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Deposition of talc, kerolite-smectite, smectite at seafloor hydrothermal vent fields: Evidence from mineralogical, geochemical and oxygen isotope studies

机译:在海底热液喷口处沉积滑石,硅藻土,蒙脱石,蒙脱石:来自矿物学,地球化学和氧同位素研究的证据

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Talc, kerolite-smectite, smectite, chlorite-smectite and chlorite samples from sediments, chimneys and massive sulfides from six seafloor hydrothermal areas have been analyzed for mineralogy, chemistry and oxygen isotopes. Samples are from both peridotite- and basalt-hosted hydrothermal systems, and basaltic systems include sediment-free and sediment-covered sites. Mg-phyllosilicates at seafloor hydrothermal sites have previously been described as talc, stevensite or saponite. In contrast, new data show tri-octahedral Mg-phyllosilicates ranging from pure talc and Fe-rich talc, through kerolite-rich kerolite-smectite to smectite-rich kerolite-smectite and tri-octahedral smectite. The most common occurrence is mixed-layer kerolite-smectite, which shows an almost complete interstratification series with 5 to 85% smectitic layers. The smectite interstratified with kerolite is mostly trioctahedral. The degree of crystal perfection of the clay sequence decreases generally from talc to kerolite-smectite with lower crystalline perfection as the proportion of smectite layers in kerolite-smectite increases. Our studies do not support any dependence of the precipitated minerals on the type/subtype of hydrothermal system. Oxygen isotope geothermometry demonstrates that talc and kerolite-sinectite precipitated in chimneys, massive sulfide mounds, at the sediment surface and in open cracks in the sediment near seafloor are high-temperature (>250 degrees C) phases that are most probably the result of focused fluid discharge. The other end-member of this tri-octahedral Mg-phyllosilicate sequence, smectite, is a moderate-temperature (200-250 degrees C) phase forming deep within the sediment (similar to 0.8 in). Chlorite and chlorite-smectite, which constitute the alteration sediment matrix around the hydrothermal mounds, are lower-temperature (150-200 degrees C) phases produced by diffuse fluid discharge through the sediment around the hydrothermal conduits. In addition to temperature, other two controls on the precipitation of this sequence are the silica activity and Mg/Al ratio (i.e. the degree of mixing of seawater with hydrothermal fluid). Higher silica activity favors the formation of talc relative to tri-octahedral smectite. Vent structures and sedimentary cover preclude complete mixing of hydrothermal fluid and ambient seawater, resulting in lower Mg/Al ratios in the interior parts of the chimneys and deeper in the sediment which leads to the precipitation of phyllosilicates with lower Mg contents. Talc and kerolite-smectite have very low trace- and rare earth element contents. Some exhibit a negative or flat Eu anomaly, which suggests Eu depletion in the original hydrothermal fluid. Such Eu depletion could be caused by precipitation of anhydrite or barite (sinks for Eu2+) deeper in the system. REE abundances and distribution patterns indicate that chlorite and chlorite-smectite are hydrothermal alteration products of the background turbiditie sediment. (C) 2007 Elsevier B.V. All rights reserved.
机译:对来自六个海底热液区的沉积物,烟囱和块状硫化物中的滑石,硅藻土,绿土,绿泥石和绿泥石样品进行了矿物学,化学和氧同位素分析。样品来自橄榄岩和玄武岩托管的热液系统,而玄武岩系统包括无沉积物和沉积物覆盖的场所。以前已经将海底热液场所的页硅酸镁描述为滑石,硅镁石或皂石。相比之下,新数据显示三面体Mg-页硅酸盐从纯滑石和富铁滑石,到富含高岭石的高岭石-蒙脱石,再到富含蒙脱石的高岭石-蒙脱石和三八面体蒙脱石。最常见的现象是混合层的硅藻土-蒙脱石,它显示出几乎完整的层间化系列,其中有5%至85%的蒙皂石层。与硅藻土层合的蒙脱石大部分为三八面体。随着滑石层中蒙脱石层比例的增加,粘土序列的晶体完善度通常从滑石粉降低至硅藻土-蒙脱石,而晶体完善度较低。我们的研究不支持沉淀矿物对热液系统类型/亚型的任何依赖性。氧同位素地热法表明,滑石和硅藻土沉积在烟囱,块状硫化物堆中,沉积物表面以及海底附近沉积物中的开放裂缝中是高温(> 250摄氏度)相,这很可能是聚焦相的结果。液体排出。该三八面体镁-页硅酸盐序列的另一个末端成员是蒙脱石,是在沉积物中深处形成的中等温度(200-250摄氏度)相(类似于0.8英寸)。构成热液丘周围蚀变沉积物基质的亚氯酸盐和绿泥石-绿土,是通过分散流体通过热液管道周围的沉积物排放而产生的较低温度(150-200摄氏度)相。除温度外,对该序列沉淀的其他两个控制是二氧化硅活性和Mg / Al比(即海水与热液的混合程度)。相对于三八面体蒙脱石,较高的二氧化硅活性有利于滑石的形成。通风孔结构和沉积物覆盖层无法使热液与周围的海水完全混合,从而导致烟囱内部的Mg / Al比值降低,而沉积物中的深度更深,从而导致Mg含量较低的层状硅酸盐沉淀。滑石和硅藻土中的痕量和稀土元素含量非常低。有些表现出负的或平坦的Eu异常,这表明原始热液中的Eu耗尽。这种Eu耗尽可能是由于系统中较深的硬石膏或重晶石(Eu2 +的沉)的沉淀所致。稀土元素的丰度和分布规律表明,绿泥石和绿泥石-绿土是本底浊积沉积物的热液蚀变产物。 (C)2007 Elsevier B.V.保留所有权利。

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