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Potassium Map from ChangE-2 Constraints the Impact of Crisium and Orientale Basin on the Moon

机译:Chang娥二号的钾离子图限制了Crisium和Orientale盆地对月球的影响

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摘要

KREEP materials were thought to be last crystallized at the lunar crust and mantle boundary. Impact cratering and volcanism are mainly responsible for their distributions on the lunar surface. Therefore, observation of global KREEP materials and investigation of distributions in the areas of large basins are of critical importance to understand the geologic history of the Moon. Here we report the new global potassium distribution on the Moon detected by Chang'E-2 Gamma-ray Spectrometer. We found that our new measurements are in general agreement with previous observation. A new finding and an important difference is that relatively higher K abundances in the Mare Crisium and Mare Orientale than their surrounding rims were detected for the first time. In light of our observations in these two areas, we propose that Crisium and Orientale basin-forming impact events may have penetrated to the lower crust and excavate the deeper materials to the lunar surface.
机译:人们认为KREEP材料最后在月球地壳和地幔边界处结晶。撞击坑和火山作用是造成月球表面分布的主要原因。因此,对全球KREEP资料的观察以及对大盆地区域分布的调查对于了解月球的地质历史至关重要。在这里,我们报告由Chang娥二号伽玛射线光谱仪探测到的新的全球钾在月球上的分布。我们发现我们的新测量值与先前的观察结果基本一致。一个新发现和一个重要区别是,首次发现母马Crisium和母马东方树中的K丰度比其周围的轮缘高。根据我们在这两个区域的观察结果,我们建议形成Crisium和Orientale盆地的撞击事件可能已经渗透到下地壳,并将较深的物质挖掘到月球表面。

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