AbstractMicroscopic silicate melts are ubiquitous on surfaces of lunar regolith particles, and they record physicochemical processes of regolith reworking on the Moon. Similar microstructures are visible on surfaces of the Chang'e‐5 lunar impact glass particles, which are predominantly sourced from local mare deposits. Therefore, the microscopic silicate melts provide an invaluable opportunity to study the movements, provenances, and chemical alterations of substances involved in regolith reworking. However, the small lateral sizes and thicknesses of the surface silicate melts are a challenge for quantifying their internal structures and geochemical compositions, hampering interpretations of their origin. Here we report structural and geochemical characteristics for microscopic silicate pancakes, domes and foams on surfaces of Chang'e‐5 impact glass particles. Based on the contact and compositional differences between the surface microscopic silicate melts and their host glass, we reveal that these microstructures are consistent with being formed during impact bombardment in regolith via adhesion of impact melts to earlier‐existing glasses. Most of the microscopic silicate melts have minor compositional differences with the host glass. Our mixing calculations for compositions of impact melt formed from various proportions of local regolith minerals at the landing site reveal a dominant precursor from the local mare deposits. Few portions of the microscopic silicate melts have exotic compositions that are different from the local regolith materials, confirming that ejecta from the other geochemical terrains is minor at the landing site. Our results show that regolith formation and reworking at the Chang'e‐5 sampling site mainly involved local mare deposits.
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