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Khatyrka,a new CV3 find from the Koryak Mountains,Eastern Russia
Authors:Glenn J MacPherson  Christopher L Andronicos  Luca Bindi  Vadim V Distler  Michael P Eddy  John M Eiler  Yunbin Guan  Lincoln S Hollister  Alexander Kostin  Valery Kryachko  William M Steinhardt  Marina Yudovskaya  Paul J Steinhardt
Institution:1. Department of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, , Washington, District of Columbia, 20560 USA;2. Department of Earth & Atmospheric Sciences, Purdue University, , West Lafayette, Indiana, 47907 USA;3. Dipartimento di Scienze della Terra, Università di Firenze, , I‐50121 Florence, Italy;4. Russian Academy of Sciences, Petrography, Mineralogy, and Geochemistry (IGEM), Institute of Geology of Ore Deposits, , Moscow, 119017 Russia;5. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, , Cambridge, Massachusetts, 02139 USA;6. Division of Geological and Planetary Sciences, California Institute of Technology, , Pasadena, California, 91125 USA;7. Department of Geosciences, Princeton University, , Princeton, New Jersey, 08544 USA;8. Geoscience Technology, , Houston, Texas, 77056 USA;9. Department of Earth and Planetary Sciences, Harvard University, , Cambridge, Massachusetts, 02138 USA;10. Department of Physics and Princeton Center for Theoretical Science, Princeton University, , Princeton, New Jersey, 08544 USA
Abstract:A new meteorite find, named Khatyrka, was recovered from eastern Siberia as a result of a search for naturally occurring quasicrystals. The meteorite occurs as clastic grains within postglacial clay‐rich layers along the banks of a small stream in the Koryak Mountains, Chukotka Autonomous Okrug of far eastern Russia. Some of the grains are clearly chondritic and contain Type IA porphyritic olivine chondrules enclosed in matrices that have the characteristic platy olivine texture, matrix olivine composition, and mineralogy (olivine, pentlandite, nickel‐rich iron‐nickel metal, nepheline, and calcic pyroxene diopside‐hedenbergite solid solution]) of oxidized‐subgroup CV3 chondrites. A few grains are fine‐grained spinel‐rich calcium‐aluminum‐rich inclusions with mineral oxygen isotopic compositions again typical of such objects in CV3 chondrites. The chondritic and CAI grains contain small fragments of metallic copper‐aluminum‐iron alloys that include the quasicrystalline phase icosahedrite. One grain is an achondritic intergrowth of Cu‐Al metal alloys and forsteritic olivine ± diopsidic pyroxene, both of which have meteoritic (CV3‐like) oxygen isotopic compositions. Finally, some grains consist almost entirely of metallic alloys of aluminum + copper ± iron. The Cu‐Al‐Fe metal alloys and the alloy‐bearing achondrite clast are interpreted to be an accretionary component of what otherwise is a fairly normal CV3 (oxidized) chondrite. This association of CV3 chondritic grains with metallic copper‐aluminum alloys makes Khatyrka a unique meteorite, perhaps best described as a complex CV3 (ox) breccia.
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