Mature lunar soils from Fe-rich and young mare basalts in the Chang’e-5 regolith samples

Space weathering on airless bodies produces metallic iron (Fe 0 ) particles in the rims of mineral grains, which affect visible and near-infrared spectra and complicate the identification of surface materials. The Chang’e-5 mission provides an opportunity to couple information gained from its returned samples with in situ observations and orbital monitoring to gain insight on the details of space weathering on extremely Fe-rich basalts. By putting together all these data, we could extract a soil maturity index ( I s /FeO) at the Chang’e-5 landing site of ~66 ± 3.2, indicative of a formation age for the Xu Guangqi crater, whose ejecta dominate the site, of 240–300 Myr ago. In addition, abundant large Fe 0 particles were found in the sample, indicating that both the inherited Fe 0 particles from late-stage mare basalts and the dense clustering of oversaturated Fe 0 in extremely FeO-rich (>17 wt%) basalts contribute to observed Fe 0 abundances. We suggest that space weathering of Fe-richer basalt generates Fe 0 particles with a larger grain size and faster production rate. A multi-observational study including laboratory analysis of the Chang’e-5 mission samples, in situ measurements and orbital datasets determined the high level of maturity and iron content of the Chang’e-5 landing site regolith. Heavily processed by space weathering, it mostly comes from the nearby Xu Guangqi crater, formed 240–300 Myr ago.