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1.
关键金属是全球高科技产业不可或缺的战略性资源,其富集机制和成矿作用是目前国际矿床学研究的热点之一。我们对喜马拉雅带吉隆和亚东地区淡色花岗岩开展系统的地球化学研究,发现侵入到藏南拆离系的淡色花岗岩含有较高的Sn、Cs、Tl、Be、W、B、Li和Bi。全岩元素地球化学分析表明,这些淡色花岗岩具有如下特征:(1)富集关键金属元素;(2)为原始岩浆经历斜长石、锆石、独居石、磷灰石、云母分离结晶作用后的残余熔体;(3)关键元素的富集和矿化与花岗岩高度分离结晶作用密切相关。随着分异程度的增强,岩浆变为富挥发分的高SiO2体系,关键金属元素在残余熔体中富集,并且最后可能形成具有工业价值的矿床。由于地球化学特征的相似性,Cs和Tl呈类质同象替代钾、铷进入云母中。富集关键金属元素的花岗岩在时间上和空间上属于与藏南拆离系相关的同构造侵位花岗岩,藏南拆离系的活动促使了原始岩浆的广泛分离结晶作用,以及后期的关键金属元素(如Rb、Cs和Tl)的富集。  相似文献   
2.
The North Qilian orogenic belt is a typical plate suture zone, which is studded with numerous different sizes of fragments of micro-continental crust consisting of pre-Sinian metamorphic rocks and the North Qilian orogenic belt provides important study carrier for studying the pre-orogenic tectonic process of the North Qilian. The relatively complete volcanic-clastic-carbonate rocks formation of Zhulongguan Group, Changchengian System, Mesoproterozoic are distributed in the Kawa-Qiqing area, Western North Qilian orogenic belt. Geochemical characteristics of the Aoyougou Group basalts in the North Qilian indicated that the contents of major element were relatively stable, high K2O contents(4.27%~6.07%), TFe2O3(10.49%~13.01%),TiO2(1.96%~2.90%)and middle MgO(5.37%~6.71%,Mg# 48~51), CaO(2.57%~5.51%)content. Thus, the Aoyougou Group basalts belong to potassium alkaline basalt. The contents of Cr and Ni of the basalts decreased with the decreasing of Mg#, and there was a positive correlation between CaO and CaO/Al2O3, Furthermore, the Eu anomaly of samples was slightly negative, high contents of high field strength elements (HFSE, Nb, Ta, Ti), and the ratios of Gd/Yb(2.5~3.0), Zr/Y(8.6~10.2), Ta/Yb(0.96~1.23), Ti/Yb(5 074~6 021), Zr/Yb(81~97), Ce/Nb(1.87), Zr/Nb(6.41)indicated that the Aoyougou Group basalts had obvious OIB-type magmatic affinity. In combination with the regional geological background, the study results showed that Aoyougou Group alkaline basalt generated from deep enrichment mantle similar to the source of OIB, with fractional crystallization of olivine and monoclinic pyroxene and a certain degree of contamination of continental crust in the process of magmatism, formed in the background of continental rift, might response to the Proterozoic Columbia supercontinent rifting, which further provides important petrological evidences for the relationship between North China Craton rifting events and Columbia supercontinent rifting during Proterozoic.  相似文献   
3.
为了开展无乳链球菌(Streptococcus agalactiae)核糖结合蛋白(Ribose binding protein B,RbsB)结构功能的研究,本实验根据已知无乳链球菌ZQ0910全基因组序列设计相关引物。采用PCR方法扩增其RbsB基因,随后将该基因定向克隆到原核表达载体pGEX-6p-1中,在大肠杆菌BL21(DE3)感受态细胞中进行IPTG诱导表达;采用HRV 3C蛋白酶切除GST标签,分子筛分离获得RbsB蛋白;运用生物信息学软件对RbsB基因序列进行分析,并对RbsB蛋白二级和三级结构进行预测;采用NeXtal Tubes JCSG Core Suite结晶试剂盒筛选蛋白结晶条件。研究结果表明,该基因全长为969碱基,编码322个氨基酸,RbsB蛋白理论分子量33.9ku,等电点为9.41,二级结构中α螺旋结构所占比重最高,建立RbsB蛋白三维结构模式图;经IPTG诱导后表达的融合蛋白分子量为59ku,筛选RbsB蛋白的初始结晶条件为(0.2mol/L di-Potassium hydrogen phosphate,20%(W/V)PEG3350;1.5mol/L ammonium sulfate,25%(V/V)Glycerol),获得RbsB蛋白结晶体。本研究结果可为无乳链球菌核糖结合蛋白(RbsB)的功能解析提供实验及理论基础。  相似文献   
4.
雄村铜(金)矿区位于西藏冈底斯成矿带中段南缘,由Ⅰ、Ⅱ、Ⅲ号矿体和多个矿化体组成。本文以Ⅰ、Ⅱ号矿体钾硅酸盐化蚀变带内的热液黑云母为研究对象,采用光薄片镜下鉴定、电子探针等分析方法,系统研究了热液黑云母的产状和成分特征。结果显示,雄村矿区Ⅰ号矿体黑云母类型主要为金云母和镁质黑云母;Ⅱ号矿体黑云母类型为镁质黑云母。两个矿体黑云母都具有低Ti(TiO_2 3%)、高Al(Al_2O_315%)的特点,且具有较高的MgO含量,Mg/Fe0.5,K/Na10,显示了与矿化良好的相关性。Ⅰ号矿体热液黑云母平均结晶温度470℃,氧逸度位于镍-氧化镍缓冲剂与磁铁矿-钛铁矿缓冲剂之间(NNO—HM);Ⅱ号矿体热液黑云母平均结晶温度234℃,氧逸度位于镍-氧化镍缓冲剂与铁橄榄石-石英-磁铁矿缓冲剂之间(NNO—FQM),说明Ⅰ号矿体形成于较高温、高氧逸度的热液系统,Ⅱ号矿体形成于相对较低温、低氧逸度的热液系统。此外,Ⅰ号矿体热液黑云母Ⅳ(F)值介于0.61~2.72之间,平均值1.26,Ⅳ(Cl)值介于-5.49~-4.53之间,平均值-5.03,Ⅳ(F/Cl)值介于5.63~7.89之间,平均值6.29;Ⅱ号矿体热液黑云母Ⅳ(F)值介于1.83~3.32之间,平均值2.66,Ⅳ(Cl)值介于-5.64~-4.89之间,平均值-5.31,Ⅳ(F/Cl)值介于7.14~8.68之间,平均值7.97,说明Ⅰ、Ⅱ号矿体都形成于富Cl的热液系统,且Ⅱ号矿体热液较Ⅰ号矿体更富Cl,贫F。富Cl流体易萃取流体中的Cu和Au等金属元素并以Cl的络合物形式运移,在沿构造裂隙向上运移的过程中,物理化学条件发生改变,使得流体中金属元素络合物溶解度降低,促使硫化物沉淀成矿。  相似文献   
5.
碳酸氢钠(NaHCO_3)俗称小苏打,其产品质量取决于颗粒的大小,晶体的形貌和样品的纯度等诸多因素。本论文基于连续稳态MSMPR结晶器原理,研究了不同停留时间下,碳酸氢钠从碳酸钠溶液中冷却结晶过程动力学。利用实验数据建立了NaHCO_3的结晶动力学操作模型。实验和计算结果表明,随停留时间的增加,NaHCO_3过饱和度降低,晶体生长速率和成核速率均减小,相应的平均粒径增加,细颗粒含量减小;适当延长停留时间是制取高品质小苏打产品的有效途径。冷却结晶过程可有效增加小苏打产量,小苏打收率维持在55%左右。此外,一定Na_2CO_3存在下冷却结晶碳酸氢钠晶体形态由细长的针状变为规整的片状。  相似文献   
6.
腾冲火山岩区是我国全新世以来记载火山喷发的少数地区之一,该地区岩浆作用的性质与成因是揭示青藏高原东缘的现今侧向生长过程与深部作用的重要依据。本文对腾冲火山岩区的马鞍山、黑空山、打鹰山全新世火山岩开展了矿物化学和岩石地球化学研究,以期揭示岩石成因和深部动力学过程。腾冲全新世火山岩主体岩性为高钾钙碱性系列的玄武粗安岩和粗安岩。岩石的Ca O、Fe_2O_3~T、Ti O_2与Si O_2负相关,而K_2O与Si O_2正相关,表明岩浆演化过程中可能存在橄榄石、辉石和斜长石的分离结晶作用。岩石中存在酸性斜长石(更长石,An=28)大颗粒捕掳晶,其边部发育了基性斜长石(拉长石,An=65)增生边;在大颗粒石英捕掳晶的边部发育了辉石的反应边,这些结构表明在岩浆上升到地壳浅部时,曾受到了花岗岩围岩的混染,但岩石的Th/Nb值均小于1.16,表明地壳混染总体不显著。腾冲全新世火山岩大离子亲石元素富集、高场强元素相对亏损,高Th/U、低Ba/La,富集Sr-Nd同位素,其岩浆源区应为经历过洋壳沉积物交代后的富集地幔。腾冲火山岩属于大陆板内环境,是印度与亚洲大陆碰撞后岩浆作用的产物。火山岩是沿着腾冲盆地南北向展布,且熔岩分布面积有限。由于高原侧向生长过程中的区域性走滑断裂会引起局部的伸展,腾冲火山岩产出可能与富集岩石圈地幔的减压熔融有关。  相似文献   
7.
喜马拉雅淡色花岗岩   总被引:62,自引:33,他引:29  
在青藏高原南部的喜马拉雅地区,分布有两条世界瞩目的淡色花岗岩带。南带主要沿高喜马拉雅和特提斯喜马拉雅之间的藏南拆离系(STDS)分布,俗称高喜马拉雅淡色花岗岩带,构成喜马拉雅山的主体。北带淡色花岗岩位于特提斯喜马拉雅单元内,又被称之为特提斯喜马拉雅淡色花岗岩带。这些花岗岩多以规模不等的岩席形式侵入到周边沉积-变质岩系之中,或者呈岩株状产出于变质穹窿的核部。岩体本身大多岩性均匀,变形程度不等,但岩体边缘可见较多的围岩捕虏体,并在部分情况下见及围岩的接触变质作用,反映它们的异地侵位特征。上述两带中的淡色花岗岩在矿物组成和岩石类型上表现为惊人的相似性,主要由不同比例的石英、钾长石、斜长石、黑云母(5%)、白云母、电气石和石榴石等构成二云母花岗岩、电气石花岗岩和石榴石花岗岩三大主要岩石类型。从不同地区的野外观察来看,二云母花岗岩为喜马拉雅淡色花岗岩的主体岩石类型,而电气石花岗岩和石榴石花岗岩主要以规模不等的脉体形式赋存于二云母花岗岩之中,反映前两者晚期侵位的特征。地球化学特征上,这些花岗岩具有高Si、Al、K,低Ca、Mg、Fe、Ti的特点,接近花岗岩的低共熔点组分。绝大多数淡色花岗岩具有较高的含铝指数,属于过铝花岗岩。微量元素表现为较大的变化范围,但总体上表现为富集大离子亲石元素K、Rb和放射性元素U,而不同程度亏损Ba、Th、Nb、Sr、Ti等元素。稀土元素总量总体上明显低于世界上酸性岩的平均丰度,且绝大部分表现为轻-中等程度的稀土元素分馏和不同程度的Eu负异常。传统认为,喜马拉雅淡色花岗岩是原地-近原地侵位的纯地壳来源的低熔花岗岩。但本文通过分析提出,该花岗岩可能是从一种高温的花岗岩浆演化而来,其岩浆源区的性质或成因类型目前还难以确定。该岩浆在上升侵位的过程中曾经历过大规模地壳物质的混染,并发生了高度分离结晶作用。因此,喜马拉雅淡色花岗岩首先是一种高分异型的花岗岩,是真正意义上的异地深成侵入体,而并不是原地或半原地的部分熔融体。这种以大规模地壳混染和结晶分异作用为特征的花岗岩系,在花岗岩的研究内容中还未被充分地讨论。以前根据相关信息认为这些岩石来自于沉积岩部分熔融的结论,只是较多地注意到了后期地壳混染和结晶分异作用的特征。即使这些岩石的原始岩浆将来被证明真的来源于沉积岩系的部分熔融,那以前的结论也只能说是"歪打正着"。根据形成年龄和地质-地球化学特征,本文将这些花岗岩划分为原喜马拉雅(44~26Ma)、新喜马拉雅(26~13Ma)和后喜马拉雅(13~7Ma)三大阶段。其中第一阶段对应印度-亚洲汇聚而导致的大陆碰撞造山作用,而后两个阶段同加厚的喜马拉雅-青藏高原碰撞造山带拆沉作用有关,对应青藏高原的全面隆升。根据这些淡色花岗岩的岩石与地球化学特征,我们还不能支持青藏高原存在广泛的中地壳流动的模型。相反,俯冲的高喜马拉雅岩系在深部的部分熔融及随该岩系折返而发生的分离结晶作用可很好地解释淡色花岗岩所具有的系列特征。  相似文献   
8.
The Naga Ophiolite Belt is a part of the Naga-Arakan-Yoma flysch trough that occurs along the Indo-Myanmar border. It is represented by peridotites, mafic-ultramafic cumulates, mafic volcanics, mafic dykes, plagiogranites, pelagic sediments and minor felsic to intermediate intrusives. Minor plagiogranites, gabbros and thin serpentinite bands occur juxtaposed near Luthur, with the slate-phyllite-metagreywacke sequence (Phokpur Formation) adjacent to the contact. The development of tonalites, trondhjemites and diorites in the oceanic crust, which is grouped as plagiogranites, offers an opportunity to study the process of formation of silicic melts from mafic crust. Plagiogranites from Naga Ophiolite Belt contains moderate SiO2 (51.81–56.71 wt.%), low K2O (0.08–1.65 wt.%) and high Na2O (4.3–5.03 wt.%). The Naga Ophiolite Belt plagiogranites like ocean-ridge granites contain low K2O, high Na2O and CaO. The rocks investigated from Naga Ophiolite Belt contain TiO2 concentrations above the lower limit for fractionated Mid Oceanic Ridge Basalt which is above 1 wt% of TiO2 and the ternary plots of A (Na2O + K2O) F(FeOT) M(MgO) and TiO2-K2O-SiO2/50 indicate that the plagiogranite are tholeiitic in character and gabbro samples are calc-alkaline in nature. The plagiogranites are enriched in Rb, Ba, Th, U, Nb and Sm against chondrite with negative anomalies on Sr and Zr whereas Y and Yb are depleted to Mid Oceanic Ridge Basalt. The chondrite normalized REE patterns of the plagiogranite display enrichments in LREE (LaN/SmN: 2.37–3.62) and flat HREE (Eu/Eu*: 0.90–1.06). The Mid Oceanic Ridge Basalt normalization of gabbro is characterized by strong enrichment of LILE like Ba and Th. The REE pattern is about 50–100 times chondrite with slight enrichment of LREE (LaN/SmN = 2.21–3.13) and flat HREE (Eu/Eu*: 0.94–1.19). The major-element and trace element data of the NOB plagiogranites and their intrusive nature with host gabbroic rock suggest that the plagiogranites were produced by fractional crystallization of basaltic parental magmas at Mid Oceanic Ridge.  相似文献   
9.
Lunar anorthosite is a major rock of the lunar highlands,which formed as a result of plagioclasefloatation in the lunar magma ocean(LMO).Constraints on the sufficient conditions that resulted in the formation of a thick pure anorthosite(mode of plagioclase 95 vol.%) is a key to reveal the early magmatic evolution of the terrestrial planets.To form the pure lunar anorthosite,plagioclase should have separated from the magma ocean with low crystal fraction.Crystal networks of plagioclase and mafic minerals develop when the crystal fraction in the magma(φ) is higher than ca.40-60 vol.%,which inhibit the formation of pure anorthosite.In contrast,when φ is small,the magma ocean is highly turbulent,and plagioclase is likely to become entrained in the turbulent magma rather than separated from the melt.To determine the necessary conditions in which anorthosite forms from the LMO,this study adopted the energy criterion formulated by Solomatov.The composition of melt,temperature,and pressure when plagioclase crystallizes are constrained by using MELTS/pMELTS to calculate the density and viscosity of the melt.When plagioclase starts to crystallize,the Mg~# of melt becomes 0.59 at 1291 C.The density of the melt is smaller than that of plagioclase for P 2.1 kbar(ca.50 km deep),and the critical diameter of plagioclase to separate from the melt becomes larger than the typical crystal diameter of plagioclase(1.8-3 cm).This suggests that plagioclase is likely entrained in the LMO just after the plagioclase starts to crystallize.When the Mg~# of melt becomes 0.54 at 1263 C,the density of melt becomes larger than that of plagioclase even for 0 kbar.When the Mg~# of melt decreases down to 0.46 at 1218 C,the critical diameter of plagioclase to separate from the melt becomes 1.5-2.5 cm,which is nearly equal to the typical plagioclase of the lunar anorthosite.This suggests that plagioclase could separate from the melt.One of the differences between the Earth and the Moon is the presence of water.If the terrestrial magma ocean was saturated with H_2O,plagioclase could not crystallize,and anorthosite could not form.  相似文献   
10.
The Khalkhab–Neshveh (KN) pluton is a part of Urumieh–Dokhtar Magmatic Arc and was intruded into a covering of basalt and andesite of Eocene to early Miocene age. It is a medium to high‐K, metaluminous and I‐type pluton ranging in composition from quartz monzogabbro, through quartz monzodiorite, granodiorite, and granite. The KN rocks show subtle differentiation trends strongly controlled by clinopyroxene, plagioclase, hornblende, apatite, and titanite, where most major elements (except K2O) are negatively correlated with SiO2; and Al2O3, Na2O, Sr, Eu, and Y define curvilinear trends. Considering three processes of magmatic differentiation including mixing and/or mingling between basaltic and dacitic magmas, gravitational fractional crystallization and in situ crystallization revealed that the latter is the most likely process for the evolution of KN magma. This is supported by the occurrence of all rock types at the same level, the lack of mafic enclaves in the granitoid rocks, the curvilinear trends of Na2O, Sr, and Eu, and the constant ratios of (87Sr/86Sr)i from quartz monzodiorite to granite (0.70475 and 0.70471, respectively). In situ crystallization took place via accumulation of plagioclase and clinopyroxene phenocrysts and concentration of these phases in the quartz monzogabbro and quartz monzodiorite at the margins of the intrusion at T ≥ 1050°C, and by filter pressing and fractionation of hornblende, plagioclase, and later biotite in the granitoids at T = ~880°C.  相似文献   
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