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Shocked chromites in fossil L chondrites: A Raman spectroscopy and transmission electron microscopy study
Author(s) -
Rout Surya S.,
Heck Philipp R.,
Zaluzec Nestor J.,
Ishii Takayuki,
Wen Jianguo,
Miller Dean J.,
Schmitz Birger
Publication year - 2017
Publication title -
meteoritics and planetary science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.09
H-Index - 100
eISSN - 1945-5100
pISSN - 1086-9379
DOI - 10.1111/maps.12887
Subject(s) - chondrite , chromite , meteorite , geology , parent body , chondrule , shock metamorphism , raman spectroscopy , geochemistry , mineralogy , matrix (chemical analysis) , astrobiology , materials science , composite material , optics , physics
Chromites from Middle Ordovician fossil L chondrites and from matrix and shock‐melt veins in Catherwood, Tenham, and Coorara L chondrites were studied using Raman spectroscopy and TEM . Raman spectra of chromites from fossil L chondrites showed similarities with chromites from matrix and shock‐melt veins in the studied L chondrite falls and finds. Chromites from shock‐melt veins of L chondrites show polycrystallinity, while the chromite grains in fossil L chondrites are single crystals. In addition, chromites from shock‐melt veins in the studied L chondrites have high densities of planar fractures within the subgrains and many subgrains show intergrowths of chromite and xieite. Matrix chromite of Tenham has similar dislocation densities and planar fractures as a chromite from the fossil meteorite Golvsten 001 and higher dislocation densities than in chromite from the fossil meteorite Sextummen 003. Using this observation and knowing that the matrix of Tenham experienced 20–22 GP a and <1000° C, an upper limit for the P,T conditions of chromite from Golvsten 001 and Sextummen 003 can be estimated to be 20–22 GP a and 1000° C (shock stage S3–S6) and 20 GP a and 1000° C (S3–S5), respectively, and we conclude that the studied fossil meteorite chromites are from matrix.