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Mineralogy, petrology and geochemistry of carbonaceous chondritic clasts in the LEW 85300 polymict eucrite
Author(s) -
Zolensky M. E.,
Hewins R. H.,
Mittlefehldt D. W.,
Lindstrom M. M.,
Xiao X.,
Lipschutz M. E.
Publication year - 1992
Publication title -
meteoritics
Language(s) - English
Resource type - Journals
eISSN - 1945-5100
pISSN - 0026-1114
DOI - 10.1111/j.1945-5100.1992.tb01082.x
Subject(s) - geology , geochemistry , clastic rock , petrology , astrobiology , sedimentary rock , physics
— We have performed a detailed petrologic and mineralogic study of two chondritic clasts from the polymict eucrite Lewis Cliff (LEW) 85300, and performed chemical analyses by INAA and RNAA on one of these. Petrologically, the clasts are identical and are composed of dispersed aggregates, chondrules and chondrule fragments supported by matrix. The aggregates and chondrules are composed of olivine (Fo 100–45 ), orthopyroxene (Wo 1–2 En 98–60 ), plus some diopside. The matrix consists of fine‐grained olivine (Fo 60–53 ), and lesser orthopyroxene and augite. Fine‐grained saponite is common in the matrix. The bulk major element composition of the matrix is identical in both clasts and similar to that of CM, CO and CV chondrites. The bulk composition of the clast studied by INAA and RNAA shows unusual abundance patterns for lithophile, siderophile and chalcophile elements but is basically chondritic. The INAA/RNAA data preclude assignment of the LEW 85300,15 clast to any commonly accepted group of carbonaceous chondrite. The unusual rare earth element abundance pattern may, in part, be due to terrestrial alteration.