日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-MP 岩石学・鉱物学

[S-MP06_28PM2] Impact of volatiles on the processes of formation and evolution of the Earth's interior

2014年4月28日(月) 16:15 〜 17:45 411 (4F)

コンビーナ:*Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、Eiji OHTANI(Graduate School of Science Tohoku University 6-3 Aoba, Aramaki, Aoba-ku Sendai 980-8578)、Tatsuhiko KAWAMOTO(Univ. Kyoto Kyoto, 606-8502, JAPAN)、座長:大谷 栄治(東北大学大学院理学研究科地学専攻)

17:15 〜 17:30

[SMP06-11] Carbon dioxide in granitic magma under lower crustal conditions

*吉村 俊平1中村 美千彦2圦本 尚義3 (1.山形大学理学部地球環境学科、2.東北大学大学院理学研究科地学専攻地球惑星物質科学講座、3.北海道大学理学研究院自然史科学部門)

キーワード:CO2, H2O, solubility, granitic melt

Carbon dioxide is a major volatile component in the crust and mantle. Its solubility and speciation in silicate melts are important in understanding of mechanisms of magmatism and volcanism. However, they are not well constrained under lower-crustal conditions, especially in granitic magma, which is common in the crustal magmatism. In this study, we carried out equilibrium experiments in the CO2-H2O-granitic melt system to investigate the solubility and speciation of CO2.High-PT experiments were performed using a piston cylinder apparatus and a cold-seal pressure vessel. Obsidian flakes of a granitic composition and oxalic acid dehydrate (fluid source) were put in a gold or platinum capsule and run at 1123 and 1473 K and 0.1-1.5 GPa. Oxygen fugacity was estimated to be close to NNO. After quench, volatiles dissolved in the glass were analysed with FTIR spectroscopy. The composition of the coexisting fluid was quantified either by manometric analysis or based on the low-pressure solubility law and volatile contents of the glass.FTIR spectra showed that both CO2 molecules (CO2mol) and carbonate anions (CO32-) were present in all of the glass samples. The concentrations of CO2mol, CO32- and total H2O increased generally with increasing pressure; they were 9200 ppm, 2100 ppm and 6.1 wt%, respectively, at 1.5 GPa and 1473 K. Here, we used new molar absorption coefficients of 2350 cm-1 (1192 ± 130 L cm-1 mol-1; CO2mol) and 1410 cm-1 (91 ± 28 L cm-1 mol-1; CO32-) determined in this study. The fraction of CO32 to total CO2 in the granitic melt increased with increasing total CO2 content, from 0.09 (total CO2 = 260 ppm) to 0.19 (11300 ppm). The molar fractions of CO2 in the fluids (XCO2fluid) were 0.25-0.48 for the cold-seal experiments and 0.73-0.79 for the piston cylinder experiments.We formulated the solubility law of CO2mol based on a vapour-liquid equilibrium equation. On the basis of the reaction CO2 (vapour) ⇌ CO2mol (melt), we calculated the partial molar volume of CO2mol in the granitic melt and the reaction enthalpy to be 24.9 ± 2.0 cm3/mol and -22.2 ± 6.3 kJ/mol, respectively. These values are similar to those in previous experiments carried out at < 6.6 kbar (Fogel and Rutherford, 1989; Behrens et al., 2004), indicating that the low-pressure solubility law can be extrapolated to 1.5 GPa. As for the formation of CO32-, we assumed a reaction CO2mol + O2- (non-bridging oxygen) ⇌ CO32-. Possible factors shifting the equilibrium to the right-hand side include the total pressure (e.g., Fine and Stolper, 1985; Guillot and Sator, 2011) and water content (King and Holloway, 1992; Behrens et al., 2004). In this study, it was difficult to evaluate these parameters separately, since the water content increased simultaneously with total pressure. If we assume that the effect of water is small enough to be neglected, the change of the partial molar volume of CO2 in the melt and the reaction enthalpy can be calculated to be -8.6 ± 6.0 cm3/mol and -0.4 ± 3.1 kJ/mol, respectively.Recently, unusually CO2-rich rhyolitic melt inclusions (up to 1.7 wt% total CO2) were reported by Blundy et al. (2010). The saturation pressure of this CO2 content is estimated to be 1.4 GPa when CO2 dissolved only as CO2mol (XCO2fluid = 1; T=1173 K). If we consider the formation of CO32-, the saturation pressure is estimated to 1.2 GPa.