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81.
徐文博  张铭杰  包亚文  满毅  李思奥  王鹏 《地质学报》2022,96(12):4257-4274
塔里木克拉通东北缘坡北、磁海等地二叠纪幔源岩浆活动形成了镍钴硫化物矿床和铁钴氧化物矿床,两者赋矿镁铁 超镁铁岩体的年龄相近(290~260 Ma),主、微量元素和Sr Nd Hf同位素组成相似,分配系数接近的微量元素比值分布于相同趋势线,揭示两者岩浆源区相同,可能为俯冲板片流体交代的亏损地幔或软流圈地幔。两类矿床镁铁 超镁铁质岩中Co与Ni含量正相关,Co主要富集在基性程度高的岩石中;块状硫化物与磁铁矿矿石中Co与Ni相关性差,Co和Ni具有不同的富集机制,Co热液富集作用明显。北山镁铁 超镁铁杂岩体是地幔柱相关软流圈上涌,诱发俯冲板片交代的亏损岩石圈地幔发生部分熔融,形成的高镁母岩浆演化过程中经历壳源混染、硫化物饱和富集镍钴形成铜镍钴硫化物矿床,富铁母岩浆氧逸度高、富水,岩浆分离结晶磁铁矿、叠加热液作用富集钴,形成铁钴氧化物矿床。  相似文献   
82.
ABSTRACT

Eocene intermediate to felsic plutons of different sizes and compositions are widespread in the Eastern Pontides Orogenic Belt in northern Turkey. Of these, the Ta?l?k Tepe pluton in the Havza (Samsun) area is fine-to-medium-grained, with granular, porphyritic, and micrographic textures, and include mafic microgranular enclaves (MMEs). LA-ICP-MS U-Pb zircon dating yielded emplacement ages of 42.9 (± 1.4) and 40.5 (± 1.3) Ma for the host granodioritic pluton and the dioritic MMEs, respectively. Petrochemically, the host pluton has I-type, high-K calc-alkaline, and metaluminous-to-slightly peraluminous features (A/CNK = 0.95–1.06). The host pluton also shows geochemical features of adakite-like rocks with high SiO2 (67–68 wt%) and Al2O3 (15.5–16.0 wt%) content and Ba/La (17–23), Sr/Y (40.7–61.6), and LaN/YbN (14.4–23.7) ratios and low Y (8.2–9.9 ppm) and YbN (3.1–4.4) contents. Whole-rock major and trace element variations suggest that fractional crystallisation played a significant role in the pluton evolution. The N-MORB normalised trace element patterns of the pluton are similar to those of MMEs with enrichment in large-ion lithophile elements, Th and Ce, and negative Nb and Ti anomalies. Chondrite-normalised rare earth element plots show moderate-to-highly enriched concave patterns (LaN/LuN = 14.2–21.6) with insignificant negative Eu anomalies (EuN/Eu* = 0.86–1.14), all of which imply hornblende fractionation during magmatic evolution. The pluton samples have 87Sr/86Sr ratios of 0.704767 to 0.704927, 143Nd/144Nd ratios of 0.512767–0.512774, εNd values of (+2.52) – (+2.65), and δ18O values of 7.9–9.7‰. The isotopic compositions of the host pluton and MMEs are similar to I-type granitoids derived from mantle sources. The MMEs show incomplete magma mixing/mingling, representing small bodies of mafic parental magma. Combined with regional studies, these new data suggest that the parental magma of the studied adakite-like pluton was generated from the lithospheric mantle and then modified by fractional crystallisation and assimilation in a post-collisional setting.  相似文献   
83.
Abstract  Abundant mafic microgranular enclaves (MMEs) extensively distribute in granitoids in the Gangdisê giant magmatic belt, within which the Qüxü batholith is the most typical MME‐bearing pluton. Systematic sampling for granodioritic host rock, mafic microgranular enclaves and gabbro nearby at two locations in the Qüxü batholith, and subsequent zircon SHRIMP II U‐Pb dating have been conducted. Two sets of isotopic ages for granodioritic host rock, mafic microgranular enclaves and gabbro are 50.4±1.3 Ma, 51.2±1.1 Ma, 47.0±1 Ma and 49.3±1.7 Ma, 48.9±1.1 Ma, 49.9±1.7 Ma, respectively. It thus rules out the possibilities of mafic microgranular enclaves being refractory residues after partial melting of magma source region, or being xenoliths of country rocks or later intrusions. Therefore, it is believed that the three types of rocks mentioned above likely formed in the same magmatic event, i.e., they formed by magma mixing in the Eocene (c. 50 Ma). Compositionally, granitoid host rocks incline towards acidic end member involved in magma mixing, gabbros are akin to basic end member and mafic microgranular enclaves are the incompletely mixed basic magma clots trapped in acidic magma. The isotopic dating also suggested that huge‐scale magma mixing in the Gangdisê belt took place 15–20 million years after the initiation of the India‐Asia continental collision, genetically related to the underplating of subduction‐collision‐induced basic magma at the base of the continental crust. Underplating and magma mixing were likely the main process of mass‐energy exchange between the mantle and the crust during the continental collision, and greatly contributed to the accretion of the continental crust, the evolution of the lithosphere and related mineralization beneath the portion of the Tibetan Plateau to the north of the collision zone.  相似文献   
84.
85.
The structural organization of a giant mafic dyke swarm, the Okavango complex, in the northern Karoo Large Igneous Province (LIP) of NE Botswana is detailed. This N110°E-oriented dyke swarm extends for 1500 km with a maximum width of 100 km through Archaean basement terranes and Permo-Jurassic sedimentary sequences. The cornerstone of the study is the quantitative analysis of N>170 (exposed) and N>420 (detected by ground magnetics) dykes evidenced on a ca. 80-km-long section lying in crystalline host-rocks, at high-angle to the densest zone of the swarm (Shashe area). Individual dykes are generally sub-vertical and parallel to the entire swarm. Statistical analysis of width data indicates anomalous dyke frequency (few data <5.0 m) and mean dyke thickness (high value of 17 m) with respect to values classically obtained from other giant swarms. Variations of mean dyke thicknesses from 17 (N110°E swarm) to 27 m (adjoining and coeval N70°E giant swarm) are assigned to the conditions hosting fracture networks dilated as either shear or pure extensional structures, respectively, in response to an inferred NNW–SSE extension. Both fracture patterns are regarded as inherited brittle basement fabrics associated with a previous (Proterozoic) dyking event. The Okavango N110°E dyke swarm is thus a polyphase intrusive system in which total dilation caused by Karoo dykes (estimated frequency of 87%) is 12.2% (6315 m of cumulative dyke width) throughout the 52-km-long projected Shashe section. Assuming that Karoo mafic dyke swarms in NE Botswana follow inherited Proterozoic fractures, as similarly applied for most of the nearly synchronous giant dyke complexes converging towards the Nuanetsi area, leads us to consider that the resulting triple junction-like dyke/fracture pattern is not a definitive proof for a deep mantle plume in the Karoo LIP.  相似文献   
86.
CCSD主孔100~2950m榴辉岩、退变榴辉岩类岩石叶理倾角明显较片麻岩类岩石叶理倾角陡,前者总体倾角55°左右,后者28°左右,局部可见片麻岩类叶理切割榴辉岩类叶理,因此两者叶理可能形成于不同时期;两类岩石之间现部分为韧性剪切带接触关系,韧性剪切带形成于苏鲁地体折返主期自SEE向NWW的韧性剪切作用。榴辉岩、退变榴辉岩类岩石叶理产状对发育于该类岩石内的微断层产状有一定控制作用,而片麻岩类岩石叶理产状对发育于该类岩石内的微断层产状控制作用相对较弱。孔区脆性变形主要反映白垩纪以来SEE-NWW向伸展构造应力场的变形特征,主孔100~1620m倾伏向以SEE向占绝对优势的微正滑断层擦痕即为该期变形的产物。  相似文献   
87.
对于变质岩 Sm-Nd 和 Rh-Sr 同位素年代学来说,其中一个重要问题是等时线矿物之间在一特定的变质事件过程中是否达到并在随后保持同位素平衡。矿物 O 同位素地质测温也是如此。由于许多情况下 Nd、Sr 和 O 在变质矿物中的扩散速率具有可比性,变质矿物之间 O 同位素平衡状况能够为矿物 Sm-Nd 和 Rb-Sr 内部等时线定年结果的有效性提供制约。为了验证其适用性,本文对大别造山带双河超高压榴辉岩和片麻岩 Sm-Nd 和 Rh-Sr 等时线矿物进行了 O 同位素地质测温。尽管Sm-Nd 等时线给出一致的三叠纪年龄(213~238Ma),同一样品 Rb-Sr 等时线却给出侏罗纪年龄(171~174Ma)。片麻岩、榴辉岩和榴闪岩矿物对 O 同位素测温得到600~720℃和420~550℃两组温度,分别对应于约225±5Ma 榴辉岩相变质和约 175±5Ma 角闪岩相退变质条件下停止同位素扩散交换的温度。同一样品三叠纪 Sm-Nd 等时线年龄的保存、侏罗纪 Rh-Sr 等时线年龄的出现以及有规律的 O 同位素温度,表明在角闪岩相退变质过程中,Sr 和 O 在含水矿物(如黑云母和角闪石)中的扩散速率在手标本尺度上比石榴石 Nd 和多硅白云母 Sr 的扩散速率快。在退变质作用过程中,等时线矿物之间的初始同位素比值均一化速率主要受扩散速率慢的矿物控制,而矿物等时线时钟的启动主要受具有高母/子体比值的矿物控制。只有当高母/子体比值矿物具有快的放射成因同位素扩散速率时,才能够应用合理的矿物等时线确定变质再造的时间。  相似文献   
88.
Mafic to intermediate enclaves are evenly distributed throughoutthe dacitic 1991–1995 lava sequence of Unzen volcano,Japan, representing hundreds of mafic recharge events over thelife of the volcano. This study documents the morphological,textural, chemical, and petrological characteristics of theenclaves and coexisting silicic host lavas. The eruptive productsdescribed in this study appear to be general products of magmamingling, as the same textural types are seen at many othervolcanoes. Two types of magmatic enclaves, referred to as Porphyriticand Equigranular, are easily distinguished texturally. Porphyriticenclaves display a wide range in composition from basalt toandesite, are glass-rich, spherical and porphyritic, and containlarge, resorbed, plagioclase phenocrysts in a matrix of acicularcrystals and glass. Equigranular enclaves are andesitic, non-porphyritic,and consist of tabular, medium-grained microphenocrysts in amatrix glass that is in equilibrium with the host dacite magma.Porphyritic enclaves are produced when intruding basaltic magmaengulfs melt and phenocrysts of resident silicic magma at theirmutual interface. Equigranular enclaves are a product of a moreprolonged mixing and gradual crystallization at a slower coolingrate within the interior of the mafic intrusion. KEY WORDS: mafic enclaves; quenched mafic inclusions; magma mingling; Unzen volcano; Unzen Scientific Drilling Project; resorbed plagioclase  相似文献   
89.
东昆仑约格鲁岩体暗色微粒包体特征及成因   总被引:26,自引:10,他引:26  
刘成东  张文秦等 《地质通报》2002,21(11):739-744
对东昆仑约格鲁花岗岩体中暗色微粒包体的形态、大小、成分和分布等主要特征进行了较详细地研究。发现包体形态多样,以强烈的塑性流变为特征;包体大小悬殊,多数直径为几十厘米,最大者长轴达4m;包体成分以闪长质为主,结构总体上比寄主岩石的粒度细,岩体中不同部位的包体成分和结构都有所变化;包体分布不均匀,经常呈族状、条带状密集分布,具定向性。镜下研究发现,在包体中经常见到针状磷灰石、石英捕虏晶和斜长石的自形内核环带及增生边等现象,显示了岩浆混合成因的特点。  相似文献   
90.
柳沟峡花岗质片麻岩是在鱼儿红幅1∶5万区调过程中从北大河岩群变质杂体中解体出的古花岗质侵入体。通过对其进行单矿物锆石U-Pb法年龄测定,获得了(1463±74)Ma和(623±138)Ma两组年龄值。结合区调成果认为(1463±74)Ma代表古花岗质侵入体上侵就位时代,(623±138)Ma代表后期叠加的变形变质热事件时代。两组年龄的获得为北祁连山早期大陆裂解及碰撞造山作用的确定提供了直接证据。  相似文献   
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