川西甲基卡地区侏倭组沉积物源分析—来自碎屑锆石U- Pb年龄证据

松潘- 甘孜造山带是青藏高原东北部的重要组成单元,是华北板块、扬子板块和羌塘块体的主要汇聚地区,主要由中生代浅变质沉积地层和一系列岩浆岩组成,记录了印支期以来块体之间的收敛汇聚等构造活动。其中,雅江残余盆地发育一套厚度巨大的中生代碎屑岩和岩浆岩地层组合,是研究松潘- 甘孜造山带地质构造演化的理想地区之一。本文对川西甲基卡地区侏倭组的样品进行了碎屑锆石LA- ICP- MS U- Pb年龄测试,碎屑锆石U- Pb年龄存在四个峰值,分别为231~281Ma、424~502Ma、707~983Ma、1539~1850Ma,表明扬子克拉通西缘及松潘甘孜造山带南部至少经历了四期强烈的构造—岩浆热事件,这四期事件在三叠系沉积地层中有非常清楚的记录。231~281Ma的锆石来自东昆仑,这一年龄段的锆石最可能来自北部晚二叠世松潘洋向北俯冲于华北板块之下所形成的东昆仑岛弧花岗岩。424~502Ma的锆石来自北秦岭,代表了加里东期南秦岭与北秦岭和华北板块的拼合事件。722~983Ma的锆石来自扬子板块,这一年龄段的锆石最可能来自盆地东部新元古界拉伸系上扬子克拉通盆地向北西俯冲于华北板块之下所形成的南秦岭花岗岩,形成于扬子板块晋宁期陆壳增生事件。1539~1850Ma与华北板块基底年龄特征值正相对应,是吕梁期华北克拉通东西两大块体在中部发生碰撞,华北古陆进一步固结、扩大的时间,这其中包含了继承东西块体的太古宙物质和新生的火成岩和沉积岩,在中- 晚三叠世,随着秦岭洋的关闭和碰撞造山,将大量碎屑物质经华北板块南缘东西向的疏导体系注入松潘甘孜盆地。说明松潘甘孜三叠纪复理石盆地侏倭组主要接受来自东昆仑、华北板块和秦岭造山带的物质。最年轻碎屑锆石可以限定沉积岩的最大沉积年龄,侏倭组4颗年轻碎屑锆石加权平均计算得出241. 8±4. 5Ma（n=4）,推测侏倭组沉积年龄介于231. 6~249. 9Ma之间。     

额尔古纳地块新元古代花岗岩榍石原位微区LA- ICP- MS U- Pb定年及其地质意义

本文首次报道了额尔古纳地块新元古代花岗岩榍石原位微区LA-ICP-MS U-Pb定年数据,以明确其形成时代,进而为准确厘定额尔古纳地块新元古代岩浆作用期次提供新的证据,并进一步揭示其地质意义。研究区内分别采自满归岩体和莫尔道嘎岩体的2个代表性样品中的榍石呈菱形自形—半自形晶,不具有变质榍石特有的杏仁孔或孔洞特征,暗示其为岩浆成因。对原生榍石的定年结果显示,满归岩体和莫尔道嘎岩体数据点的线性拟合性均较好,拟合线下交点年龄分别为873±22 Ma和783±31 Ma,均与~(206)Pb/~(238)U加权平均年龄(872±18Ma和789±17 Ma)相一致。同时结合已有研究成果表明,原定为额尔古纳地块新元古代最早期岩浆作用产物的满归岩体实际形成于～850 Ma,而非前人认为的957～927 Ma;莫尔道嘎岩体形成于～790 Ma,也并非前人认为的～762 Ma。综合校正后的岩体年龄以及近年来前人研究成果,现阶段额尔古纳地块新元古代岩浆作用期次可大致分为五个阶段,即915～905 Ma、～847 Ma、818～808 Ma、～792 Ma和～738 Ma。     

海南岛琼中地区琼中岩体锆石U-Pb年龄及其地质意义

琼中地区琼中岩体为钙碱性的铝弱过饱和型花岗岩,具有壳源物质来源,岩石普遍发育定向组构,生成于同碰撞期—晚造山期。其锆石U-Pb年龄为226. 5±2. 9~234. 2±2. 3Ma,为晚三叠世。通过区域分析,认为海南岛海西—印支期花岗岩从西往东,具有由老至新的演化规律,形成了略向南面突出的弧状面理构造。表明同期造山活动消减方向由西至东,呈现出剪刀式闭合的特征。     

Trace element and isotopic (Sr, Nd, Pb, O) arguments for a mid-crustal origin of Pan-African garnet-bearing S-type granites from the Damara orogen (Namibia)

Geochronological data, major and trace element abundances, Nd and Sr isotope ratios, δ¹⁸O whole rock values and Pb isotope ratios from leached feldspars are presented for garnet-bearing granites (locality at Oetmoed and outcrop 10 km north of Omaruru) from the Damara Belt (Namibia). For the granites from outcrop 10 km N′ Omaruru, reversely discordant U–Pb monazite data give ²⁰⁷Pb/²³⁵U ages of 511±2 Ma and 517±2 Ma, similar to previously published estimates for the time of regional high grade metamorphism in the Central Zone. Based on textural and compositional variations, garnets from these granites are inferred to be refractory residues from partial melting in the deep crust. Because P–T estimates from these xenocrystic garnets are significantly higher (800°C/9–10 kbar) than regional estimates (700°C/5 kbar), the monazite ages are interpreted to date the peak of regional metamorphism in the source of the granites. Sm–Nd garnet–whole rock ages are between 500 and 490 Ma indicating the age of extraction of the granites from their deep crustal sources. For the granites from Oetmoed, both Sm–Nd and Pb–Pb ages obtained on igneous garnets range from 500 to 490 Ma. These ages are interpreted as emplacement ages and are significantly younger than the previously proposed age of 520 Ma for these granites based on Rb/Sr whole rock age determinations. Major and trace element compositions indicate that the granites are moderately to strongly peraluminous S-type granites. High initial ⁸⁷Sr/⁸⁶Sr ratios (>0.716), high δ¹⁸O values of >13.8‰, negative initial _Nd values between −4 and −7 and evolved Pb isotope ratios indicate formation of the granites by anatexis of mid-crustal rocks similar to the exposed metapelites into which they intruded. The large range of Pb isotope ratios and the lack of correlation between Pb isotope ratios and Nd and Sr isotope ratios indicate heterogeneity of the involved crustal rocks. Evidence for the involvement of isotopically highly evolved lower crust is scarce and the influence of a depleted mantle component is unlikely. The crustal heating events that produced these granites might have been caused by crustal thickening and thrusting of crustal sheets enriched in heat-producing elements. Very limited fluxing of volatiles from underthrust low- to medium-grade metasedimentary rocks may have also been a factor in promoting partial melting. Furthermore, delamination of the lithospheric mantle and uprise of hot mantle could have caused localized high-T regions. The presence of coeval A-type granites at Oetmoed that have been derived at least in part from a mantle source supports this model.     

Origin of Meso-Proterozoic post-collisional leucogranite suites (Kaokoveld, Namibia): constraints from geochronology and Nd, Sr, Hf, and Pb isotopes

Leucocratic granites of the Proterozoic Kaoko Belt, northern Namibia, now preserved as meta-granites, define a rock suite that is distinct from the surrounding granitoids based on their chemical and isotopic characteristics. Least evolved members of this ~1.5–1.6-Ga-old leucogranite suite can be distinguished from ordinary calc-alkaline granites that occur elsewhere in the Kaoko Belt by higher abundances of Zr, Y, and REE, more radiogenic initial ε_Nd values and unradiogenic initial ⁸⁷Sr/⁸⁶Sr. The leucogranites have high calculated zircon saturation temperatures (mostly > 920°C for least fractionated samples), suggesting that they represent high-temperature melts originating from deep crustal levels. Isotope data (i.e., ε_Ndi: +2.3 to –4.2) demonstrate that the granites formed from different sources and differentiated by a variety of processes including partial melting of mantle-derived meta-igneous rocks followed by crystal fractionation and interaction with older crustal material. Most fractionation-corrected Nd model ages (T_DM) are between 1.7 and 1.8 Ga and only slightly older than the inferred intrusion age of ca. 1.6 Ga, indicating that the precursor rocks must have been dominated by juvenile material. Epsilon Hf values of zircon separated from two granite samples are positive (+11 and +13), and Hf model ages (1.5 and 1.6 Ga) are similar to the U–Pb zircon ages, again supporting the dominance of juvenile material. In contrast, the Hf model ages of the respective whole rock samples are 2.3 and 2.4 Ga, demonstrating the involvement of older material in the generation of the granites. The last major tectonothermal event in the Kaoko Belt in the Proterozoic occurred at ca. 2.0 Ga and led to reworking of mostly 2.6-Ga-old rocks. However, the presence of 1.6 Ga “post-collisional” granites reflects addition of some juvenile mantle-derived material after the last major tectonic event. The results suggest that similar A-type leucogranites are potentially more abundant in crustal terranes but are masked by AFC processes. In the case of the Kaoko Belt, it is suggested that this rock suite indicates a yet unidentified period of mantle-derived crustal growth in the Proterozoic of South Western Africa.     

Geochronological,geochemical and Pb isotopic compositions of Tasmanian granites (southeast Australia): Controls on petrogenesis,geodynamic evolution and tin mineralisation

Large volumes of Devonian-Carboniferous granites were emplaced across Tasmania in southeast Australia, which was along the easternmost boundary of mid-Palaeozoic Gondwana. Some of these granites are associated with world class Sn–W deposits. Previous studies have focused mainly on relationships between granite petrogenesis and source rocks, and rarely on geochemical controls on Sn mineralisation. New zircon U-Pb ages of 405 to 396 Ma reveal that the George River Granodiorite, Grant Point Granite and Mt. Pearson Granite from eastern Tasmania intruded prior to the Tabberabberan Orogeny. The Coles Bay Granite has a U-Pb age of 388 ± 7 Ma, implying that it was emplaced simultaneously with the Tabberabberan Orogeny in Tasmania. The western Tasmanian granites mostly intruded from 374 to 360 Ma, after the Tabberabberan Orogeny. Granites associated with Sn–W deposits are moderately to strongly fractionated, including the Housetop, Meredith, Pine Hill and Heemskirk granites. Lead isotopic compositions of K-feldspars from the analysed granites, combined with isotopic evidence from other studies, suggest that differentiated granites in Tasmania had been highly contaminated by a crustal (sedimentary) component, and that western Tasmanian granites had a crustal source with substantially different isotopic characteristics to that of eastern Tasmania, which has a character similar to the Lachlan Orogen in southeast Australia. Tin-mineralised granites in Tasmania formed in a post-collisional extensional margin, a favourable environment for the production of Sn-rich melts from the lower crust. Prolonged fractional crystallisation, low oxygen fugacity and enrichments of volatiles are crucial factors to promote Sn enrichment in magmatic-hydrothermal fluids exsolved from crystallised felsic magmas.     

山西青尖坡石英二长岩锆石U-Pb年龄及其地质意义

通过对华北克拉通北缘青尖坡石英二长岩锆石U-Pb同位素年龄分析,并结合相关主量和稀土元素数据探讨其地质意义。研究表明,石英二长岩LA-ICP-MS锆石U-Pb同位素年龄为241.1±1.7Ma,为早中三叠世岩浆活动的产物。岩石具有富K、Na、Si、Al,贫Mg、Ca、Ti等特征,为高钾碱性钾玄岩系列,属于过铝质花岗岩类;轻稀土元素相对富集,重稀土元素相对亏损,具有稳定的弱负Eu异常。总体为I型花岗岩成因,但兼具S型花岗岩的特征。青尖坡石英二长岩为中下地壳部分熔融成因,有地幔物质参与,为华北克拉通北缘三叠纪碱性岩带的组成部分,形成于晚造山-造山后的伸展构造环境。     

黑龙江晨明地区桦皮沟岩体和达里岱岩体LA-ICP-MS锆石U-Pb年龄及其意义

前人认为,黑龙江省晨明地区的桦皮沟岩体(花岗质糜棱岩)和达里岱岩体(糜棱岩化黑云母花岗岩)分别由形成于元古宙和海西期的花岗岩组成。LA-ICP-MS锆石U-Pb测年对2个岩体的定年结果显示,桦皮沟岩体中的花岗质糜棱岩和达里岱岩体中的糜棱岩化黑云母花岗岩的206Pb/238U年龄加权平均值分别为453.5±6.0Ma和454.8±2.6Ma,表明二者均形成于早古生代,应是伊春—延寿构造带早古生代花岗岩带的组成部分,而非形成于元古宙和晚古生代。     

Controls on Devonian–Carboniferous magmatism in Tasmania,based on inherited zircon age patterns,Sr, Nd and Pb isotopes,and major and trace element geochemistry

Devonian–Carboniferous granites are widespread in Tasmania. In eastern Tasmania, Devonian granites intrude Ordovician–Early Devonian quartz-rich turbidites of the Mathinna Supergroup. The earliest (～400 Ma) I-type granodiorites may be arc-related. Following the Tabberabberan Orogeny (～389 Ma), more felsic and, finally, strongly fractionated I- and S-type granites were emplaced until ～373 Ma. In contrast, western Tasmania granites intrude a more diverse terrane of predominantly marine shelf successions, with depositional ages as old as Late Mesoproterozoic. They are mostly felsic and fractionated I- and S-types emplaced from ～374–351 Ma, possibly in response to post-collisional crustal extension following juxtaposition of the eastern and western Tasmanian terranes. Granites from the two terranes are readily distinguishable by the age spectra of their inherited zircon, which are noticeably similar to those of the detrital zircon from sedimentary successions in their respective terranes. Furthermore, within each terrane, both I and S-types yield similar inheritance patterns. This suggests a pivotal role for the sedimentary successions in the petrogenesis of both types. Western Tasmanian granites are also enriched in ～1600 Ma zircon, which is essentially unrepresented in the exposed supracrustal succession. Subtle differences between the inheritance and detrital age spectra in eastern Tasmania probably relate to unrepresentative sampling of the supracrustal rocks. Nd, Sr and Pb isotopic characteristics of the granites are consistent with their derivation by mixing of magmas derived from the mantle, possibly the lower crust, and from supracrustal rocks. Systematic isotopic trends in some eastern Tasmanian I-types, particularly in the Scottsdale Batholith, correlate well with major and trace element geochemistry and age. The isotopes are inconsistent with simple restite unmixing or crystal fractionation in a closed magma chamber, and indicate progressive contamination by the Mathinna Supergroup, or similar rocks. The isotopic characteristics of late, strongly fractionated granites, although sometimes obscured by hydrothermal alteration, are also consistent with concurrent assimilation-fractional crystallisation processes. Together with the close association of some strongly fractionated I- and S-types, this suggests that such granites were generated directly in the lower crust, and were not derived from unfractionated parental granite magmas.     

Early Proterozoic 87Rb-86Sr Model Ages of Pegmatitic Muscovite from Rare Metal-bearing Granite-Pegamtite System of Kawadgaon, Bastar Craton, Central India

Seven muscovite mica separates from the rare metal pegmatites of Kawadgaon, Bastar Craton, Central India, give model 87Rb-86Sr ages ranging from 2330 to 1850 Ma. The oldest age of the muscovite almost overlaps within 20 error with the age (2497k152 Ma) of the parent fertile granites. The data suggest possible derivation of pegmatites shortly after the emplacement of Kawadgaon granites at ca. 2500 Ma. Most of the muscovite ages (n = 6) indicate tectonomagmatic ages after pegmatite injections. The 87Sr/86Sr ratio (0.7142) of granites suggests their derivation from crustal material.     

Isotope geochronology,geochemistry, and mineral chemistry of the U-bearing and barren granites from the Zhuguangshan complex,South China: Implications for petrogenesis and uranium mineralization

The Zhuguangshan complex carries some of the most important granite-hosted uranium deposits in South China. Here we investigate the Changjiang and Jiufeng granites which represent typical U-bearing and barren granites in the complex, using zircon U-Pb ages, whole-rock geochemistry, Sr-Nd isotopic and zircon Hf isotopic data, and mineral chemistry, to constrain the petrogenesis and uranium mineralization. LA-ICP-MS zircon U-Pb dating shows that both the Changjiang and Jiufeng granites were emplaced ca. 160 Ma. These rocks show high silica, weakly to strongly peraluminous compositions, enrichment in Rb, Th, and U, and depletion in Ba, Nb, Sr, P, and Ti. These features coupled with the high initial ⁸⁷Sr/⁸⁶Sr ratios, negative εNd(t) values and εHf(t) values, and the Paleoproterozoic two stage model ages of these two granites suggest that the two granites belong to S-type granites, and the parental magmas of the two granites were derived from the Paleoproterozoic metasedimentary rocks. However, the granitoids show different mineralogical characteristics. The biotite in the Changjiang granite belongs to siderophyllite, marking higher degree of chloritization, whereas the biotite in the Jiufeng granite is ferribiotite, characterized by only slight chloritization. Compared with the Jiufeng granite, the biotite in the Changjiang granite has lower crystallization temperature and oxygen fugacity, but higher F content, and the uraninite has higher UO₂ content but lower ThO₂ content, and stronger corrosion. The chemical ages of uraninites from both granites are (within error) consistent with the zircon U-Pb ages and are considered to represent the emplacement ages of granites. Chemical ages of pitchblende in the Changjiang granite yield 118 ± 8 Ma, 87 ± 4 Ma, and 68 ± 6 Ma, representing multiple episodes of hydrothermal events that are responsible for the precipitation of U ores in the Changjiang uranium ore field. Our study suggests that the degree of magma differentiation and physicochemical conditions of the magmatic-hydrothermal system are the key factors that control the different U contents of these two granites. The mineralogical characteristics of uraninite and biotite can be used to distinguish between U-bearing and barren granites, and serve as a potential tool for prospecting granite-hosted uranium deposits.     

黑龙江省漠河县富源沟林场含电气石 花岗岩的形成时代及地质意义

本文对额尔古纳地块北段的富源沟林场含电气石花岗岩体进行了LA-ICP-MS锆石U-Pb同位素定年和岩石地球化学研究。含电气石花岗岩的锆石²⁰⁶Pb/²³⁸U年龄加权平均值为458±4 Ma（MSWD = 1.8）,表明含电气石花岗岩形成于晚奥陶世初期。岩石地球化学特征表明该花岗岩应为高钾钙碱性系列（K₂O = 3.45%～4.83%）,铝饱和指数A/CNK＞1.1（1.11～1.28）,属强过铝质的S型花岗岩,富集Th、U、Rb、K等元素,相对亏损Sr、Ba、 Nb、Ti、 P、Eu等元素,是同碰撞构造背景下地壳部分熔融的产物。结合前人研究资料和本文数据提出,富源沟林场含电气石花岗岩的形成与额尔古纳地块和兴安地块的碰撞拼贴有关,形成于额尔古纳地块与兴安地块碰撞拼贴作用所引发的碰撞构造背景,由于地缘因素,构造岩浆作用滞后于额尔古纳地块东缘的碰撞拼贴时限,是额尔古纳地块和兴安地块碰撞拼贴的远程效应。     

十杭带湘南—桂北段中生代A型花岗岩带成岩成矿特征及成因讨论

十杭带是华南内陆一条重要的北北东向、具有高εNd (t )值和低t DM值的花岗岩带,该带在湘南—桂北段的花岗质岩体（千里山、骑田岭、西山、金鸡岭、花山和姑婆山等）均形成于151~163 Ma间。但从西南往东北方向,形成时代有逐渐变年轻的趋势。这些岩体在地球化学组成上显示出较为相似的特征,岩石均富碱、高钾,富含Rb,Th,U等大离子亲石元素（LILE）和REE,Nb,Ta,Zr,Hf等高场强元素（HFSE）。在地球化学图解上均落入A型花岗岩区域,因此该花岗岩带应属于一条A型花岗岩带。进一步划分,这些花岗岩应该属于A2亚类。这些花岗岩均具有较低的（87Sr/86Sr）i 值、较高的εNd (t )值和相对低的Nd模式年龄值,但从西南往东北方向,εNd (t )值具有逐渐降低的趋势。在这些花岗质岩体中暗色包体非常发育,岩石学和地球化学,特别是锆石的Hf同位素组成,指示这些花岗质岩石是通过壳-幔岩浆混合作用形成的,幔源岩浆端元来自亏损地幔,可能是软流圈地幔物质的直接参与。该A型花岗岩带可能形成于古太平洋板块俯冲引起的弧后或弧内拉张构造环境,软流圈地幔上涌及诱发的幔源岩浆沿超壳深断裂底侵,导致了强烈的壳幔岩浆混合作用,形成了该花岗岩带。该拉张事件从西南往东北方向进行,拉张强度由强变弱,混入花岗岩中的地幔物质也由多变少。该花岗岩带也是我国 一条重要的W-Sn多金属成矿带。研究表明,这些花岗岩均属于富Sn花岗岩,但Sn在这些花岗岩中的富集机制与传统的结晶分异富集的方式不同。该区锡矿化类型十分丰富,除了存在传统的岩浆热液演化成矿外,还存在新类型的绿泥石化花岗岩锡矿化,丰富了A型花岗岩的成矿理论。     

湘东-赣西地区早古生代晚期花岗岩体的LA-ICPMS锆石U-Pb定年研究

对湘东板杉铺岩体、宏夏桥岩体和赣西张佳坊岩体、丰顶山岩体以及山庄岩体共5个早古生代晚期花岗岩体的LA—ICPMS锆石U—Pb年龄测定结果表明,采自上述5个岩体的代表性样品分别给出了（418±2）Ma（板杉铺岩体）、（432±6）Ma（宏夏桥岩体）、（440±2）Ma（张佳坊岩体）、（402±2）Ma（丰顶山岩体）和（424±3）Ma（山庄岩体）的锆石u—Ph谐和年龄,代表了区内早古生代晚期花岗岩的形成时代。结合其他的年代学和地质资料,认为华南早古生代晚期花岗岩空间上呈面状展布,时代上主体集中在400～440Ma间,且区内早古生代晚期片麻状花岗岩和块状花岗岩的形成时代无明显差异,动力学上倾向于认为华南内部加里东事件很可能不是洋陆俯冲作用的结果。     

东昆仑祁漫塔格花岗片麻岩记录的岩浆和变质事件

东昆仑青海祁漫塔格尕林格一带原定为金水口群的眼球状花岗片麻岩,实际为新元古代早期形成的花岗岩.采用SHRIMP和LA-MC-ICP-MS两种方法对其中的锆石进行了测试,获得的年龄分别为938±5Ma和938±2Ma,代表了花岗岩的形成时代.花岗岩地球化学特征显示为S-型,属于钙碱性系列的弱过铝-过铝质花岗岩,εNd(0)为-9.4～-11.7,εNd(t=938Ma)为-0.6～-3.2,显示低的负值,tDM为1.6 ～2.1Ga,推测其源岩与白沙河岩组类似.东昆仑东段、柴北缘以及阿尔金均有1000～900Ma的花岗岩形成,表明这次岩浆活动比较广泛,可能与我国西部不同陆块间的汇聚有关,是我国西部新元古代克拉通基底形成的反映,同时也响应于全球Rodinia超大陆的形成.花岗片麻岩中1粒锆石边部获得了416±11Ma的年龄,与区域上志留-泥盆纪花岗岩形成时代一致,代表了新元古代花岗岩发生变质作用的时代,其中白云母40Ar/39Ar的坪年龄和等时线年龄为406±2Ma,代表了变质花岗岩的冷却年龄,这些年龄表明新元古代花岗岩卷入了古生代中期与祁漫塔格洋/海盆关闭有关的造山事件.     

东昆仑东段都兰热水花岗岩锆石U- Pb年龄、地球化学及构造意义

都兰热水地区位于东昆仑造山带东段,发育着大量花岗岩岩石组合,主要岩石类型为二长花岗岩和花岗闪长岩,本文报道了对都兰热水地区二长花岗岩和花岗闪长岩的地球化学、LA-ICP-MS锆石U-Pb定年的研究结果,为建立完善的年代学格架和构造演化提供了新资料。锆石U-Pb同位素定年研究表明东昆仑东段都兰热水地区的二长花岗岩和花岗闪长岩的结晶侵位时代分别是232.4±1.3 Ma、230.8±1.1 Ma,属中三叠世花岗岩浆作用的产物。岩矿特征和岩石地球化学特征显示二长花岗岩和花岗闪长岩属高钾钙碱性I型花岗岩,具较高的K_2O含量(2.2%～4.74%);铝饱和指数A/CNK值都小于1.1,显示准铝质特征;P_2O_5与SiO_2之间存在明显的负相关性,还表现出富集轻稀土元素、大离子亲石元素(如K、Rb、La),亏损重稀土元素和高场强元素(如Nb、Ta、Ti、P)及Eu负异常特征。结合前人区域地质研究,我们认为东昆仑东段都兰热水地区花岗岩岩石组合是受幔源岩浆的底侵作用导致下地壳部分熔融而形成,幔源岩浆与壳源岩浆发生不同比例混合,并在岩浆演化过程中发生了一定的分离结晶作用。晚二叠世阿尼玛卿洋向东昆仑板块俯冲,直至中三叠世都兰热水地区仍处于洋壳俯冲而产生的火山弧环境,二长花岗岩和花岗闪长岩就是这一阶段的典型产物。     

大别山地壳结构的Pb同位素地球化学示踪

研究了大别山东部北大别变质杂岩，南大别变质杂岩和白垩纪花岗岩的全岩Pb同位素组成，结果表明，北大别变质杂岩与南大别变质杂岩相比，前者以相对低放射成因Pb同位素组成为特征，按照Pb同位素组成在地壳垂向剖面上的变化模型，指出在大别山地壳垂向结构上，北大别变质杂岩应位于南大别变质杂岩之下，这一认识得到大别山不同构造岩石单元中产出的白垩纪花岗岩Pb同位素对岩浆源区示踪的有力支持，因此南大别超高压变质带是发育在北大别杂岩之上的一个构造岩片，这对进一步确定扬子克拉通向华北克拉通俯冲－碰撞的缝合线位置具有重要意义。     

西准噶尔谢米斯台西段花岗岩年代学、地球化学、锆石Lu-Hf同位素特征及大地构造意义

西准噶尔谢米斯台花岗岩研究程度偏低, 运用锆石LA-ICP-MS U-Pb年代学、地球化学及锆石Lu-Hf同位素方法研究西准谢米斯台西段地区花岗岩, 结果表明: 谢米斯台岩体(427.6±2.3 Ma)和哈勒盖特希岩体(428.6±2.5 Ma)均形成于中志留世; 谢米斯台碱长花岗岩地球化学特征类似于Ⅰ型花岗岩, 哈勒盖特希碱长花岗岩地球化学特征类似于A型花岗岩; 锆石Hf同位素组成较均一, ε_Hf(t)=12.4~14.5, 二阶段模式年龄t_DM2变化范围在497~603 Ma之间, Ⅰ型花岗岩和A₂型花岗岩可能形成于后碰撞阶段的挤压-伸展转变期, 是中志留世额尔齐斯-斋桑洋壳向南俯冲至波谢库尔-成吉斯火山弧底部, 俯冲板片与岛弧底部岩石圈之间剪切带的物质发生变形、变质及部分熔融作用, 使得由亏损地幔形成不久的年轻地壳(由洋壳和岛弧组成)发生部分熔融形成的长英质岩浆经进一步分离结晶作用形成分异Ⅰ型花岗岩和高温、缺水A₂型花岗岩, A₂型花岗岩较Ⅰ型花岗岩分离结晶程度高.      

新疆库米什地区晚石炭世-早二叠世花岗岩年代学、地球化学及其地质意义

南天山东缘库米什地区花岗岩广泛出露,沿库米什断裂形成NWW向花岗岩带.该地区发现有忠宝和桑树园子矽卡岩型白钨矿床,矿化与二云母花岗岩关系密切.锆石U-Pb LA-ICP-MS定年分别获得忠宝岩体年龄为296±4 Ma,桑树园子岩体年龄为293±3 Ma,形成时代为晚石炭世-早二叠世.两岩体总体具有高SiO₂(72.51%~74.84%,70.68%~74.14%),K₂O＞Na₂O,铝饱和(A/CNK=1.11~1.48,1.05~1.11),可见原生白云母矿物等特征,反映了同碰撞S型花岗岩的特点.样品总体富集LILE元素、亏损HFSE元素,稀土元素表现为轻稀土富集、重稀土亏损的“右倾”型特征,具中等的负Eu异常.综合岩体的I_Sr值(0.707 6~0.708 8和0.706 5~0.707 7)、负的ε_Nd(t)值(-6.3~-7.1和-4.7~-5.1)、岩体单阶段模式年龄(T_DM)值(1.59~1.8 Ga和1.50~1.56 Ga)及古老的继承锆石年龄(2.5~0.8 Ga)分析认为,忠宝及桑树园子岩体为库米什地区星星峡群变泥质岩云母类矿物脱水部分熔融的产物,并可能混有杂砂岩成分,而南天山东部存在古老基底.本次研究显示南天山洋东部(库米什地区)于晚石炭世-早二叠世最终闭合,早中二叠世A型花岗岩及基性岩浆活动的出现表明该地区进入板内伸展阶段.富钨的星星峡群是本地区钨矿化可能的矿源层,早二叠世挤压向伸展的转换阶段为南天山东部钨矿有利的成矿构造体制,经历多旋回构造重熔的星星峡群在早二叠世造山过程的再次“重熔”作用致使成矿元素最终富集成矿.      

Cassiterite LA-MC-ICP-MS U/Pb and muscovite 40Ar/39Ar dating of tin deposits in the Tengchong-Lianghe tin district,NW Yunnan,China

The Tengchong-Lianghe tin district in northwestern Yunnan, China, is an important tin mineralization area in the Sanjiang Tethyan Metallogenic Domain. There are three N–S trending granite belts in the Tengchong-Lianghe area, with emplacement ages ranging from Early Cretaceous to Late Cretaceous and Early Cenozoic. Tin mineralization is spatially associated with these granitic rocks. However, the petrogenetic link between the tin deposits and the host granites is not clear because of the lack of age data for the tin mineralization. We investigate the possibility of direct dating of cassiterite from three typical tin deposits in the Tengchong-Lianghe tin district, using laser ablation multicollector inductively coupled plasma mass spectrometry (LA-MC-ICP-MS). In situ LA-MC-ICP-MS dating of seven cassiterite samples from the Lailishan (LLS-1 and LLS-2), Xiaolonghe (XLH, WDS, DSP, and HJS), and Tieyaoshan (TYS) tin deposits yielded well-defined ²⁰⁶Pb/²⁰⁷Pb–²³⁸U/²⁰⁷Pb isochron ages. To assess the accuracy of the in situ U/Pb dating of cassiterite, ⁴⁰Ar/³⁹Ar dating of coexisting muscovite (in samples LLS-1, DSP, and TYS) was also performed. The cassiterite in situ U/Pb ages (47.4?±?2.0, 71.9?±?2.3, and 119.3?±?1.7 Ma, respectively) are in excellent agreement with the coexisting muscovite ⁴⁰Ar/³⁹Ar ages (48.4?±?0.3, 71.9?±?1.4, and 122.4?±?0.7 Ma, respectively). The U/Pb ages of cassiterite combined with the ⁴⁰Ar/³⁹Ar ages of muscovite indicate that there are three tin mineralization events in this district: the Lailishan tin deposit at 47.4?±?2.0 to 52?±?2.7 Ma, the Xiaolonghe tin deposit at 71.6?±?2.4 to 3.9?±?2.0 Ma, and the Tieyaoshan tin deposit at 119.3?±?1.7 to 122.5?±?0.7 Ma. These ages are highly consistent with the zircon U/Pb ages of the host granites. It is su.ggested that the Cretaceous tin mineralization might have taken place in a subduction environment, while the Early Tertiary tin metallogenesis was in a postcollisional geodynamic setting.