期刊文献+
共找到5篇文章
< 1 >
每页显示 20 50 100
A primitive mantle source for the Neoarchean mafic rocks from the Tanzania Craton 被引量:7
1
作者 Y.A.Cook I.V.Sanislav +2 位作者 J.Hammerli T.G.Blenkinsop P.H.G.M.Dirks 《Geoscience Frontiers》 SCIE CAS CSCD 2016年第6期911-926,共16页
Mafic rocks comprising tholeiitic pillow basalt, dolerite and minor gabbro form the basal stratigraphic unit in the ca. 2.8 to 2.6 Ga Geita Greenstone Belt situated in the NW Tanzania Craton. They outcrop mainly along... Mafic rocks comprising tholeiitic pillow basalt, dolerite and minor gabbro form the basal stratigraphic unit in the ca. 2.8 to 2.6 Ga Geita Greenstone Belt situated in the NW Tanzania Craton. They outcrop mainly along the southern margin of the belt, and are at least 50 million years older than the supracrustal assemblages against which they have been juxtaposed. Geochemical analyses indicate that parts of the assemblage approach high Mg-tholeiite (more than 8 wt.% MgO). This suite of samples has a restricted compositional range suggesting derivation from a chemically homogenous reservoir. Trace element modeling suggests that the mafic rocks were derived by partial melting within the spinel peridotite field from a source rock with a primitive mantle composition. That is, trace elements maintain primitive mantle ratios (Zr/Hf = 32-35, Ti/Zr - 107-147), producing flat REE and HFSE profles [(La/Yb)pm = 0.9 -1.3], with abundances of 3-10 times primitive mantle and with minor negative anomalies of Nb [(Nb/ La)pm - 0.6-0.8] and Th [(Th/La)pm = 0.6-0.9]. Initial isotope compositions (εNd) range from 1.6 to 2.9 at 2.8 Ga and plot below the depleted mantle line suggesting derivation from a more enriched source compared to present day MORB mantle. The trace element composition and Nd isotopic ratios are similar to the mafic rocks outcropping -50 km south. The mafic rocks outcropping in the Geita area were erupted through oceanic crust over a short time period, between -2830 and-2820 Ma; are compositionally homogenous, contain little to no associated terrigenous sediments, and their trace element composition and short emplacement time resemble oceanic plateau basalts. They have been interpreted to be derived from a plume head with a primitive mantle composition. 展开更多
关键词 Mafic rocks Archean tanzania craton Primitive mantle MORB Oceanic plateau
下载PDF
Apatite fission track and (U-Th)/He thermochronology from the Archean Tanzania Craton: Contributions to cooling histories of Tanzanian basement rocks
2
作者 Charles H. Kasanzu 《Geoscience Frontiers》 SCIE CAS CSCD 2017年第5期999-1007,共9页
Borehole and surface samples from the Archean Tanzania Craton were analysed for apatite fission track(AFT) and(U-Th)/He data with the aim of deciphering cooling histories of the basement rocks. Fission track dates fro... Borehole and surface samples from the Archean Tanzania Craton were analysed for apatite fission track(AFT) and(U-Th)/He data with the aim of deciphering cooling histories of the basement rocks. Fission track dates from borehole and outcrop samples are Carboniferous-Permian(345± 33.3 Ma to271±31.7 Ma) whereas(U-Th)/He dates are Carboniferous-Triassic(336±45.8 Ma to 213±29 Ma) for outcrop grains and are consistently younger than corresponding AFT dates. Single grain(U-Th)/He dates from the borehole are likely to be flawed by excessive helium implantation due to their very low effective uranium contents, radiation damage and grain sizes. All AFT and(U-Th)/He dates are significantly younger than the stratigraphic ages of their host rocks, implying that the samples have experienced Phanerozoic elevated paleo-temperatures. Considerations of the data indicate removal of up to 9 km overburden since the Palaeozoic.Thermal modelling reveals a protracted rapid cooling event commencing during the early Carboniferous(ca. 350 Ma) at rates of 46 m/Ma ending in the Triassic(ca. 220 Ma). The model also suggests minor cooling during the Cretaceous of the samples to surface temperatures. The suggested later cooling event remains to be tested. The major cooling phase during the Carboniferous is interpreted to be associated with compressional tectonics during the Variscan Orogeny sensu far field induced stresses. Coeval sedimentation in the Karoo basins in the region suggests that most of the cooling of cratonic rocks during the Carboniferous was associated with denudation. 展开更多
关键词 THERMOCHRONOLOGY EXHUMATION tanzania craton
下载PDF
Seismic Potential of the Dodoma Area Within the Manyara Dodoma Rift Segment,Tanzania
3
作者 Athanas S.Macheyeki Damien Delvaux +1 位作者 Marc De Batist Abdulkarim Mruma 《地学前缘》 EI CAS CSCD 北大核心 2009年第S1期53-53,共1页
On 5th November 2003,the central part of Tanzania (Dodoma),located within the eastern branch of the East African Rift System was struck by an M_s 5.5 earthquake that destroyed a school,a dispensary near its epicenter ... On 5th November 2003,the central part of Tanzania (Dodoma),located within the eastern branch of the East African Rift System was struck by an M_s 5.5 earthquake that destroyed a school,a dispensary near its epicenter and caused a huge crack on the Parliamentary building of Tanzania.This was one of the relatively large earthquakes that affected the area after the M_s 6.1 that occurred north of the Dodoma within the Manyara-Dodoma rift segment in May 7, 展开更多
关键词 tanzania craton EAST AFRICAN RIFT system tanzania DIVERGENT zone Manyara-Dodoma RIFT SEGMENT seismic risk assessment
下载PDF
坦桑尼亚Kagera地区地质成矿条件与找矿前景预测 被引量:3
4
作者 王武名 张遵忠 《有色金属》 CSCD 北大核心 2010年第3期137-141,共5页
分析坦桑尼亚Kagera地区地质成矿条件,预测找矿前景。坦桑尼亚西北部的Kagera地区,地处著名的Kibaran造山带东缘,经历了多次构造-岩浆活动,变质作用强烈,地质演化历史复杂,具备了较好的成矿条件。在Kagera地区的大岩体发现超大型的Kaba... 分析坦桑尼亚Kagera地区地质成矿条件,预测找矿前景。坦桑尼亚西北部的Kagera地区,地处著名的Kibaran造山带东缘,经历了多次构造-岩浆活动,变质作用强烈,地质演化历史复杂,具备了较好的成矿条件。在Kagera地区的大岩体发现超大型的Kabanga镍矿,而且其他小的基性-超基性岩体均有矿化。区域的北部出现类似于Kabanga镍矿的较强磁异常。中西部沿石英岩和泥岩接触带出露串珠状辉长岩,辉长岩中常见石英细脉,局部见星点状黄铁矿、黄铜矿硫化物。中部发现两个大的磁异常及地球化学Ni异常。地质工作表明,Kagera地区对于寻找与正岩浆有关的铜镍硫化物矿床有较好前景。 展开更多
关键词 地质找矿 镍矿 坦桑尼亚克拉通 Kibaran造山带 东非镍带
下载PDF
坦桑尼亚东马拉金矿矿床地质特征及找矿方向
5
作者 周雷 陈志友 陆国章 《世界有色金属》 2020年第3期66-68,共3页
坦桑尼亚东马拉金矿位于马拉-穆索马绿岩带上的马拉绿岩带,是近期在马拉绿岩带上发现的又一中型金矿床。赋金地质体为太古代尼安兹系的片麻岩、片岩,蚀变类型有硅化、黄(磁黄)铁矿化、碳酸盐化及粘土化,偶见方铅矿化;矿体呈脉状和透镜状... 坦桑尼亚东马拉金矿位于马拉-穆索马绿岩带上的马拉绿岩带,是近期在马拉绿岩带上发现的又一中型金矿床。赋金地质体为太古代尼安兹系的片麻岩、片岩,蚀变类型有硅化、黄(磁黄)铁矿化、碳酸盐化及粘土化,偶见方铅矿化;矿体呈脉状和透镜状,金矿物主要为自然金;矿床类型为中温热液脉型金矿床;矿区主要为石英脉型金矿。加强金矿体产出特征研究,寻找有利含金构造部位,有望扩大找矿远景。 展开更多
关键词 坦桑尼亚 克拉通 尼安兹系 绿岩带 变质热液
下载PDF
上一页 1 下一页 到第
使用帮助 返回顶部