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红土型风化壳和次生锰矿床形成于温暖和潮湿的古气候条件 ,其中含有丰富的表生钾锰矿物。因此 ,对表生钾锰矿物进行精确的40 Ar/ 3 9Ar年龄测定 ,不仅能查明大陆化学风化和矿床次生富集的时间和过程 ,而且可以为区域古气候的反演提供重要的年代学资料。透射电子显微镜、热重分析、离子交换实验和40 Ar/ 3 9Ar同位素分析表明 ,层状结构的黑锌锰矿、锂锰矿和钠水锰矿以及具有 1× 1隧道结构的软锰矿不适合于40 Ar/ 3 9Ar年龄测定 ;而隐钾锰矿、锰钡矿和锰铅矿因具有致密和稳定的 2× 2隧道结构及很强的保存K Ar体系的能力 ,是40 Ar/ 3 9Ar同位素定年的理想对象。硬锰矿和钙锰矿分别具有 2× 3和 3× 3隧道结构 ,由于隧道孔径过大 ,晶体结构的稳定性较差 ,其作为40Ar/ 3 9Ar测年的适用性有待于进一步证实。采用精细的激光阶段加热技术 ,可以有效克服表生钾锰矿物40 Ar/ 3 9Ar测年过程中3 9ArK 的反冲损失、多世代表生钾锰矿物的共生 ,以及表生钾锰矿物中原生矿物的污染和过量大气氩的存在等问题 ,并获得有意义的风化年龄。已有数据表明 ,表生钾锰矿物的形成主要集中在白垩纪末期、始新世末期—渐新世早期、中新世和上新世中期等 4个时期 ,可能记录了地史时期周期性的化学风化及气候的交替演变 相似文献
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ALESSANDRA SPADAFORA EDOARDO PERRI† JUDITH A. MCKENZIE CRISÓGONO VASCONCELOS Associate Editor: Gert-Jan Reichart 《Sedimentology》2010,57(1):27-40
Modern Ca:Mg carbonate stromatolites form in association with the microbial mat in the hypersaline coastal lagoon, Lagoa Vermelha (Brazil). The stromatolites, although showing diversified fabrics characterized by thin or crude lamination and/or thrombolitic clotting, exhibit a pervasive peloidal microfabric. The peloidal texture consists of dark, micritic aggregates of very high‐Mg calcite and/or Ca dolomite formed by an iso‐oriented assemblage of sub‐micron trigonal polyhedrons and organic matter. Limpid acicular crystals of aragonite arranged in spherulites surround these aggregates. Unlike the aragonite crystals, organic matter is present consistently in the dark, micritic carbonate comprising the peloids. This organic matter is observed as sub‐micron flat and filamentous mucus‐like structures inside the interspaces of the high‐Mg calcite and Ca dolomite crystals and is interpreted as the remains of degraded extracellular polymeric substances. Moreover, many fossilized bacterial cells are associated strictly with both carbonate phases. These cells consist mainly of 0·2 to 4 μm in diameter, sub‐spherical, rod‐like and filamentous forms, isolated or in colony‐like clusters. The co‐existence of fossil extracellular polymeric substances and bacterial bodies, associated with the polyhedrons of Ca:Mg carbonate, implies that the organic matter and microbial metabolism played a fundamental role in the precipitation of the minerals that form the peloids. By contrast, the lack of extracellular polymeric substances in the aragonitic phase indicates an additional precipitation mechanism. The complex processes that induce mineral precipitation in the modern Lagoa Vermelha microbial mat appear to be recorded in the studied lithified stromatolites. Sub‐micron polyhedral crystal formation of high‐Mg calcite and/or Ca dolomite results from the coalescence of carbonate nanoglobules around degraded organic matter nuclei. Sub‐micron polyhedral crystals aggregate to form larger ovoidal crystals that constitute peloids. Subsequent precipitation of aragonitic spherulites around peloids occurs as micro‐environmental water conditions around the peloids change. 相似文献
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PATRICK MEISTER† JUDITH A. MCKENZIE† CRISOGONO VASCONCELOS† STEFANO BERNASCONI† MARTIN FRANK‡ MARCUS GUTJAHR§ DANIEL P. SCHRAG¶ 《Sedimentology》2007,54(5):1007-1032
Early diagenetic dolomite beds were sampled during the Ocean Drilling Programme (ODP) Leg 201 at four reoccupied ODP Leg 112 sites on the Peru continental margin (Sites 1227/684, 1228/680, 1229/681 and 1230/685) and analysed for petrography, mineralogy, δ13C, δ18O and 87Sr/86Sr values. The results are compared with the chemistry, and δ13C and 87Sr/86Sr values of the associated porewater. Petrographic relationships indicate that dolomite forms as a primary precipitate in porous diatom ooze and siliciclastic sediment and is not replacing the small amounts of precursor carbonate. Dolomite precipitation often pre‐dates the formation of framboidal pyrite. Most dolomite layers show 87Sr/86Sr‐ratios similar to the composition of Quaternary seawater and do not indicate a contribution from the hypersaline brine, which is present at a greater burial depth. Also, the δ13C values of the dolomite are not in equilibrium with the δ13C values of the dissolved inorganic carbon in the associated modern porewater. Both petrography and 87Sr/86Sr ratios suggest a shallow depth of dolomite formation in the uppermost sediment (<30 m below the seafloor). A significant depletion in the dissolved Mg and Ca in the porewater constrains the present site of dolomite precipitation, which co‐occurs with a sharp increase in alkalinity and microbial cell concentration at the sulphate–methane interface. It has been hypothesized that microbial ‘hot‐spots’, such as the sulphate–methane interface, may act as focused sites of dolomite precipitation. Varying δ13C values from −15‰ to +15‰ for the dolomite are consistent with precipitation at a dynamic sulphate–methane interface, where δ13C of the dissolved inorganic carbon would likewise be variable. A dynamic deep biosphere with upward and downward migration of the sulphate–methane interface can be simulated using a simple numerical diffusion model for sulphate concentration in a sedimentary sequence with variable input of organic matter. Thus, the study of dolomite layers in ancient organic carbon‐rich sedimentary sequences can provide a useful window into the palaeo‐dynamics of the deep biosphere. 相似文献
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PATRICK MEISTER† STEFANO M. BERNASCONI IVANO W. AIELLO‡ CRISÓGONO VASCONCELOS JUDITH A. MCKENZIE 《Sedimentology》2009,56(5):1552-1568
The occurrence of early diagenetic Ca‐rhodochrosite [(Mn,Ca)CO3] is reported in association with ‘griotte’‐type nodular limestones from basinal settings in the geological record; however, without the comparison of analogous modern examples, the controls on precipitation remain speculative. Here the findings of four layers of primary Ca‐rich rhodochrosite recovered from a modern deep‐sea setting in the Eastern Equatorial Pacific, from bioturbated sediments 300 m below sea floor, are reported (Ocean Drilling Program, Leg 201, Site 1226). The mineralogy is similar to cements in burrows recovered during Deep Sea Drilling Project Leg 68 at Eastern Equatorial Pacific Site 503 and from Ca‐rhodochrosite laminae in sediments of the central Baltic Sea. Petrographic relationships and constant oxygen isotopic compositions in the Ca‐rhodochrosite around 5‰ at all depths indicate a shallow burial depth of formation. The onset of 1‰ heavier oxygen isotope composition of Ca‐rhodochrosite at Site 503, about 30 m below the Pliocene/Pleistocene boundary, further suggests that precipitation occurs in the range of 30 m below sea floor. The approximate depth of formation allowed an approximate empirical fractionation factor for marine Ca‐rhodochrosite to be constrained that strongly differs from previously published theoretical values. Based on the approximate precipitation depth, authigenic Ca‐rhodochrosite forms within the SO42?‐reduction zone. Moderately negative δ13C values (around ?3‰) and total organic carbon lower than 2 wt% indicate a relatively low contribution of CO32? from organic C mineralization within the expanded redox zonation in the Eastern Equatorial Pacific. It is suggested that the alkalinity is increased by a rise in pH at focused sites of Mn‐reduction coupled with S2? oxidation. High concentrations of Mn‐oxide can accumulate in layers or burrows because of Mn‐cycling in suboxic sediments as suggested for the Baltic Sea Ca‐rhodochrosites. This study demonstrates how early diagenetic precipitates document biogeochemical processes from past diagenetic systems. 相似文献
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Dolomite formation within microbial mats in the coastal sabkha of Abu Dhabi (United Arab Emirates) 总被引：1，自引：0，他引：1
TOMASO R. R. BONTOGNALI CRISÓGONO VASCONCELOS ROLF J. WARTHMANN STEFANO M. BERNASCONI CHRISTOPHE DUPRAZ CHRISTIAN J. STROHMENGER JUDITH A. McKENZIE 《Sedimentology》2010,57(3):824-844
Microbial mediation is the only demonstrated mechanism to precipitate dolomite under Earth surface conditions. A link between microbial activity and dolomite formation in the sabkha of Abu Dhabi has, until now, not been evaluated, even though this environment is cited frequently as the type analogue for many ancient evaporitic sequences. Such an evaluation is the purpose of this study, which is based on a geochemical and petrographic investigation of three sites located on the coastal sabkha of Abu Dhabi, along a transect from the intertidal to the supratidal zone. This investigation revealed a close association between microbial mats and dolomite, suggesting that microbes are involved in the mineralization process. Observations using scanning electron microscopy equipped with a cryotransfer system indicate that authigenic dolomite precipitates within the exopolymeric substances constituting the microbial mats. In current models, microbial dolomite precipitation is linked to an active microbial activity that sustains high pH and alkalinity and decreased sulphate concentrations in pore waters. Such models can be applied to the sabkha environment to explain dolomite formation within microbial mats present at the surface of the intertidal zone. By contrast, these models cannot be applied to the supratidal zone, where abundant dolomite is present within buried mats that no longer show signs of intensive microbial activity. As no abiotic mechanism is known to form dolomite at Earth surface conditions, two different hypotheses can reconcile this result. In a first scenario, all of the dolomite present in the supratidal zone formed in the past, when the mats were active at the surface. In a second scenario, dolomite formation continues within the buried and inactive mats. In order to explain dolomite formation in the absence of active microbial metabolisms, a revised microbial model is proposed in which the mineral‐template properties of exopolymeric substances play a crucial role. 相似文献
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M. A. R. VASCONCELOS K. WÜNNEMANN A. P. CRÓSTA E. C. MOLINA W. U. REIMOLD E. YOKOYAMA 《Meteoritics & planetary science》2012,47(10):1659-1670
Forward modeling is commonly applied to gravity field data of impact structures to determine the main gravity anomaly sources. In this context, we have developed 2.5‐D gravity models of the Serra da Cangalha impact structure for the purpose of investigating geological bodies/structures underneath the crater. Interpretation of the models was supported by ground magnetic data acquired along profiles, as well as by high resolution aeromagnetic data. Ground magnetic data reveal the presence of short‐wavelength anomalies probably related to shallow magnetic sources that could have been emplaced during the cratering process. Aeromagnetic data show that the basement underneath the crater occurs at an average depth of about 1.9 km, whereas in the region beneath the central uplift it is raised to 0.5–1 km below the current surface. These depths are also supported by 2.5‐D gravity models showing a gentle relief for the basement beneath the central uplift area. Geophysical data were used to provide further constraints for numeral modeling of crater formation that provided important information on the structural modification that affected the rocks underneath the crater, as well as on shock‐induced modifications of target rocks. The results showed that the morphology is consistent with the current observations of the crater and that Serra da Cangalha was formed by a meteorite of approximately 1.4 km diameter striking at 12 km s?1. 相似文献
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Dolomite Mountains and the origin of the dolomite rock of which they mainly consist: historical developments and new perspectives 总被引：3，自引：0，他引：3
Beginning in the late 18th Century, the Dolomite Mountains in Northern Italy have been the location for major sedimentological developments, from the discovery of the mineral dolomite to the formulation of the coral-reef hypothesis to explain the origin of the massive dolomite structures that define the splendid scenery of the region. Further, the Dolomite Mountains have inspired voluminous research into the origin of dolomite, questioning whether dolomite is a primary precipitate or a secondary replacement product. Recently, with the recognition that microbes can mediate dolomite precipitation, a new geomicrobiological approach, combining the study of modern natural environments with bacterial culture experiments, is now being used to calibrate or interpret microbial evidence derived from the dolomite rock record. This three-pronged methodology applied to the study of dolomite formation holds great promise for future research into the 'Dolomite Problem' and provides a new impetus to revisit the Dolomite Mountains in the 21st Century. 相似文献
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氧化锰矿是我国仅次于沉积型碳酸锰矿的重要锰矿床类型,主要分布在广西、湖南、广东和福建等南方省区,但由于定年手段的限制,迄今对我国氧化锰矿形成时代的了解还极其有限.作者近几年利用激光阶段加热40Ar/39Ar同位素分析技术对华南地区典型氧化锰矿进行了系统和精确的年龄测定,获得了一大批可靠的成矿年龄,年龄值介于23.64 ± 0.29 Ma和0.48 ± 0.17 Ma (2σ),表明华南氧化锰矿的大规模成矿至少在渐新世末-中新世初就已开始并一直持续到更新世末期.基于多数氧化锰矿的上部矿石已被剥蚀或开采殆尽这一事实,可将华南氧化锰矿的成矿时间上溯到渐新世早期甚至始新世末期.研究发现,氧化锰矿的保存程度和年龄分布明显受新构造运动的影响;如果剔除后期剥蚀程度和采样系统性的影响,可以认为华南氧化锰矿的形成在区域上具有同时性.本次研究还说明,次生氧化锰矿的成矿是一个极其漫长的过程,形成一个具有工业意义的氧化锰矿可能需要上千万年的时间;这明显有别于多数内生热液矿床的成矿.本项研究为我国氧化锰矿以及其他类型的风化矿床(如红土型金矿和红土型镍矿)的年代学研究提供了新的思路和途径. 相似文献
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Thomas KENKMANN Marcos A. R. VASCONCELOS Alvaro P. CRÓSTA Wolf U. REIMOLD 《Meteoritics & planetary science》2011,46(6):875-889
Abstract– Serra da Cangalha is a complex impact structure with a crater diameter of 13,700 m and a central uplift diameter of 5800 m. New findings of shatter cones, planar fractures, feather features, and possible planar deformation features are presented. Several ring‐like features that are visible on remote sensing imagery are caused by selective erosion of tilted strata. The target at Serra da Cangalha is composed of Devonian to Permian sedimentary rocks, mainly sandstones that are interlayered with siltstone and claystones. NNE–SSW and WNW–ESE‐striking joint sets were present prior to the impact and also overprinted the structure after its formation. As preferred zones of weakness, these joint sets partly controlled the shape of the outer perimeter of the structure and, in particular, affected the deformation within the central uplift. Joints in radial orientation to the impact center did not undergo a change in orientation during tilting of strata when the central uplift was formed. These planes were used as major displacement zones. The asymmetry of the central uplift, with preferred overturning of strata in the northern to western sector, may suggest a moderately oblique impact from a southerly direction. Buckle folding of tilted strata, as well as strata overturning, indicates that the central uplift became gravitationally unstable at the end of crater formation. 相似文献
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