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Data · dataset · 2026

Microscopic slickenside as a record of weak shock metamorphism in the surface layer of asteroid Ryugu [* Cross-Reference *]

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The surface morphology of regolith grains from the C-type asteroid Ryugu was studied in search of evidence of impact events on the asteroid.

Description

Scanning electron microscopy revealed that ~8% of C0105-042 Ryugu grains have a smooth surface on one side of the grains. One of these grains has striated linear grooves (striations) on its smooth surface.

Transmission electron microscopy of the grain showed that a porous fine-grained Mg-Fe phyllosilicate assemblage, which is the main component of Ryugu grains, is compacted near the smooth surface. The smooth surface with striations closely resembles a slickenside, a characteristic texture found in terrestrial fault rocks formed by shear deformation. There is no evidence of melting/decomposition in the Mg-Fe phyllosilicates near the smooth surface, indicating that the shear heating temperature is less than ~1100 K. Assuming that the average length of the striations corresponds to the minimum displacement of the micro-fault, the shock pressure recorded in the C0105-042 Ryugu grain is estimated to be <~4.5 GPa by a fault mechanics calculation.

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The shock pressures of C0105-042, together with those of C0014 (~2 GPa) and C0055 (>~3.9 GPa) in previous studies suggest that the impact velocities recorded in these grains are < ~0.89–1.63 km s−1. Based on the impact velocities, these grains may record an impact event that occurred when asteroid Ryugu was in the orbit in Main Belt. ***This entry has been automatically imported via Infodoc(ASO) CSV by LIST harvest scripts.

Please refer to doi.org/10.1111/maps.14271 for the original and latest version of the dataset and data downloads***

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Microscopy 75%
Provenance · 1 source records, 9 field assertions
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concepts[modality].local:modality:microscopyenrichment · lore list lukeyword-concept-rules@1.0.0title+description (75%)
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