Sequestration of carbon in the forearc mantle wedge

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Guoji Wu, Yongsheng Huang, Michihiko Nakamura, Tatsuki Tsujimori, Yuan Li
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引用次数: 0

Abstract

Subduction zones are crucial in governing the global carbon (C) cycle. Recent geochemical and geophysical observations have revealed extensive serpentinite carbonation in the forearc mantle wedges, hinting at a potentially vast C reservoir within these serpentinized areas. In this study, we conducted experimental investigations on serpentinite carbonation in multicomponent (H2O–CO2–NaCl) fluids under various pressure–temperature (P-T) conditions that mimic the mantle wedge. Our aim was to precisely determine the reaction extent (RE, RE = Vmgs / V0mgs, where Vmgs represents the actual magnesite volume in the run product and V0mgs denotes the theoretical magnesite volume through the complete reaction of CO2.) of serpentinite carbonation in the multicomponent fluids and, subsequently, estimate C storage in the forearc mantle wedge. Our findings indicate that serpentinite reacts with CO2 to form magnesite and talc. Time-series experiments demonstrated that reaction equilibrium is attained within 48 h. The results revealed that RE increases with rising P-T and CO2 concentration in fluids. However, a notable decrease in RE was observed with increasing salinity, particularly at low salinities (< 10 wt%). This decrease can be attributed to the reduced fluid pH, decreased CO2 and H2O activities (aCO2 and aH2O), and increased magnesite solubility in salt-bearing fluids. Based on previous and our experimental data, we derived an empirical equation to describe the RE of serpentinite carbonation in H2O–CO2–NaCl fluids. We extrapolated the potential RE regarding P-T conditions and fluid compositions within the mantle wedge to estimate C inventory in forearc mantle wedges. Our calculations indicated that even a minimal degree of serpentinization (< 10 vol%) in the mantle wedge could result in the sequestration of 49–76 % of C from slab-derived fluids originating from depths of 15–80 km through serpentinite carbonation, leading to the formation of magnesium-rich carbonates. On a global scale, this carbonation process has the capacity to sequester 0.02–4.17 million tons of C per year (Mt C/yr) within forearc mantle wedges. Consequently, a portion of the C stored in carbonated serpentinite may persist in the cold, stagnant regions of the wedge, potentially contributing to long-term C storage and seismic activity. Furthermore, due to processes such as down-dragging and subduction erosion, some of the C fixed in the lower carbonated layer may be transported to partial melting regions, ultimately contributing to volcanic emissions in arc regions. This highlights the multi-stage nature of C migration within the mantle wedge. Our study offers significant insights into the C cycle and seismic responses within subduction zones.
弧前地幔楔体中碳的固存
俯冲带对控制全球碳(C)循环至关重要。最近的地球化学和地球物理观测显示,弧前地幔楔中存在广泛的蛇纹岩碳酸化,暗示在这些蛇纹岩化区域可能存在巨大的碳储集层。在模拟地幔楔的不同压力-温度(P-T)条件下,对多组分(H2O-CO2-NaCl)流体中的蛇纹岩碳酸化进行了实验研究。我们的目的是精确地确定多组分流体中蛇纹岩碳酸化的反应程度(RE, RE = Vmgs / v0mg,其中Vmgs表示流动产物中菱镁矿的实际体积,v0mg表示通过CO2完全反应得到的菱镁矿的理论体积),并随后估算弧前地幔楔中的C储量。我们的研究结果表明,蛇纹岩与二氧化碳反应生成菱镁矿和滑石。时间序列实验表明,反应在48 h内达到平衡。结果表明,RE随流体中P-T和CO2浓度的升高而增加。然而,随着盐度的增加,RE显著下降,特别是在低盐度(<;10 wt %)。这种降低可归因于流体pH值降低,CO2和H2O活性(aCO2和aH2O)降低,以及菱镁矿在含盐流体中的溶解度增加。基于前人数据和实验数据,推导了蛇纹岩在H2O-CO2-NaCl流体中碳酸化RE的经验方程。我们根据地幔楔内的P-T条件和流体组成推断出潜在的稀土含量,以估计弧前地幔楔的碳储量。我们的计算表明,即使是最小程度的蛇纹石化(<;在地幔楔中,通过蛇纹岩碳酸化作用,可以从深度为15-80 km的板块衍生流体中吸收49 - 76%的碳,从而形成富镁碳酸盐。在全球范围内,这种碳酸化过程有能力在弧前地幔楔中每年吸收0.02 - 417万吨碳(公吨碳/年)。因此,储存在碳酸蛇纹岩中的部分碳可能会持续存在于楔体的寒冷停滞区域,这可能有助于长期的碳储存和地震活动。此外,由于下拉和俯冲侵蚀等作用,部分固定在碳酸层下部的碳可能被输送到部分熔融区,最终导致弧区火山排放。这凸显了地幔楔内碳运移的多阶段性。我们的研究对俯冲带内的C旋回和地震反应提供了重要的见解。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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