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161.
王松  李双应  杨栋栋  何刚  赵大千 《岩石学报》2012,28(8):2453-2465
本文通过对天山南缘石炭系-三叠系碎屑岩岩石学特征和地球化学特征的分析,揭示了研究区石炭系-三叠系碎屑岩的物质组分特征及其物源区的大地构造背景.碎屑岩的岩石学、地球化学分析表明,天山南缘石炭系、三叠系砂岩成分成熟度和结构成熟度均不高,杂基含量较高,从石炭系至三叠系砂岩不稳定组分依次增加.石炭系、二叠系具有相似的稀土元素含量特征,三叠系稀土元素含量明显低于石炭系和二叠系,石炭系-三叠系轻、重稀土元素分馏程度依次减弱,La/Th、La/Y 比值依次增大,Th/U比值减小,来自再旋回的物质依次增多.综合碎屑组分、常量元素、稀土元素及微量元素特征的判别,天山南缘石炭系物源区构造背景为既有指示大陆岛孤、活动大陆边缘的证据,也有指示为被动大陆边缘,二叠系物源区示为大陆岛弧,三叠系物源区示为大陆岛弧和含有古老沉积岩的陆块.对比石炭系、二叠系及三叠系物源区的大地构造属性,石炭系物源区示有多种属性,而二叠系、三叠系则相对较为单一,这可能与中天山-伊犁地块和塔里木陆块的碰撞有关.  相似文献   
162.
《International Geology Review》2012,54(16):1980-1999
ABSTRACT

The formation of the Three Gorges (TG), the most important capture point along the Yangtze River, has been debated since the last century. Most of hypotheses on its formation are based on the timing of unconformities detected in the sedimentary basins along the riverbed. These unconformities may mark periods of tectonic activity and enhanced hydrodynamic condition. Herein, we detail the Cenozoic sedimentary provenance of the Jianghan Basin through LA-ICP-MS zircon U-Pb geochronology and heavy mineral analyses. The obtained data suggest that during Palaeocene-Oligocene time, the Jianghan Basin was supplied by sediments from the nearby mountain belts. However, the occurrence of zircons with ages <32 Ma above the unconformity at ~24.6 Ma indicates a provenance from Cenozoic igneous rocks which are exposed only in the Qiangtang Block and the Songpan-Ganzi Orogen. We propose therefore that the TG formed between the late Oligocene and the early Miocene and that the ~24.6 Ma unconformity in the Jianghan Basin represents the best dating of the TG formation.  相似文献   
163.
造山带隆起剥蚀过程与沉积记录   总被引:1,自引:0,他引:1       下载免费PDF全文
大别山造山带是中生代碰撞造山作用的产物,其隆起过程中形成了合肥盆地。本文对合肥盆地侏罗系碎屑岩进行了成分分析,发现砾岩中有两类榴辉岩,一类为高压变质榴辉岩,另一类为超高压变质榴辉岩。对砂岩中碎屑白云母的成分分析表明,指示高压变质作用的多硅白云母在较低层位已大量出现。重建的碎屑物注入顺序为:非超高压变质岩—高压变质岩—超高压变质岩。结合变质岩石学研究和地球物理观测资料重建的大别山造山带内部结构,可进一步重建大别山的剥蚀历史:大别山造山带最先(三尖铺组沉积初期)受到剥蚀的是非超高压变质的片岩、片麻岩及大理岩,高压变质岩折返到地表受到剥蚀不晚于中侏罗世初期(三尖铺组沉积早期),而超高压变质岩折返到地表经受剥蚀的时间稍早于中侏罗世中期(凤凰台组沉积初期)。天山是典型的陆内造山带,其隆起是新生代以来印度板块与欧亚板块碰撞的一种远程效应。本文对天山发育的花岗岩磷灰石裂变径迹分析,并对南侧的塔里木盆地北部古近系及新近系沉积岩进行了碎屑岩物源分析,在新的磁性地层学格架中讨论了天山的隆起剥蚀历史。砾石组分的突然变化发生在75~35 Ma,26~17 Ma和12~8 Ma间,从中天山物源区逐渐变为南天山物源区,12 Ma后变为以南天山为主要物源区。砂岩及重矿物组分变化表明,物源在124 Ma、26(~24)Ma及15(~12)Ma时发生过变化。磷灰石裂变径迹则进一步揭示了天山的3阶段差异性隆起历史:天山的早期隆起发生在124~80 Ma间,从中天山和南天山的交界处开始并向南扩展;第二次隆起发生在大约100~60 Ma间,从中天山开始向南扩展;第三次隆起从大约50 Ma开始,并向北南两侧扩展,至大约30 Ma时扩展到北天山,约20 Ma时扩展至南天山;其后,南天山在15(~12)Ma时发生了独立的隆起事件。本文的两个研究实例表明,盆地的充填符合计算机数据结构的堆栈过程,但造山带的隆起剥蚀却会出现明显的差异性。不能简单地说造山带的剥蚀和盆地的充填具镜像对称关系,这有可能导致错误的认识,一定要具体事例具体分析。  相似文献   
164.
怒江河砂岩屑磷灰石裂变径迹结果与流域地貌演化   总被引:2,自引:0,他引:2  
河流搬运沉积的河砂作为流域内地质体的平均产物,可以有效地揭示整个流域内区域性的地质体热史演化。对同一河流进行分段采样能够揭示更为详实的热史演化差异。本文对滇西境内怒江上游至下游采集了7个河砂样品进行磷灰石裂变径迹定年,主要年龄峰值依次为: 12.2 Ma和12.8 Ma, 7.7 Ma, 5.3 Ma、4.4 Ma和4.9 Ma, 7.3 Ma,总体上呈现出上游老、中游年轻、下游老的年龄格局。怒江中游河段相对年轻的流域热史经历说明中游河段较其他区域经受了构造地貌的快速演化。由于这一位置对应三江并流,而且气候作用与现代西南季风的水汽通道吻合,降雨量与上、下游流域截然不同。可以推断,气候因素导致了其快而新的构造地貌演化,促成代表年轻冷却历史信息的地质体被迅速剥露造就了怒江河道不同位置流域热史演化的差异。测得的7个样品所有年龄峰值可分为5个区段: 5.3~4.4 Ma、7.7~7.3 Ma、12.8~10.7 Ma、26.8~22.2.3 Ma、48.7~30.1 Ma,基本反映了流域范围新生代以来主要的热史演化阶段。此外,怒江不同河段河砂样品的分段性特征,证实河砂岩屑磷灰石裂变径迹分析方法在解释流域区域热史演化方面具有独特的优点。  相似文献   
165.
166.
167.
The 642 Ma-old Brauna Kimberlite Field is located on the northeastern sector of the São Francisco Craton (Serrinha block) and is one of the rare Neoproterozoic kimberlitic events in South America. Zircon xenocrysts from the volumetric most important kimberlite pipes Brauna 03, Brauna 07 and Brauna 04 were used as a tool to identify different components of the lithosphere beneath the northeast region of the São Francisco craton. A composite kimberlite sample of eight representative and different drill holes and three samples of the host rocks (Nordestina granodiorite) were sampled for SHRIMP geochronology. The results were compared with precise U–Pb age data for the regional rocks, i.e. the Archaean basement and the Palaeoproterozoic Rio Itapicuru greenstone belt. Samples from the Nordestina granodiorite gave three different ages: 2155 Ma in the western part of the batholith, 2139 Ma in its central part, and 2132 Ma in its eastern part. Zircon 207Pb/206Pb ages of the Brauna kimberlite zircon grains spread over the timespan 2107–2223 Ma and indicate four age groups at 2105 ± 3 Ma, 2138 ± 7 Ma, 2166 ± 5 Ma, and 2198 ± 4 Ma. Source rocks for the three former age groups can be found in the Rio Itapicuru greenstone belt, including zircon xenocrysts from the Nordestina granodiorite, whereas the latter age group has not yet been reported in the Serrinha block. The new zircon ages show that only rocks of the Palaeoproterozoic Rio Itapicuru greenstone belt and of a hidden 2.17–2.20 Ga crust were sampled by the kimberlite magma during its ascent through the lithosphere. It is proposed that there is none or a few Archaean crust beneath the kimberlite emplacement area, hence implying a thick Palaeoproterozoic lithosphere for this portion of the São Francisco craton.  相似文献   
168.
华北克拉通南缘新太古代-古元古代变质结晶基底之上不整合覆盖着巨厚的中-新元古代陆源碎屑岩-碳酸盐岩沉积盖层,根据沉积建造特征,将其划分为三个不同的地层分布小区,分别为嵩箕地层小区、渑池-确山地层小区和熊耳山地层小区.嵩箕小区位于熊耳裂谷盆地东北缘,以硅质碎屑岩(砂岩)为主,渑池-确山地层小区位于熊耳裂谷盆地北缘,以硅质碎屑岩-碳酸盐岩(白云岩)过渡相为主,熊耳山地层小区位于熊耳裂谷盆地南缘,以碳酸盐岩为主.本文通过对三个地层小区的沉积地层剖面和岩石学特征进行研究,认为华北南缘从中元古代开始处于河流相-浅海相的沉积环境,从南向北,海水由深变浅.根据地层的岩性、沉积构造及其组合特征,将其划分为低水位、海侵和高水位沉积体系,最大海侵时期为青白口系早期.通过对熊耳山地区的官道口群的岩相学和地球化学分析,并结合其已有的碎屑锆石年龄和另外两个地层小区的五佛山群和汝阳群的碎屑锆石年龄以及它们的地球化学特征,表明三个地层区的沉积地层在中元古代均处于被动大陆边缘环境,而新元古代则可能处于与大陆岛弧相关的沉积盆地,这一结果表明从中元古代到新元古代华北南缘可能受到秦岭造山带早期微陆块俯冲碰撞的影响,由被动大陆边缘向活动大陆边缘过渡的过程.三套地层最年轻的碎屑锆石207 Pb/206Pb年龄基本上在1600Ma左右,从而限定了其最大沉积时代不早于1600Ma.其锆石年龄大多数都分布于古元古代(1700 ~ 2400Ma),太古代的年龄极少,说明其物源区以古元古代的地质体为主,且碎屑锆石年龄峰值为~ 1.93Ga,反映了华北南缘在~1.93Ga发生过重要的构造-热事件,与华北克拉通古元古代中期发生的变质作用时间(~ 1.91Ga)一致.三套沉积地层的碎屑锆石εHf(t)值变化较大(-20~ +6),表明既有新生地壳物质的加入,也有古老地壳物质的再循环.Hf两阶段模式年龄分布于2.3~3.8Ga之间,明显大于其207pb/206pb年龄,大部分锆石的Hf同位素组成集中于2.6Ga和3.0Ga地壳演化线区域内,峰值为2.75Ga,表明2.75Ga左右是华北克拉通南缘重要的陆壳生长期.  相似文献   
169.
ABSTRACT

Placer mineral exploration has been undertaken along the beach of Central Tamil Nadu coast from Pondicherry to Vedaranyam. On the basis of the drainage network, geomorphology, and the coastal environment, the study area has been grouped into three sectors, North, Central, and South. Heavy mineral by Wt% shows a slightly higher abundance in the Northern sector, an enrichment of opaques in the Central sector from stations between Poompuhar and Karaikal, and a total depletion in the Southern sector. An abundance of heavies in the Northern sector is considered to be the result of a higher wave energy, and the cymatogenic downwarping of the basin during the present transgression. An enrichment of heavies in the Central sector from Poompuhar to Karaikal is attributable to the reworking of the beach ridges, which were submerged during the present transgression, and to the role of density sorting. A depletion of heavies in the Southern sector is accounted for by the absence of a terrigenous supply and the prevalence of wave shadow conditions throughout the year. The nature of the heavy mineral assemblage reflects the derivation of sediments principally from khondalites, granites, metamorphic rocks and paleo-sediments. Factor analysis also supplements the predominant role of a density factor in the segregation of heavy minerals in the study area. A five-stage model is proposed for the formation of placer deposits in the study region. The present study has disclosed rich concentrations of ilmenites in the central sector between Poompuhar and Karaikal that can be commercially exploited.  相似文献   
170.
The provenance of loess in Chinese Loess Plateau, including origin, transport pathways and source areas, has long been one of the most important questions. In this study, the vertical variations of the luminescence sensitivity of quartz grains from the central Chinese Loess Plateau were investigated by using optically stimulated luminescence (OSL) techniques. Our results indicate that the luminescence sensitivity of quartz grains of paleosols can be much higher than that of loess beds. In addition, the quartz grains from the loess-paleosol sequence exhibit a temporal trend in the strength of luminescence sensitivity, characterized by higher values in soils and lower values in loess beds. The OSL sensitivity of quartz grains of the loess-paleosol sequence also shows very similar trend to the magnetic susceptibility and particle size fluctuations, implying that the luminescence sensitivity might be climatic dependent. The possible factors affecting the variations of luminescence sensitivity were discussed including particle size, natural radioactivity, and the provenance of eolian deposits. We suggest that the temporal variations of luminescence sensitivity can be attributed to the retreat-advance of deserts, the different contributions of glacial origin quartz particles associated with mountain processes, and wind patterns during glacial/interglacial cycles. Therefore, the secular variations of luminescence sensitivity of quartz grains are ultimately influenced by past climatic change through its controlling on sediment provenance changes.  相似文献   
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