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This study utilizes imaging spectroscopy data to analyze the spectral diversity and compositional characteristics of the Mare Serenitatis/Tranquillitatis region on the Moon. The research identifies basaltic units with varying titanium content and employs clustering techniques to produce mineralogical maps, enhancing the understanding of lunar surface composition. The findings indicate significant spectral heterogeneity in the region, contributing to the broader mapping efforts of the Moon
- Author
- Kajal Kumari
- Language
- EN