Abundant microchondrules in 162173 Ryugu suggest a turbulent origin for primitive asteroids.

ABSTRACT: Chondrules are a characteristic feature of primitive Solar System materials and are common in all primitive meteorites except the CI-chondrites. They are thought to form owing to melting of solid dust aggregates by energetic processing within the solar nebula and thus record fundamental processes within protoplanetary disks. We report the discovery of abundant altered microchondrules (>350 ppm) with modal sizes of 6-8 µm within sample A0180 from C-type asteroid Ryugu. These microchondrules have similar log-normal size and shape distributions to normal-sized chondrules, implying evolution by similar size-sorting. We suggest here formation of microchondrules in an outer Solar System chondrule factory, located in the Jovian pressure-bump, followed by turbulent diffusion and concentration rela

SUBMITTER: Genge MJ 

PROVIDER: S-EPMC12287358 | biostudies-literature | 2025 Jul

REPOSITORIES: biostudies-literature