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901.
The Kooh-Shah region located in a Tertiary volcanic-plutonic belt of the Lut Block in eastern Iran comprises several subvolcanic intermediate to acidic intrusive rocks, diorite to syenite in composition, which have intruded into volcanic rocks. The Kooh-Shah granitoid rocks are characterized by enrichment in large ion-lithophile elements (LILE: e.g. Sr, Ba, Rb) and depletion in high field-strength elements (HFSE: e.g. Nb, Ta, Ti). The chondrite-normalized REE patterns are characterized by moderate LREE enrichment (La/Yb)N=6.01-10.01, medium-heavy REE enrichment, and absence of Eu anomalies. The Kooh-Shah intrusive rocks are metaluminous, shoshonitic with calc-alkaline affinity and high values of magnetic susceptibility, and classified as the magnetite-series of oxidant I-type granitoids. The age of Kooh-Shah granitoid rocks based on zircon U-Pb age dating is 39.7±0.7 Ma (=Middle Eocene) and the ranges of their initial 87Sr/86Sr and 143Nd/144Nd ratios are from 0.704812 to 0.704920 and 0.512579 to 0.512644, respectively, when recalculated to an age of 39 Ma. The initial ?Nd isotope values for the Kooh-Shah intrusive rocks range from -0.18 to 1.09. This geochemical data indicates that the Kooh-Shah granitoid rocks formed from depleted mantle in an island arc setting. The geochemical signature of the studied granitoid rocks represents a characteristic guide for future exploration of copper-gold porphyry-type deposits in the Lut block.  相似文献   
902.
通过对茶梁子矿区的地质背景、矿体特征、矿石特征及岩石地球化学特征进行综合研究,初步探讨了矿床的成因。认为矿体是由含硫质的低温热液携带矿质运移到断裂构造的有利部位沉淀而形成的。同时在表生环境下,原生矿体经过后期的次生改造作用后,形成了富含铁、锰氧化物的土状矿石,并且以较为富集的铁、锰氧化物作为寻找钴的直接标志。  相似文献   
903.
研究区属复杂景观地球化学区,取样位置经常位移,样品高值点难以确定.常规方法圈定化探弱异常范围大,异常中心不明显.经化探数据规格化、聚类分析、因子分析及综合衬度计算圈定的化探异常指导野外找矿,发现多处铜矿体(点).  相似文献   
904.
通过对济宁北矿区区域构造特征以及区内各井田地质资料的统计研究分析,系统总结了该矿区断层构造的发育特征和展布组合规律。研究发现:在区域上,研究区构造以断裂为主,且规模和强度较大,褶皱强度小,均为宽缓褶皱。矿区内的主要断裂有两组,一组为SN向的区域性断裂,构成井田边界,另一组为由其附生的NE向断裂,使其开采地质条件复杂化。区内NE向褶皱发育,多呈背、向斜相间分布。  相似文献   
905.
Over much of arid Western Australia a red and brown hardpan occurs on broad plains; it may lie either on the surface or buried beneath a shallow mantle of soil. It is proposed that, because of its lithological character and its considerable thickness and extent, it should be given the name of Wiluna Hardpan. The proposed type section is north of Wiluna, near Bulloo Downs homestead, where headward erosion of the Ashburton River is exposing sections 30 m deep. Although both ferruginous and calcareous cement may be present, Wiluna Hardpan is largely indurated with silica. It is younger than laterite, but broadly contemporaneous with calcrete and Robe Pisolite. Initially it was probably geographically restricted by a coincidence of suitable conditions of low relief and a climate resulting in episodic flooding and desiccation. Its present distribution is partly controlled by current erosional and depositional processes.  相似文献   
906.
Lord Howe Island is the eroded remnant of a large shield volcano. Tholeiitic lavas of the North Ridge Basalt comprise the main shield building phase and were erupted about 6.9 Ma ago. The Boat Harbour Breccia probably formed within the throat of the volcano and, together with the North Ridge Basalt, is intruded by numerous basaltic dykes, which grade into a cone sheet complex near the main vent. Large scale collapse of the summit area of the volcano produced a caldera which was filled rapidly by lavas of the Mount Lidgbird Basalt some 6.4 Ma ago, bringing to a close the volcanic history of Lord Howe Island. The shield volcano thus was built during a short interval in the late Miocene.

Palaeomagnetic data show that the North Ridge Basalt and the Mount Lidgbird Basalt were erupted during periods when the geomagnetic field had normal polarity, and that their formation was separated by at least one interval of reversed polarity when the dykes and cone sheets were emplaced. The directions of magnetisation for the lavas and intrusives are such that, palaeomagnetically, no movement of Lord Howe Island is detected since its formation.

Lord Howe Island is the subaerial part of a large seamount which lies at the southern end of a northerly‐trending line of volcanic seamounts extending for more than 1000 km. The Lord Howe seamount chain probably was produced by movement of the Australian lithospheric plate over a magma source or hot spot located below the plate within the upper mantle. Other data suggest that the Australian plate is moving N at about 6 cm/a and from this it is predicted that the seamount underlying Nova Bank, at the northern end of the chain, was constructed by volcanic activity about 23 Ma ago. Similarly, if volcanism were to occur now in the Lord Howe seamount chain we predict that its location would be about 400 km S of Lord Howe Island.  相似文献   
907.
A ~400 km long deep crustal reflection seismic survey was acquired in central Victoria, Australia, in 2006. It has provided information on crustal architecture across the western Lachlan Orogen and has greatly added to the understanding of the tectonic evolution. The east-dipping Moyston Fault is confirmed as the suture between the Delamerian and western Lachlan Orogens, and is shown to extend down to the Moho. The Avoca Fault, the boundary between the Stawell and Bendigo Zones, is a west-dipping listric reverse fault that intersects the Moyston Fault at a depth of about 22 km, forming a V-shaped geometry. Both the Stawell and Bendigo Zones can be divided broadly into a lower crustal region of interlayered and imbricated metavolcanic and metasedimentary rocks and an upper crustal region of tightly folded metasedimentary rocks. The Stawell Zone was probably part of a Cambrian accretionary system along the eastern Gondwanaland margin, and mafic rocks may have been partly consumed by Cambrian subduction. Much of the Early Cambrian oceanic crust beneath the Bendigo Zone was not subducted, and is preserved as a crustal-scale imbricate thrust stack. The seismic data have shown that a thin-skinned structural model appears to be valid for much of the Melbourne Zone, whereas the Stawell and Bendigo Zones have a thick-skinned structural style. Internal faults in the Stawell and Bendigo Zones are mostly west-dipping listric faults, which extend from the surface to near the base of the crust. The Heathcote Fault Zone, the boundary between the Bendigo and Melbourne Zones, extends to at least 20 km, and possibly to the Moho. A striking feature in the seismic data is the markedly different seismic character of the mid to lower crust of the Melbourne Zone. The deep seismic reflection data for the Melbourne Zone have revealed a multilayered crustal structure that supports the Selwyn Block model.  相似文献   
908.
The molybdenite and scheelite mineralisation in the Native Dog Pluton at Monkey Gully near Yea is hosted within an I-type (post-orogenic) pluton, which shows extensive fractionation and magma mixing, and was emplaced in an extensional environment. The pluton comprises four principal rock types: tonalite, granodiorite, dacite and leucogranite. Emplacement of the pluton was in an extensional northwest to southeast paleostress field. Early extensional quartz veins, related to cooling, are overprinted by both dacitic dykes and late-stage quartz sheeted veins. The late-stage veins host the molybdenum and tungsten mineralisation in the deposit. 206Pb/238U zircon ages of 356 ±14 Ma and 375 ± 22 Ma place pluton formation and mineralisation at the onset of the Kanimblan Orogeny and later than other major molybdenum deposits in Victoria. Key factors governing the source for the granite and its associated mineralisation are: (1) the presence of a highly fractionated and sulfur-rich leucogranite; and (2) the pluton's location in a regional jog overlying the Selwyn basement block. Finally, a model is developed to explain the differences between this Melbourne Zone molybdenum and tungsten deposit compared with other metallogenic porphyry deposits.  相似文献   
909.
出露于扬子地块西南缘的盐边群为一套火山-沉积岩系,其深入研究对探讨扬子西缘新元古代构造环境具有重要意义.本文对盐边群中碎屑沉积岩进行了较系统的岩石学、碎屑物质组成和地球化学研究,并从小坪组和乍古组中各选取了1件变质砂岩样品进行锆石U-Pb年龄和Hf同位素分析.变质砂岩主要由棱角状-次棱角状火山岩岩屑、石英和长石矿物碎屑组成.碎屑沉积岩Al2O3/SiO2值为0.12~0.4,K2O/Na2O值范围为0.14 ~9.45(其中板岩K2O/Na2O值多大于1.0,而变质砂岩中多数样品的K2O/Na2O值小于1.0).所有样品具有轻-中等程度的轻重稀土元素分异((La/Yb)N=1.6 ~9.37),多数样品具有明显的负Eu异常.εNd(t)值范围为-1.77~ +5.01.变质砂岩碎屑锆石U-Pb年龄峰值为900~ 910Ma,同时存在少量太古代-古元古代碎屑锆石.小坪组和乍古组变质砂岩中年轻碎屑锆石206pb/238U年龄加权平均值分别为888±8Ma和884±14Ma.碎屑物质组成、地球化学和锆石U-Pb年龄结果共同表明,盐边群碎屑沉积为近源沉积,物源区主要为岛孤中酸性火山岩和花岗岩.结合关刀山岩体(857Ma)和荒田组玄武岩(880~830Ma)研究结果,进一步限定盐边群的时代为880~830Ma,形成于弧后盆地环境,其沉积物源区为华夏地块向扬子地块俯冲过程中,扬子西南缘形成的火山岛孤.  相似文献   
910.
华北地块南缘黑山-木龙沟地区晚中生代中酸性岩的LA-ICPMS锆石U-Pb定年结果表明,黑山下斜辉石黑云母闪长岩和木龙沟花岗闪长斑岩的成岩年龄分别为154±2Ma(2σ,N=16)和151±1Ma(2σ,N=15).该中酸性岩的A/CNK=0.75~1.04,Na2O+ K2O =6.15% ~8.42%,K2O/Na2O =0.77 ~2.29,属于准铝质-弱过铝质和高钾钙碱性/钾玄岩系列.在稀土和微量元素上,富集LREE和Rb、Ba、K、Pb、Sr等大离子亲石元素,亏损HREE和Zr、Hf、Ta、Nb、P、Ti等高场强元素,具有弱的负铕异常(δEu=0.85~0.99).在同位素上,全岩的ISr为0.708676~0.711480,εNd(t)变化于-22 ~-16.1之间,tDM2为2.25~2.72Ga;锆石的εHf(t)为-27.8~-18.4,二阶段模式年龄tDM2为2.37~2.96Ga.岩石地球化学和Sr-Nd-Hf同位素组成特征显示,这些中酸性岩的源区物质由古老的壳源物质和年轻组分组成,其中以壳源物质为主,可能为太古宙太华群.岩相学和区域地质特征显示,年轻组分可能为幔源组分,岩体可能是由底侵的幔源岩浆与其诱发部分熔融的壳源岩浆混合形成的.  相似文献   
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