日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 S (固体地球科学) » S-MP 岩石学・鉱物学

[S-MP29] Oceanic and Continental Subduction Processes

2019年5月28日(火) 13:45 〜 15:15 A08 (東京ベイ幕張ホール)

コンビーナ:Hafiz Ur REHMAN(Department of Earth and Environmental Sciences, Graduate School of Science and Engineering, Kagoshima University)、辻森 樹(東北大学)、Chin-Ho Tsai(Department of Natural Resources and Environmental Studies, National Dong Hwa University)、岡本 和明(埼玉大学教育学部地学)、座長:Hafiz REHMAN(Kagoshima University)、Tatsuki Tsujimori

14:15 〜 14:45

[SMP29-03] Continental subduction, “Intraslab UHP Metasomatism”, and the formation of metamorphic diamond

★招待講演

*小笠原 義秀1 (1.Department of Earth Sciences, Waseda University)

キーワード:intraslab UHP metasomatism、UHP metamorphism、diamond、carbonate、fluid、Kokchetav Massif

Deep continental subduction is the process carrying supracrustal materials into deep mantle, and UHP metamorphic rocks are the direct evidence for this process as the materials having the information of P-T and the chemical environments during subduction, escaped from the homogenization with mantle rocks. Usually, UHPM silicate rocks have been strongly retrograded during exhumation, and the preservation of UHPM information is limited excepting inclusions in refractory minerals; decoding the chemical processes in subducted materials is difficult. In carbonate and calc-silicate rocks, UHPM information has been well preserved and can be decoded even in the matrix because the chemical reactions in these rocks make distinct changes from the protolith chemistries, not erased during exhumation.

Carbonate-bearing assemblages have large P-T stabilities at HP/UHP and low H2O activity, and this indicates high possibility of survival of carbonates and transportation of carbon into deep mantle. H2O-fluid supply is necessary for metamorphic reactions in these rocks because H2O-fluid lowers temperatures of decarbonations. As a model showing the processes in deeply subducting continental materials, Intraslab UHP Metasomatism (metasomatism within subducting continental materials at UHP mantle depths) will be introduced on the basis of our last 20 years research on the Kokchetav UHPM rocks. In this model, key materials are H2O and CO2 in the subducting continental slab, and a key process is H2O-fluid infiltration within the slab. The outline of this model is as follows. 1) In the subducting slab, silicate rocks (gneisses and eclogite) were a H2O reservoir, and carbonate and calc-silicate rocks were a CO2 reservoir. 2) During subduction, H2O-fluid with several components (e.g. C, K, Ti) occurred by dehydrations of silicate rocks. 3) Dehydrations in silicate rocks preceded decarbonation reactions in carbonate and calc-silicate rocks. 4) Infiltration of H2O-fluid into carbonate and calc-silicate rocks was a trigger for decarbonations. 5) H2O-fluid infiltration was controlled by the timing of dehydrations in silicate rocks and vaired in mm to cm scales to form or to characterize the mineral assemblages in carbonate and calc-silicate rocks. 6) H2O-fluid (with C-bearing species) contributed to the formation of diamond in some carbonate calc-silicate rocks. 7) Modal compositions of carbonates in the protoliths controlled the survival of carbonate depending on the intensity of fluid infiltration.

The following subjects from the Kokchetav UHPM rocks support this model. A) Dolomite marble contains abundant diamond formed at two stages; 2nd stage diamond (δ13C: -17 to -27 ‰) from H2O-fluid. Dol + Di is not the highest-T assemblage and was controlled by fluid composition, XCO2 as 0.1, which was suitable for diamond formation. B) Dolomitic marble has the highest-T assemblages, Arg-Fo, Arg-Ti-Chum, but diamond was unstable because of low XCO2 as 0.01. C) Calcite (after Arg) marble with Coe exsolution in Ttn contains diamond only in Di layer, and other parts do not; this indicates short-term stability of diamond in this rock depending on changing XCO2. The later fluid was low XCO2 as 0.02; too low for diamond formation. D) Two types of Grt-Cpx rocks occur; diamond-bearing and diamond-free. Their protoliths are a mixture of silicates and carbonates. Minor diamond occurs as two modes in diamond-bearing Grt-Cpx rock; one is fine-grained (several μm) and the other is cubic (max. 200 μm). A cubic diamond has fine core and crystallized slowly from H2O-fluid on a fine grain as a seed crystal. E) In gneisses, diamond occurrence is diverse; several morphologies with different colors were observed. Two-stage growth was not confirmed. Dissolution of carbon from diamond in gneisses could be possible, and carbon was carried into dolomite marble by H2O-fluid to crystallize 2nd stage diamond.

Many of the subjects being still unclear will be mentioned as the targets of future research.