The compositional classification of chondrites. IV - Ungrouped chondritic meteorites and clasts

Computer Science

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Chondrites, Meteoritic Composition, Petrography, Sediments, Chemical Composition, Classifications, Neutron Activation Analysis, Recrystallization, Textures, Meteorites, Chondrites, Composition, Classification, Samples, Meteorite, Clasts, Neutron Activation Analysis, Recrystallization, Texture, Enon, Cumberland Falls, Metamorphism, Acapulco, Ll Chondrites, Tierra Blanca, Antarctic Meteorites, Unequilibrated Ordinary Chondrites, Iab Meteorites, Allan Hills Meteorites, Alha77081, Comparisons, Udei Station, Iso

Scientific paper

INAA and RNAA are used to determine the abundances of 30 elements in the unusual chondrites Acapulco (A), Allan Hills A77081 (AH), Cumberland Falls (CF), Enon, Tierra Blanca (TB), and Udei Station (US). The results are presented in tables and graphs and characterized in detail. A, AH, and Enon are grouped together on the basis of their subpristine composition; US is classified as IAB; TB is found to have an altered composition with evidence of phosphate-phase loss like US but is left ungrouped due to its high delta-(O-18); and CF is found to resemble the LL chondrites, with evidence of in situ reduction by exchange with the aubritic host.

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