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The Kaidun chondrite breccia: Petrology, oxygen isotopes, and trace element abundances |
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| Authors: | Glenn J MacPherson David W Mittlefehldt Michael E Lipschutz Robert N Clayton Emma S Bullock Andrei V Ivanov Toshiko K Mayeda Ming-Sheng Wang |
| Institution: | a Dept. of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560-0119, USA b NASA Johnson Space Center, Mail Code KR, Houston, TX 77058, USA c Dept. of Chemistry, BRWN/WTHR Chemistry Bldg., 560 Oval Dr., Purdue University, W. Lafayette, IN 47907-2084, USA d Enrico Fermi Inst., 5640 S. Ellis Ave., University of Chicago, Chicago, IL 60637, USA e Vernadsky Inst. of Geochemistry and Analytical Chemistry, Kosygin St. 19, Moscow 119991, Russia |
| Abstract: | Oxygen isotope and trace element data for 13 samples of the Kaidun chondritic breccia reaffirm the complex polymict nature of this unique meteorite. Bulk Kaidun samples most closely resemble CR chondrites, but the matrix is CI-like. Two separated clasts are CR-like but have some properties that resemble CM, two clasts are enstatite chondrites (one EL and one EH), one clast is an aubrite-like metal-rich impact melt, and one clast is a unique layered olivine-bearing pyroxenite with the isotopic composition of an aubrite. Yet, although each clast resembles a known meteorite group, all deviate in some respect from the norms for those groups. Collectively, Kaidun has sampled materials not yet represented in the world meteorite collections and which greatly extend the definitions of known meteorite groups. Phyllosilicates in Kaidun span a very wide range in composition and vary from clast to clast, suggesting that the aqueous alteration experienced by the clasts predated assembly of the Kaidun parent body. |
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