Japan Geoscience Union Meeting 2014

Presentation information

Oral

Symbol S (Solid Earth Sciences) » S-CG Complex & General

[S-CG62_2AM1] Geofluids and dynamics in subduction zones

Fri. May 2, 2014 9:00 AM - 10:45 AM 502 (5F)

Convener:*Atsushi Okamoto(Graduate School of Environmental Studies), Tatsuhiko Kawamoto(Institute for Geothermal Sciences, Graduate School of Science, Kyoto University), Ikuo Katayama(Department of Earth and Planetary Systems Science, Hiroshima University), Chair:Atsushi Okamoto(Graduate School of Environmental Studies), Ikuo Katayama(Department of Earth and Planetary Systems Science, Hiroshima University)

10:15 AM - 10:30 AM

[SCG62-06] The regional and single-vein scale distribution of the CO2 fluids in the Shimanto accretionary complex, Muroto area, SW

*Michimasa MUSHA1, Noriyoshi TSUCHIYA1, Atsushi OKAMOTO1 (1.Enviromnetal Studies of Tohoku University)

Keywords:fluid inclusions, accretionary complexes, calcite, mineral veins, C-H-O fluid, Shimanto belt

Carbon dioxide and methane are major carbonic components of the fluids in the crust. The crustal fluids generally have composition of C-H-O system, mainly composed of H2O, CO2, and CH4, and they may be carried down into Earth's interior at subduction zones. Many studies have examined fluid components in various accretionary prisms under low-grade metamorphic conditions, and CH4 is showed as the only carbonic species. Therefore, there is little information on the variation of the components of C-H-O fluids in subduction zones. The Tertiary (Paleogene and Neogene system) Shimanto belt, southwest in Japan, is one of the best-studied ancient accretionary complexes. The Muroto Peninsula belongs to the Tertiary Shimanto belt, and it is mainly composed of sandstones, mudstones and conglomerates with small amount of basalt. Mineral veins were mainly composed of quartz, with small amount of calcite near the vein walls, while many studies have showed CH4 is the only carbonic component in the Shimanto belt, therefore it is unclear why calcite precipitated in the veins in absence of CO2. Lewis (2000) reported the fluid inclusions of CH4 and CO2 mixture at one area in the Muroto Peninsula, but the extensive distribution of CO2 fluids in the whole peninsula is not clear. In this study, we examined the distribution of C-H-O fluids from the Murotohanto Peninsula, as fluid inclusions in the mineral veins, using microthemometry and Laser Raman spectroscopy, in regional scale and single vein scale. Fluid inclusions from quartz in the veins are composed of one-phase carbonic inclusions (only CH4) and two-phase aqueous inclusions (carbonic vapor and H2O liquid). Carbonic components of the vapor phase in the two-phase inclusions are gradually transited from CH4-dominant in the north area of the belt to a CO2?CH4 mixture in the south; the CO2/(CO2 + CH4) ratio in mole fraction (XCO2) vary from 0 ~ 0.3 in the north area to 0 ~ 0.9 in the south. In single vein scale, we examined single CO2-bearing vein from the south area of the Peninsula, where XCO2 is 0 ~ 0.8. The CO2 ratio in the carbonic species is decreased from the vein wall (XCO2 = 0.5?0.8) to the vein center, in which carbonic species in the fluids is only CH4 (XCO2 = 0). The existence of CO2 only near the vein walls is in good agreement of the precipitation of calcite near the vein walls. The homogenization temperature increases from ~180 ℃ to 240?250 ℃, indicating the transition of the carbonic species from CO2?CH4 to CH4 during vein formation. The dominant species of carbonic species in most accretionary prisms is CH4 under low-grade metamorphic conditions, and thermodynamic calculation about equilibrium in the C-H-O fluids also shows that CH4 is dominant carbonic species in the equilibrium with graphite under the P?T conditions of formation of the CO2-bearing veins (235?245 ℃, 165?200 MPa). The CO2-fluids are preferentially distributed close to an out-of-sequence thrust that brings the Murotohanto sub-belt into contact with the late Oligocene?early Miocene Nabae sub-belt with its many volcanic lavas and intrusive rocks. Therefore, the CO2-fluids were considered to be magmatic-origin, and that the fluids were injected and mixed with the CH4 pore-fluids of the sediments in the accretionary prism in the timing of formation of CO2-bearing veins.