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Compositional Variations in the Vicinity of the Lunar Crust-Mantle Interface From Moon Mineralogy Mapper Data.
M Martinot1,2, J Flahaut3, S Besse4
1Faculty of Science, Vrije Universiteit Amsterdam Amsterdam The Netherlands.
This study analyzed lunar impact craters using Moon Mineralogy Mapper data to understand the crust-mantle interface. Mineral variations suggest depth-related compositional changes and deep lateral heterogeneities within the Moon.
Area of Science:
- Lunar geology
- Planetary science
- Mineralogy
Background:
- The Moon's crust-mantle interface is poorly understood.
- Impact craters offer windows into the lunar subsurface.
Purpose of the Study:
- Investigate the mineralogy of lunar impact crater central peaks and peak rings.
- Characterize the lunar crust-mantle interface and its heterogeneity.
- Assess the depth of origin for materials within these structures.
Main Methods:
- Utilized Moon Mineralogy Mapper (M3) spectroscopic data.
- Calculated crater central peak/ring depths using empirical equations.
- Compared depths with Gravity Recovery and Interior Laboratory (GRAIL) crustal thickness models.
Main Results:
- Plagioclase is widespread; Low-Calcium Pyroxene found in central peaks.
- Olivine detections are scarce, found both above and below the crust-mantle interface.
- Pyroxene composition evolves with depth, suggesting crust-to-mantle transition.
- High-Calcium Pyroxene correlates with maria, indicating deep lateral heterogeneities.
Conclusions:
- Lunar crustal and mantle materials exhibit distinct mineralogical signatures.
- Impact craters provide crucial insights into deep lunar structure.
- Evidence suggests significant lateral variations exist at the crust-mantle boundary.
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