Articlenpj space exploration2026
Remanent crustal strain on Mars in non-poikilitic olivine of NWA 7721.
Article in npj space exploration, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.
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8 authors.
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Abstract
We present a multiscale, non-destructive analysis of non-poikilitic olivine in the shergottite NWA 7721 using dark-field X-ray microscopy, electron backscatter diffraction, and 2D micro-X-ray diffraction. We report striking bimodal microstructures within a single olivine crystal: fine Type 1 subgrains (around 5 μm), weakly oriented, and nearly strain-free; coarser Type 2 subgrains (>15 μm), aligned, and strongly strained. Layered DFXM data reveal slip-band features in Type 2 that are absent in Type 1. This bimodal microstructure, not observed in other Martian meteorites, including the paired NWA 1950 and ALH A77005, points to a heterogeneous response to impact at the crystallographic scale. We interpret Type 1 as shock-assisted recrystallites and Type 2 as relic partitioned from a highly deformed parental grain with a pre-existing fabric. The subsequent shock wave imposed a rapid load-release cycle that generated heterogeneous deformation within the crystal. Highly strained regions underwent recrystallization to form Type 1 subgrains, whereas less-strained domains retained deformation structures as Type 2. Grain-growth constraints limit the post-shock heating to ≈2.3 s, consistent with rapid quenching. Together, these observations illustrate a dynamic Martian crustal activity in the Late Amazonian and demonstrate DFXM, combined with EBSD and micro-XRD, as a promising tool for resolving complex fabrics in 3D.
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