock-induced residual temperatures liquefy the sulfide component and enable melt distribution. However, the distribution mechanism is not yet fully understood. Capillary forces are proposed as agents of melt distribution; yet, no laboratory experiments were conducted to assess the role that capillary forces play in the redistribution of iron sulfide in post-shock conditions. To investigate this further, we conducted thermal experiments under reducing conditions (N2(g)) using dunitic fragments, suitable chondritic analog materials that were doped with synthesized troilite (stoichiometric exact FeS). We observed extensive iron sulfide (troilite) migration that partially resembles that of ordinary chondrites, without the additional influence of shock pressure-induced fracturing. The iron sulfide melt infiltrated grain boundaries and pre-existing fractures that darkened the analog material pervasively. We also observed that the iron sulfide melt, which mobilized into grain boundaries, got systematically enriched in Ni from the surrounding host olivine. Consequently, FeNi metal fractionated from the melt in several places. Our results indicate that capillary forces majorly contribute to melt migration in the heated post-shock environment.

软玉类似物中实验诱导的特罗拉熔体侵蚀:对软玉中铁镍铁硫变暗的研究
球粒状物质中的硫化铁和金属熔体脉与动态冲击的晚期阶段有关。冲击引起的残余温度液化了硫化物成分,使熔体分布成为可能。然而,其分布机制尚不完全清楚。提出毛细管力是影响熔体分布的因素;然而,没有进行实验室实验来评估毛细力在冲击后条件下硫化铁重新分配中的作用。为了进一步研究这一点,我们在还原条件下(N2(g))使用双晶碎片进行了热实验,这是一种合适的球粒状模拟材料,掺杂了合成的三亚石(化学计量精确FeS)。我们观察到广泛的硫化铁(troilite)迁移,部分类似于普通球粒陨石,没有额外的冲击压力诱导压裂的影响。硫化铁熔体渗透到晶界和原有的裂缝中,使模拟材料普遍变暗。硫化铁熔体运移到晶界,系统地从周围的寄主橄榄石中富集镍。结果,镍金属在几个地方从熔体中分离出来。我们的研究结果表明,毛细力主要有助于熔体在加热后冲击环境中的迁移。
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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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