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Pervasive impact modification of pristine lunar clasts.
M Barboni1, E Needham2, D Trail3
1School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. mbarboni@asu.edu.
Nature Communications
|March 14, 2025
Summary
Pristine lunar rock fragments may not be pristine. New analysis shows zircons in these samples are not in equilibrium with their surroundings, indicating extensive impact reworking. Re-evaluating lunar sample origins is crucial.
Area of Science:
- Geochemistry
- Planetary Science
- Mineralogy
Background:
- Lunar rock fragments, especially pristine ones, are key to understanding Moon's formation and evolution.
- Traditionally, pristine samples were believed to have escaped significant impact history, preserving early lunar crustal information.
- The definition and identification of "pristine" lunar samples are increasingly questioned due to potential impact alteration.
Purpose of the Study:
- To critically assess lunar samples using a novel geochemical and experimental approach.
- To investigate the chemical equilibrium of zircons within lunar samples and their parent melt composition.
- To challenge the assumption that certain lunar samples represent primary igneous lithologies.
Main Methods:
- Application of a novel high-resolution geochemical and experimental approach.
- Linking aluminum (Al) content in zircon to parent melt composition.
- Analysis of clast and matrix zircons in brecciated lunar samples.
Main Results:
- Zircons from lunar samples (both clast and matrix) were found to be in chemical disequilibrium with their surrounding glass.
- Heterogeneous zircon ages further support evidence of significant impact reworking.
- The findings challenge the notion that these samples preserve pristine magmatic histories.
Conclusions:
- Lunar samples, even those considered pristine, show evidence of pervasive impact reworking.
- Traditional criteria for identifying pristine lunar samples may be insufficient.
- New analytical methods, like the Al-in-zircon technique, are essential for re-evaluating lunar materials and their formation history.
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