“…Kallemeyn et al (1991) applied some of the petrographic criteria used in studies of ordinary chondrite to carbonaceous chondrites, including: 1) homogeneity of olivine composition, 2) mean diameter of plagioclase, 3) presence or absence of primary glass, 4) chondrule delineation, and 5) coarseness of ground mass grains, and suggested that CK chondrites form a metamorphic sequence, as observed in ordinary Structural state of plagioclase from the Kobe CK chondrite chondrites. Tomeoka et al (2005) analyzed the Kobe meteorite and found that olivine crystals have homogeneous compositions (standard deviation of Fa content = 0.4), grain sizes of plagioclase typically range from 50 to 150 μm, primary glass is absent, chondrules are moderately defined to well defined, and the grain size of matrix olivine is typically 5 30 μm. Based on the latter two criteria, the authors concluded that a CK4 classification is most appropriate for the Kobe meteorite, although the grain size of plagioclase is consistent with a type 6 classification (Kallemeyn et al, 1991).…”