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首页> 外文期刊>Geo-marine letters >Authigenic carbonates related to active seepage of methane-rich hot brines at the Cheops mud volcano, Menes caldera (Nile deep-sea fan, eastern Mediterranean Sea)
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Authigenic carbonates related to active seepage of methane-rich hot brines at the Cheops mud volcano, Menes caldera (Nile deep-sea fan, eastern Mediterranean Sea)

机译:自燃碳酸盐与梅内斯火山口(Chenes)火山口(Cheops)的富含甲烷的热盐水主动渗漏有关(尼罗河深海扇,地中海东部)

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On the passive margin of the Nile deep-sea fan, the active Cheops mud volcano (MV; ca. 1,500 m diameter, ~20- 30m above seafloor, 3,010-3,020 m water depth) comprises a crater lake with hot (up to ca. 42 °C) methane-rich muddy brines in places overflowing down the MV flanks. During the Medeco2 cruise in fall 2007, ROV dives enabled detailed sampling of the brine fluid, bottom lake sediments at ca. 450 m lake depth, sub-surface sediments from the MV flanks, and carbonate crusts at the MV foot. Based on mineralogical, elemental and stable isotope analyses, this study aims at exploring the origin of the brine fluid and the key biogeochemical processes controlling the formation of these deepsea authigenic carbonates. In addition to their patchy occurrence in crusts outcropping at the seafloor, authigenic carbonates occur as small concretions disseminated within subseafloor sediments, as well as in the bottom sediments and muddy brine of the crater lake. Aragonite and Mg-calcite dominate in the carbonate crusts and in sub-seafloor concretions at the MV foot, whereas Mg-calcite, dolomite and ankerite dominate in the muddy brine lake and in subseafloor concretions near the crater rim. The carbonate crusts and sub-seafloor concretions at the MV foot precipitated in isotopic equilibrium with bottom seawater temperature; their low δ~(13)C values (-42.6 to -24.5‰) indicate that anaerobic oxidation of methane was the main driver of carbonate precipitation. By contrast, carbonates from the muddy lake brine, bottom lake concretions and crater rim concretions display much higher δ~(13)C (up to -5.2‰) and low δ~(18)O values (down to -2.8‰); this is consistent with their formation in warm fluids of deep origin characterized by ~(13)C-rich CO_2 and, as confirmed by independent evidence, slightly higher heavy rare earth element signatures, the main driver of carbonate precipitation being methanogenesis. Moreover, the benthic activity within the seafloor sediment enhances aerobic oxidation of methane and of sulphide that promotes carbonate dissolution and gypsum precipitation. These findings imply that the coupling of carbon and sulphur microbial reactions represents the major link for the transfer of elements and for carbon isotope fractionation between fluids and authigenic minerals. A new challenge awaiting future studies in cold seep environments is to expand this work to oxidized and reduced sulphur authigenic minerals.
机译:在尼罗河深海扇的被动边缘,活动的Cheops泥火山(MV;直径约1,500 m,在海底之上约20-30 m,水深3,010-3,020 m)包括一个火山口湖(温度最高可达42°C)在MV侧面溢流的地方富含甲烷的浑浊盐水。在2007年秋季的Medeco2航行期间,ROV潜水使能了对盐水,底湖沉积物的详细采样。湖深450 m,中压侧翼的表层沉积物,中压脚下的碳酸盐结壳。基于矿物学,元素学和稳定同位素分析,本研究旨在探索盐水的起源以及控制这些深海自生碳酸盐形成的关键生物地球化学过程。除了在海底的地壳露头中出现零星的碳酸盐外,自生的碳酸盐还发生在散布在海底沉积物中以及火山口湖底部沉积物和泥泞盐水中的小凝结物中。文石和镁方解石在MV脚的碳酸盐结壳和海底亚成体中占主导地位,而镁质方解石,白云石和白云母在火山口边缘的泥泞盐湖和海底成因中占主导地位。与底部海水温度成同位素平衡时,MV脚的碳酸盐结壳和海底地下沉淀物沉淀出来;其较低的δ〜(13)C值(-42.6至-24.5‰)表明甲烷的厌氧氧化是碳酸盐沉淀的主要驱动力。相比之下,来自泥湖卤水,湖底结石和火山口边缘结石的碳酸盐显示出更高的δ〜(13)C(高达-5.2‰)和低的δ〜(18)O值(下降至-2.8‰)。这与它们在深层起源于温暖的流体中的形成相一致,深层流体的特征是富含〜(13)C的CO_2,并且有独立证据证实,重稀土元素的签名略高,碳酸盐沉淀的主要驱动力是甲烷生成。此外,海底沉积物中的底栖活动增强了甲烷和硫化物的需氧氧化,从而促进了碳酸盐的溶解和石膏的沉淀。这些发现暗示碳和硫微生物反应的耦合代表了元素与流体和自生矿物之间的转移以及碳同位素分馏的主要联系。等待在冷渗流环境中进行未来研究的新挑战是将这项工作扩展到氧化和还原的硫自生矿物。

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