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Halogen and 129-I systematics in gas hydrate fields at the northern Cascadia margin (IODP Expedition 311): insights from numerical modeling

机译:卡斯卡迪亚北部边缘天然气水合物田中的卤素和 129 -I系统(IODP Expedition 311):数值模拟的见解

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摘要

We measured halogen concentrations and I-129/I ratios in five drilling sites of Integrated Ocean Drilling Program Expedition 311 (offshore Vancouver Island, Canada) in order to identify potential sources of fluids and methane in gas hydrate fields. Iodine is dominated by organic decomposition and transports with fluids in reducing environments and the presence of the cosmogenic radioisotope I-129 (T-1/2 = 15.7 Ma) allows the age determination of organic sources for iodine. Here we report halogen concentrations in 135 pore water samples, I concentrations in 48 sediment samples, and I-129/I ratios measured in a subset of 20 pore water samples. Most I-129/I ratios fall into a range around 500 x 10(-15), corresponding to a minimum age of 25 Ma and the lowest ratio of 188 x 10(-15) (T-min = 47 Ma) was observed at 208 m below sea floor (mbsf) in Site 1326. These ages are considerably older than that of the local sediments in the gas hydrate fields and that of the subducting sediments on the Juan de Fuca plate, indicating that old, accreted sediments in the accretionary wedge contribute a significant amount of iodide and, by association, of methane to the gas hydrate occurrences. A geochemical transport-reaction model was applied to simulate the advection of deeply sourced fluids and the release of iodide, bromide, and ammonia in the host sediments due to organic matter degradation. The model was first tested with data from two well studied areas, Ocean Drilling Program Site 1230 (Peru margin) and Site 1245 (Hydrate Ridge). The model results for the Expedition 311 sites indicate that the in situ release of young iodine is relatively minor in comparison to the contribution of migrating fluids, carrying large amounts of old iodine from deep sources. The comparison between the sites demonstrates that the total organic content has a strong effect on the rate of in situ iodine release and that lateral flows along fractures can have a significant influence on pore water chemistry, especially at the Cascadia margin. The iodine results indicate that mobilization and transport of methane from sources in the upper plate of active margins is an important process which can also play a substantial role in the formation of gas hydrate fields.
机译:为了确定天然气水合物气田中潜在的流体和甲烷的来源,我们在“综合海洋钻探计划”远征311号的五个钻探地点(加拿大近海温哥华岛)中测量了卤素浓度和I-129 / I比。碘主要由有机物分解并在还原性环境中以液体运输,并且存在宇宙性放射性同位素I-129(T-1 / 2 = 15.7 Ma)可以确定碘的有机来源的年龄。在这里,我们报告了135个孔隙水样品中的卤素浓度,48个沉积物样品中的I浓度以及在20个孔隙水样品的子集中测得的I-129 / I比。大多数I-129 / I比率都落在500 x 10(-15)左右的范围内,对应于最小年龄25 Ma,观察到最低比率188 x 10(-15)(T-min = 47 Ma)在1326号站点海床(mbsf)下方208 m处。这些年龄远比天然气水合物田中的局部沉积物年龄和胡安德富卡板块上的俯冲沉积物年龄大,这表明该地区较老的,增生的沉积物增生楔形物对气体水合物的产生贡献了大量的碘化物和甲烷。应用地球化学输运-反应模型来模拟深层流体的对流以及由于有机物降解而在宿主沉积物中释放的碘化物,溴化物和氨。该模型首先使用来自两个研究区域的数据进行了测试,这两个区域分别是Ocean Drilling Program Site 1230(秘鲁边界)和Site 1245(水合物岭)。 Expedition 311站点的模型结果表明,与从深处携带大量旧碘的迁移流体的贡献相比,年轻碘的原位释放相对较小。位置之间的比较表明,总有机物含量对原位碘释放速率有很大影响,而沿裂缝的侧向流动对孔隙水化学,尤其是在卡斯卡迪亚边缘的孔隙水化学有重要影响。碘的结果表明,甲烷从有效边界上板的源中动员和运输是一个重要过程,在天然气水合物田的形成中也可以发挥重要作用。

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