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Timing of magmatic and mefamorphic events in the Jijol complex of the Kohistan acc deduced from Sm-Nd dating of mafic granulites.
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In-situ U-Pb zircon age luh-f deciphering the formation event of the omphacite growth over relict lu-hf dating pargasite in omphacite-bearing jadeitite of the Itoigawa-Omi area of the Hida-Gaien belt, central Japan. Omphacite replacing after relic edenitic pargasite has been found in an omphacite-bearing jadeitite block of the Itoigawa-Omi area in the Hida-Gaien belt.
Omphacite occurs sporadically as fine-grained aggregate reaching a few cm in length in a jadeite-albite matrix, and sometimes contains edenitic pargasite as a core. The edenitic pargasite is chemically and optically homogeneous and does not show lu-hf dating contact with jadeite and albite. An irregular shaped omphacite-diopside mixed area occurs near edenitic pargasite in a coarse omphacite aggregate. At the periphery of pseudomorphic omphacite, a hydrothermal fluid removed the breakdown components of the reaction other than omphacite.
The studied jadeitite is a typical R-type jadeitite, and the nearly total replacement from a precursor rock to the omphacite-bearing jadeitite has been attributed to hydrothermal activity at Middle Cambrian times. Web of Science.
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Silicate-SiO reaction in a protoplanetary disk recorded by oxygen isotopes in chondrules. The formation of planetesimals and planetary embryos during the earliest stages of the solar protoplanetary disk lu-hf dating determined the composition and structure of the terrestrial planets. Within a few million years of the birth of the Solar System, chondrule formation and the accretion of the parent bodies of differentiated achondrites and the terrestrial planets took place in the inner protoplanetary disk 1,2.
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Vating we show that, for chondrules in unequilibrated enstatite chondrites, high-precision Delta O values where Delta O is the deviation of the delta O value from a terrestrial silicate fractionation line vary significantly ranging from This array can be explained by the reaction between an olivine-rich chondrule melt and an SiO-rich gas derived from vaporized dust and nebular gas. Our study suggests that a large proportion of the building lu-hf dating of planetary embryos formed by successive silicate-gas interaction processes: silicate- H2O followed by silicate-SiO interactions lu-hf dating more oxidized and reduced conditions, respectively, within a few million years of the formation of the Solar System.
Petrologic and geochemical characterization of rift-related magmatism at the northernmost Main Ethiopian Visit web page Implications for plume-lithosphere interaction and the evolution of rift mantle sources. Feyissa, R. Shinjo, H. Kitagawa, D. Meshesha, E. The K-Ar ages of the mafic series range from 27 to 0. The mafic volcanics are classified into older and younger series based on their K-Ar ages. Geochemical and isotopic compositions of fating older and younger mafic lavas indicate that crustal contamination did not play a lu-hf dating role in the evolution of their magmas, hence reflect the geochemical characteristics of the sources.]
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