The first natural occurrence of ringwoodite lamellae was found in the olivine grains inside and in areas adjacent to the shock veins of a chondritic meteorite, and these lamellae show distinct growth mechanism. Inside the veins where pressure and temperature were higher than elsewhere, ringwoodite lamellae formed parallel to the {101} planes of olivine, whereas outside they lie parallel to the (100) plane of olivine. The lamellae replaced the host olivine from a few percent to complete. Formation of these lamellae relates to a diffusion-controlled growth of ringwoodite along shear-induced planar defects in olivine. The planar defects and ringwoodite lamellae parallel to the {101} planes of olivine should have been produced in higher shear stress and temperature region than that parallel to the (100) plane of olivine. This study suggests that the time duration of high pressure and temperature for the growth of ringwoodite lamellae might have lasted at least for several seconds, and that an intracrystalline transformation mechanism of ringwoodite in olivine could favorably operate in the subducting lithospheric slabs in the deep Earth. N atural ringwoodite had been found in many shocked chondritic meteorites, in which the ringwoodite occurs as finegrained polycrystalline aggregates formed through a phase transition of olivine during exogenous dynamic events on the parent asteroids (1-4). It was also suggested that the olivineringwoodite transformation could take place in cold subducting slabs at the deep transition zone, where pressure oversteps the ringwoodite stability field (5-9). An experiment-produced texture characteristic of this phase transition in the slabs is the formation of ringwoodite lamellae within individual olivine crystals (6,7,(10)(11)(12). A number of laboratory experiments on compositions like Mg 2 GeO 4 , Fe 2 SiO 4 , and (Mg,Fe) 2 SiO 4 showed that the spinel-structured lamellae lie parallel to the (100) planes of olivine (6,(10)(11)(12)(13)(14)(15)(16)(17)(18). These ringwoodite lamellae form platelets from several unit cells to 100 nm in thickness (6,(10)(11)(12)(14)(15)(16)(17)(18). The formation of ringwoodite lamellae in olivine was attributed either to a martensitic transformation mechanism (6,13,(15)(16)(17)(18)(19) or an intracrystalline nucleation and growth mechanism by which coherent nucleation of ringwoodite occurs on the stacking faults of olivine (10-12). However, no natural occurrence of ringwoodite lamellae had been found so far either in the shocked meteorites or exhumed subducted slabs.Sixiangkou meteorite is a heavily shock-metamorphosed L6-chondrite with a number of shock-produced veins up to 10 mm in thickness. The shock veins contain abundant high-pressure minerals including ringwoodite, majorite, garnet, and magnesiowüstite, for which the shock-produced pressure and temperature of Ϸ20 GPa and 2,000°C were inferred (4). Polycrystalline aggregates of ringwoodite and majorite up to 100 m in size and porphyroclastic grains of olivine and pyroxene up to 1.5 mm in size distr...