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Figure1.pptx

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DataCite Commons2023-10-27 更新2025-04-15 收录
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Thin section Dhofar 1769 (PL15019) studied at the Institut für Planetologie (Münster). The lunar regolith breccia contains abundant large, light-colored lithic clasts and the dark IMB (which is the IM-3 lithology of the present study) embedded in a fine-grained clastic matrix. Data on the dark IMB with one particular impact melt fragment (arrow; see Figure 2) are discussed in this study. Image in transmitted light. (Color figure can be viewed at wileyonlinelibrary.com) [Colour figure can be viewed at wileyonlinelibrary.com]
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