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Target rocks, impact glasses, and melt rocks from the Lonar crater, India: Highly siderophile element systematics and Sr-Nd-Os isotopic signatures

机译:印度Lonar火山口的目标岩石,冲击玻璃和融化岩石:高度嗜铁元素元素系统和Sr-Nd-Os同位素特征

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摘要

The Lonar crater is a similar to 0.57-Myr-old impact structure located in the Deccan Traps of the Indian peninsula. It probably represents the best-preserved impact structure hosted in continental flood basalts, providing unique opportunities to study processes of impact cratering in basaltic targets. Here we present highly siderophile element (HSE) abundances and Sr-Nd and Os isotope data for target basalts and impactites (impact glasses and impact melt rocks) from the Lonar area. These tools may enable us to better constrain the interplay of a variety of impact-related processes such as mixing, volatilization, and contamination. Strontium and Nd isotopic compositions of impactites confirm and extend earlier suggestions about the incorporation of ancient basement rocks in Lonar impactites. In the Re-Os isochron plot, target basalts exhibit considerable scatter around a 65.6Myr Re-Os reference isochron, most likely reflecting weathering and/or magma replenishment processes. Most impactites plot at distinctly lower Re-187/Os-188 and Os-187/Os-188 ratios compared to the target rocks and exhibit up to two orders of magnitude higher abundances of Ir, Os, and Ru. Moreover, the impactites show near-chondritic interelement ratios of HSE. We interpret our results in terms of an addition of up to 0.03% of a chondritc component to most impact glasses and impact melt rocks. The magnitude of the admixture is significantly lower than the earlier reported 12-20 wt% of extraterrestrial component for Lonar impact spherules, reflecting the typical difference in the distribution of projectile component between impact glass spherules and bulk impactites.
机译:Lonar陨石坑类似于位于印度半岛Deccan陷阱中的具有0.57年历史的撞击结构。它可能代表了大陆洪水玄武岩中保存最完好的撞击结构,为研究玄武岩目标撞击坑的过程提供了独特的机会。在这里,我们介绍了来自Lonar地区的目标玄武岩和撞击矿(撞击玻璃和撞击熔岩)的高度嗜铁元素(HSE)丰度以及Sr-Nd和Os同位素数据。这些工具可以使我们更好地限制各种与冲击相关的过程(例如混合,挥发和污染)的相互作用。陨石的锶和Nd同位素组成证实并扩展了关于在月球陨石中掺入古代基底岩石的早期建议。在Re-Os等时线图中,目标玄武岩在65.6Myr Re-Os参考等时线周围表现出相当大的分散性,很可能反映了风化和/或岩浆补充过程。与目标岩石相比,大多数冲积岩以明显较低的Re-187 / Os-188和Os-187 / Os-188比绘制,并且Ir,Os和Ru的丰度高出两个数量级。此外,这些膨润土显示出HSE的近晶间元素比率。我们将结果解释为在大多数冲击玻璃和冲击熔岩中最多添加0.03%的软骨素成分。该混合物的量级显着低于较早前报道的月球撞击小球的地外成分的12-20 wt%,这反映了撞击玻璃小球与块状撞击石之间弹丸成分分布的典型差异。

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