A record of low-temperature asteroidal processes of amoeboid olivine aggregates from the Kainsaz CO3.2 chondrite
نویسندگان
چکیده
Amoeboid olivine aggregates (AOAs) from the Kainsaz CO3.2 chondrite were analyzed using transmission electron microscopy in order to gain a more complete understanding of thermal metamorphism on parent body and role fluids during metamorphic heating. The AOAs are dominated by strongly zoned, fine-grained, grains (Fa2-31) with heterogeneous Fe enrichments along grain boundaries, which interpreted as result Fe2+-Mg2+ interdiffusion matrix metamorphism. However, our diffusion calculations show that such AOA zoning compositions cannot be produced simple diffusional exchange heating, unlike chondrule compositions. In addition, fine-grained ferroan overgrowths occur heterogeneously crystallographic continuity olivines exteriors. (Fa33-36) compositionally distinct underlying not fully equilibrated (Fa∼20-55). likely formed precipitation an epitaxial relationship forsteritic edges AOAs. Texturally diverse chromite also observed grains, pore spaces between grains. They share similar orientation adjacent olivine, suggestive their formation exsolution and/or growth. Collectively, these observations provide evidence for mobilization Fe, Mg, Si, Cr, Al presence boundaries into We conclude AOAs, strong zonation development individual fluid-driven process occurred at relatively low temperatures (<500 °C), cooling history CO3 body, following peak
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Fagan, M. Miyamoto, A.N. Krot and T. Mikouchi, The University Museum, University of Tokyo, 7-3-1 Hongo Bunkyo-ku Tokyo, Japan ([email protected]), Department of Earth Sciences, School of Education, Waseda University, 1-6-1 Nishiwaseda Shinjuku-ku Tokyo, Japan, Department of Earth & Planetary Science, University of Tokyo, Japan. Hawaii Institute of Geophysics and Planetology, University o...
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ژورنال
عنوان ژورنال: Geochimica et Cosmochimica Acta
سال: 2022
ISSN: ['1872-9533', '0016-7037']
DOI: https://doi.org/10.1016/j.gca.2022.02.007