Abstracts of Annual Meeting of the Geochemical Society of Japan
Abstracts of Annual Meeting of the Geochemical Society of Japan
Displaying 1-50 of 310 articles from this issue
  • Atsuyuki Ohta, Kazuya Tanaka, Hiroshi Tsuno
    Pages 22-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS
  • Keita Itano, Tsuyoshi Iizuka, Mihoko Hoshino
    Pages 23-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS
  • Kodai Mano, Yoshihiro Asahara, Motohiro Tsuboi, Hossein Azizi, Kicheol ...
    Pages 24-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS
  • Tsuyoshi Ishikawa, Kohtaro Ujiie, Tatsuya Kawai, Kazuya Nagaishi
    Pages 25-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS
  • Mayuko Fukuyama, Masatsugu Ogasawara, Rhanul Huq Siddiqui
    Pages 26-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS
  • Zu Bo, Xue Chunji, Pak Nikolay, Zhao Xiaobo
    Pages 27-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS

    A number of word-class gold deposits in the Kassan area in the west Kyrgyzstan are associated with the Andagul granitic intrusion. These gold deposits share similarities with the class of “intrusion-related gold deposits”, implying that the gold mineralization may be genetically related to the intrusion. In order to evaluate this potential relationship, it is important to study the petrogenesis of the intrusion. This study examines the sources and physiochemical conditions of crystallization of the Andagul intrusion and their implications for gold mineralization, through an integrated study involving zircon geochronology, mineral chemistry, whole-rock chemistry and isotopic geochemistry. The Andagul intrusion consists mainly of granodiorite, which is characterized by metaluminous and medium-K calc-alkaline compositions, very high Ba (>2000 ppm) and Sr (>1500 ppm) abundances, high LREE, LILE, low HFSE , right-inclined REE pattern with a flat HREE pattern, and insignificant Eu anomalies ((Eu/Eu*)N = 0.80 - 0.85). These geochemical characteristics, together with relatively low positive εNd(t) values (+2.1 to +4.2), moderately low (87Sr/86Sr)i ratios (0.70497 to 0.70666), relatively low initial Pb isotopic ratios ( (206Pb/204Pb)t = 17.642 to 18.398, (207Pb/204Pb)t = 15.599 to 15.618, and (208Pb/204Pb)t = 38.034 to 38.297), juvenile εHf(t) (+2.29 to +4.78) and relatively young model ages (T2DM(Hf)=1027 to 1180 Ma, T2DM(Nd)= 729 - 898 Ma) indicate that the magma was sourced from partial melting of juvenile basaltic lower crust with amphibole as dominant residual. The high Zr saturation temperatures (807oC to 825 oC), relatively high Mg# values (43-52) and presence of mafic enclaves, and development of acicular apatite and oscillatory plagioclases and titanite, suggest that the magmatism was related to injection of hot mantle material into the lower crust, which took place in a slab-break off setting at ca. 300 Ma. The high water contents (4.0 to 5.2 wt.% H2O) and moderately oxidized to weakly reduced state (ΔFMQ = -0.29 ~ +2.82) deduced from amphibole composition and zircon Ce anomaly are favorable for enrichment of gold in magmatic fluids.

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  • Li Jianwei, Hu Hao
    Pages 28-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS

    The Tieshan Fe-Cu skarn deposit in the Daye district of eastern China provides a valuable opportunity to better understand the nature and genesis of hydrothermal REEs mineralization associated with calc-alkaline intermediate magmatism. This deposit is genetically associated with an intrusive complex locally called Tieshan pluton. The Tieshan complex consists of six intrusive bodies which are, from a temporal order, syenodiorite, gabbroic diorite, monzodiorite, granodiorite, and quartz diorite or monzodiorite. The geochemical signatures, combined with whole-rock Sr-Nd and zircon Hf isotopic results, suggest that the Tieshan intrusion was derived from an enriched mantle sources metasomatized by slab-derived fluids and/or melts (Li et al., 2009). The Tieshan deposit contains proven reserves of 160 Mt Fe at an average of 53 % (up to 70 %) and 0.67 Mt Cu at 0.58 % (up to 12 %) (Yao et al., 1993). Skarn assemblages are well developed throughout the ore zones and consist of diopside, garnet, scapolite, phlogopite, actinolite, chlorite, albite, plagioclase, tremolite, pargasite, and epidote, which are frequently overprinted by quartz, calcite, ankerite, anhydrite, and fluorite. Common metallic minerals are magnetite, hematite, chalcopyrite, bornite, marcasite, pyrrhotite, molybdenite, specularite, and siderite. Native gold or electrum is present as inclusions mainly in pyrite and chalcopyrite. Our recent drill-core logging has revealed extensive REEs mineralization closely associated with the skarn assemblages and iron ores. The REEs mineralization is spatially related to the gabbroic diorite of the Tieshan complex and mostly developed in the endoskarn zone dominated by diopside. Individual REEs ore zones are 7.9-12 m thick and average in REE2O3 contents at 1-13 %. REEs ores are variably associated with Fe or Fe-Cu skarn ores. The ore minerals are dominated by allanite with minor parasite and titanite. They typically occur as hydrothermal overprints on diopside, garnet, scapolite, and albite, are texturally intergrown with minor magnetite, hematite, apatite, chlorite, and epidote, and are locally overprinted by anhydrite, pyrite, chalcopyrite, and calcite. Allanite grains typically show oscillatory zoning and dissolution-reprecipitation textures that indicate at least four generations of allanite. The textural relations imply episodic REEs mineralization. Allanite, epidote, and diopside host abundant primary fluid inclusions that have homogenization temperatures of 500-670 ºC and calculated salinities of 40-60 wt% NaCl equiv., consistent with common presence of multiple daughter minerals dominated by halite and sylvite. Parasite is locally observed in a few inclusions. The fluid inclusion data thus demonstrate the REEs were transported by and precipitated from high-temperature saline to hyposaline magmatic fluids. The widespread scapolite and the very high salinity of the fluid inclusions led us to conclude that chlorine has been important in transporting REEs at Daye. The skarn formation involving interaction between the carbonate wallrocks and the magmatic-derived fluids would have enhanced the pH of the latter and consequently facilitated the precipitation of REEs minerals to form the ores. On the U-Pb Tera-Wasserburg diagram, titanite has lower-intercept age of 141 ± 1 Ma and a weighted mean206Pb/238U age of 140 ± 2 Ma, which are consistent with the zircon U-Pb age of the gabbroic diorite. This age consistency demonstrate a genetic relations between the REEs mineralization and the intermediate magmatism represented by the Daye pluton. We suggest that REEs were sourced from the magmas produced by partial melting of an enriched mantle source that have previously been metasomatised by slab-derived fluids and/or melts, a processes enriching the mantle peridotite by REEs, particularly light REEs in the case of Daye deposit.

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  • Liu yun, Yang Yuhong
    Pages 29-
    Published: 2017
    Released on J-STAGE: November 09, 2017
    CONFERENCE PROCEEDINGS FREE ACCESS

    The carbon budget in the Earth interior is currently not well constrained because the sample of the Earth’s core is unavailable. Several ways have been used to estimate the Earth’s carbon inventory but their results vary more than one order of magnitude. Recently, using isotope signals to solve this kind of budget problem becomes an alternative way for various different isotope systems (Satish-Kumar et al., 2011; Shahar et al., 2011; Moynier et al., 2011; Lazar et al., 2012; Horita and Polyakov, 2015; Shahar et al., 2016; Elardo and Shahar, 2017; Liu et al., 2017). Here equilibrium carbon isotope fractionation factors for almost all kinds of carbon-bearing species in the deep Earth are provided by using first-principles methods. For the first time, silicate melts and iron melts are calculated directly other than using their crystalline analogues in the previous studies. We find that melts have very different compressibility than those crystalline analogues. Besides, compared to a fixed crystalline structure, melts have numerous local different configurations. A reasonable simulation of melts should considering the proper sampling of these local configurations to obtain a precise average result. Neglecting these differences between melts and crystalline analogues will let the estimations of isotope fractionation factors to be risky.In this study, we calculate the equilibrium isotopic fractionation factors of carbon between silicate melt, iron melt, magnesite, diamond, moissanite, and various iron-carbides at magma ocean conditions by first-principles density functional theory. The influences of pressure and redox condition on the chemical environment and isotope fractionation of carbon are also carefully investigated. The average value of δ13C of BSE is estimated to be about −7.2‰, according to the mantle derived diamonds (Cartigny et al., 2014). Although many people thought this signal can represent the carbon isotope composition of the whole mantle, we disagree with it. Diamonds can only represent the major C-bearing species at upper part of mantle, but not the major C-bearing species at lower mantle. Higher temperatures can destabilize diamond. Based on the mantle derived diamonds’ δ13C signal (−7.2‰) and those isotope fractionation factors we provided, we can deduce out the signal for the BSE. Our new carbon isotope fractionation results cannot compromise the mantle-core differentiation scenario at magma ocean period, no matter it is an equilibrium or a Rayleigh distillation process. However, if most of carbon was delivered from one or several giant impacts from the accretion feeding zone of Mars (i.e., with the similar chemistry), and with 2 times of the current mass of Mars to be delivered to the proto-Earth, all discrepancies will be resolved perfectly. This scenario coincides with the giant impact hypothesis of the Moon formation and the unexpected small size of Mars. Finally the carbon content of Earth’s core is estimated about 0.2wt% of the core. Carbon is not a major light element in the Earth's core.

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