Affiliation:
1. State Key Laboratory of Lunar and Planetary Sciences Macau University of Science and Technology Taipa China
2. College of Earth Science Guilin University of Technology Guilin China
3. Center for Lunar and Planetary Sciences Institute of Geochemistry Chinese Academy of Sciences Guiyang China
4. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China
5. Astronomical Research Center Shanghai Science & Technology Museum Shanghai China
Abstract
AbstractThe diverse microstructures of Fe‐Ni metal in 10 L groups ordinary chondrites that experienced progressive shock alteration were investigated using the electron backscattered diffraction technique. Through a combination of metallography and a silicate‐based shock classification scheme, we established the shock metamorphic features of metal phases corresponding to particular impact stages. In weakly shocked chondrites (S1–S2), the interlaced Neumann bands occur in polycrystalline kamacite, resulting from multiple small impact events on its parent body, and the internal crystallographic orientation difference of each kamacite monocrystal exceeds 5°. In moderately shocked samples (S2–S4), partial austenitization of metal occurs, accompanied by the emergence of net plessite. In strongly shocked samples (S4–S6), the metal has undergone complete austenitization and transformed into a homogenous fcc phase. In subsequent different cooling processes, polycrystalline kamacite with consistent internal crystallographic orientation, martensite, pearlitic plessite, duplex plessite, and acicular plessite form and finally appear in L group chondrites. This study demonstrates the significant utility of the microstructure of metal phases as a valuable tool for both the shock classification of L chondrites and the determination of shock metamorphism stages in iron meteorites.
Publisher
American Geophysical Union (AGU)