川西双江口地区花岗岩的岩石学、地球化学特征及其成因研究

双江口地区出露的花岗岩主要为二云二长花岗岩和似斑状黑云花岗岩,二者呈侵入接触关系,在岩体特征、岩石颜色、结构、矿物组成及后期改造等方面存在较为明显的差异。岩相学特征表明二云二长花岗岩形成晚于似斑状花岗岩,岩石地球化学特征表明二者成因为部分熔融,物源为壳源,形成环境为同碰撞-造山带环境,形成时间为印支晚期。     

Petrogenesis of the Paleoproterozoic Guandishan Granitoids in Shanxi Province： Constraints from Geochemistry and Nd Isotopes

The Guandishan granitoids consist mainly of various granitoid intrusions with different scales, including the Huijiazhuang intrusion, Shizhuang intrusion and Hengjian intrusion, which were formed between 1906 Ma and 1848 Ma. On the basis of geological and petrological characteristics, these granitoids can be classified into two groups： the earlier gneissic granodiorites and monzogranites, and the later massive leuco-monzogranites. Their geochemical and Nd isotopic features indicate that they could be derived from complicated partial melting of supracrustal rocks with an affinity of continental arc materials, such as sandy shale and pelite, and with garnet, pyroxene, hornblende and plagioclase as residual phases. Biotite, feldspar and other minerals were most likely fractionated during the magma evolution. Their source may have an affinity with continental arcs, and the granitoids could be derived from the main syn-collisional to late-orogenic tectonic environment, which may be related to the final amalgamation between the Eastern and Western continental blocks in the North China Craton.     

微量元素模拟限定大别造山带中生代花岗岩类的源岩成分

摘 要　 大陆碰撞造山带中花岗岩浆主要是因下部地壳缺乏流体熔融过程而形成的。对其源 岩成分限制而进行的微量元素模拟不仅要考虑源岩和熔体中有关矿物相比例的变化‚还要考 虑熔融过程中源岩矿物相组合的变化‚并选择合适的元素用于模拟。Rb、Sr、Ba 和 REE 模拟 结果显示‚上溪群杂砂岩作为扬子隆起带中生代花岗岩类的源岩是不合适的：大别隆起带中 的中生代花岗岩类也不可能完全由大别杂岩中的 TTG 质片麻岩熔融形成‚更可能是变基性岩 和 TTG 质片麻岩构成的复合源岩熔融的结果。     

内蒙古阿巴嘎旗中元古代片麻状花岗岩锆石U-Pb年龄、地球化学特征及大地构造意义

在内蒙古阿巴嘎旗南部新发现一处面积约为9.2km2的片麻状正长花岗岩体,采用LA-MC-ICP-MS锆石U-Pb测年法获得该岩体的同位素年龄为1377±10Ma～1385±14Ma,属中元古代。它是继苏尼特左旗南部锡林浩特微地块的中元古代花岗岩发现后又一处中元古代片麻状正长花岗岩体。片麻状正长花岗岩具条纹状-弱片麻状构造,矿物组成为石英(25%～30%)、微斜长石(30%～40%)、条纹长石(15%～20%)、斜长石5%～10%以及少量黑云母(约5%)。其地球化学成分显示高SiO_2(76.05%～78.16%)、高碱(K_2O+Na_2O=6.69%～8.04%)和较高的K_2O/Na_2O比值(1.01～2.48),低TiO_2(0.17%～0.23%)、A1_2O_3(10.99%～11.97%)、MgO(0.08%～0.44%)和CaO(0.15%～0.37%),铝饱和指数A/CNK值均大于1.1,里特曼指数主体小于1.8,属于过铝质和钙质系列;并且它们具有稀土元素总量高,轻稀土富集而重稀土亏损的特征,显示强烈负铕异常(δEu=0.44～0.53)和高的10000Ga/Al比值(均值为4.43)。上述岩相学、地球化学组成均显示A型花岗岩的特点,暗示其形成于伸展环境。片麻状正长花岗岩锆石ε_(Hf)(t)值主体介于+0.5～+4.6,两阶段模式年龄t2DM为1.88～2.10Ga,表明岩浆可能来源于古元古代新增生地壳的部分熔融。阿巴嘎旗与苏尼特左旗中元古代岩体的发现为锡林浩特微地块的存在提供了直接证据。区域对比显示中亚造山带中的阿拉善微地块、中天山微地块、库鲁克塔格微地块和锡林浩特微地块上均具有～1.4Ga岩浆事件产物,可能是全球哥伦比亚超大陆裂解事件(1.5～1.3Ga)的岩浆响应。     

伊犁地块南缘古生代花岗岩类的地质特征及构造意义

伊犁地块南缘元古宙特克斯群变质岩中侵入有花岗岩类,其形成时代和构造背景一直没有详细的研究。文章通过野外观察和室内分析,确定花岗质侵入体主要由弱面理化黑云母花岗岩、强面理化二云母花岗岩和未变形黑云母花岗岩组成。全岩地球化学和锆石U-Pb年代学分析显示,弱面理化黑云母花岗岩和强面理化二云母花岗岩属于过铝质钙碱性系列,其年龄分别为438 Ma和426 Ma;未变形黑云母花岗岩则属于典型的钙碱性系列,富集大离子亲石元素,相对亏损高场强元素,其年龄介于400~380 Ma之间。结合前人对区域地质的研究认识,笔者认为这些花岗岩类记录了两期不同构造背景的岩浆作用,指示研究区经历了两阶段构造—岩浆演化,即早古生代过铝质钙碱性弱面理化黑云母花岗岩与强面理化二云母花岗岩形成于哈萨克斯坦微大陆汇聚拼贴过程的后碰撞造山环境;中—晚古生代钙碱性未变形黑云母花岗岩则形成于准噶尔洋俯冲作用的活动大陆边缘。     

Neoarchean and Rhyacian TTG-Sanukitoid suites in the southern São Francisco Paleocontinent,Brazil: Evidence for diachronous change towards modern tectonics

The southern portion of the Sao Francisco Palaeocontinent in Brazil is denoted by Archean nuclei and Paleoproterozoic magmatic arcs that were amalgamated during Siderian to Orosirian orogenic processes(ca.2.4-2.1 Ga).New isotopic U-Pb in zircon and Sm-Nd whole rock combined with major and trace element composition analyses constrain the crystallization history of the Neoarchean Piedade block(at ca.2.6 Ga) and the Paleoproterozoic Mantiqueira Complex(ca.2.1-1.9 Ga).These therefore display quite different magmatic histories prior to their amalgamation at ca.2.05 Ga.Sm-Nd and Rb-Sr isotopes imply a mixed mantle-crustal origin for the samples in both units.A complete Palaeoproterozoic orogenic cycle,from subduction to collision and collapse,is recorded in the Piedade Block and the Mantiqueira Complex.Rhyacian to Orosirian subduction processes(ca.2.2-2.1 Ga) led to the generation of coeval(ca.2.16 Ga)TTG suites and sanukitoids,followed by late(2.10-2.02 Ga) high-K granitoids that mark the collisional stage.The collisional accretion of the Mantiqueira Complex against the Piedade Block at 2.08-2.04 Ga is also recorded by granulite facies metamorphism in the latter terrane,along the Ponte Nova suture zone.The collisional stage was closely followed by the emplacement of within-plate tholeiites at ca.2.04 Ga and by alkaline rocks(syenites and enriched basic rocks) at ca.1.98 Ga,marking the transition to an extensional tectonic regime.The discovery of two episodes of TTG and sanukitoid magmatism,one during the Neoarchean in the Piedade Complex and another during the Rhyacian in the Mantiqueira Complex,indicates that the onset of subduction-related melting of metasomatized mantle was not restricted to Neoarchean times,as generally believed,but persisted much later into the Paleoproterozoic.     

云南安宁地区石虎山花岗岩年代学、地球化学特征和锆石Hf同位素组成及其成因

石虎山花岗岩岩体位于安宁市德滋村附近,本文对该岩体开展了LA-ICP-MS锆石U-Pb定年、岩石地球化学、锆石Hf同位素组成研究。结果获得(616±20) Ma的岩浆结晶年龄和(839±17) Ma、(766±15) Ma、(705.5±9.4) Ma的继承性年龄,说明岩体形成于新元古代埃迪卡拉纪;其中(839±17) Ma、(766±15) Ma、(705.5±9.4) Ma的继承性年龄组合可能是Rodinia超大陆裂解构造过程的记录,839 Ma、616 Ma可能是Rodinia超大陆在扬子板块西缘开始裂解与最终裂解时限。花岗岩主量、微量元素特征显示,其产生于伸展环境的高硅、过铝、高钾的A型花岗岩;锆石ε_(Hf)(t)值均小于0,在t-t(Ma)和t-(~(176)Hf/~(177)Hf)图上,所有样品点均落在上地壳演化线之上,二阶段模式年龄变化范围为1.77～2.31 Ga,结合Nb/Y—Rb/Y图解,表明成岩物质主要来源于古元古代古老下地壳页岩60%部分熔融。     

鲁西蒙山山脉中段早前寒武纪花岗质岩石岩石学和单锆石年龄

用Ｋｏｂｅｒ方法测定了平邑县、蒙阴县普照寺闪长岩、松山－邱子峪二长花岗岩、周公地－花果庄－宁子洞花岗闪长岩、余粮店辉长岩和东近台英云闪长岩的锆石年龄。多数样品中的锆石反映了多于一期的地质记录，其中东近台英云闪长岩中的锆石（２８６８±１３Ｍａ、２７１２±５Ｍａ、２７１１±７Ｍａ和２５９８±６Ｍａ误差均为２σ），反映了本区最老的地质记录；部分样品中的２４００Ｍａ可能反映了太古宙最后一期的地质作用；而大部分样品中的锆石显示了２５００Ｍａ和２６００Ｍａ的地质记录，即岩浆活动多集中于２６００Ｍａ、２５００Ｍａ和２４     

辽西兴城地区早侏罗世花岗质岩浆活动——华北克拉通东部古太平洋俯冲作用的响应

华北克拉通东部中生代期间受到古太平洋板块俯冲并引发一系列的构造-岩浆-成矿作用,但古太平洋俯冲作用开始的具体时限仍未有定论.本文对辽西兴城地区中生代药王庙～磨盘山岩体进行了系统的岩相学研究、锆石U-Pb同位素定年、全岩地球化学和锆石原位Hf同位素测试分析,结果显示,花岗质岩石中岩浆成因锆石加权平均年龄为193～186 ...     

Petrogenesis of A-type granites and origin of vertical zoning in the Katharina pluton, Gebel Mussa (Mt. Moses) area, Sinai, Egypt

The central pluton within the Neoproterozoic Katharina Ring Complex (area of Gebel Mussa, traditionally believed to be the biblical Mt. Sinai) shows a vertical compositional zoning: syenogranite makes up the bulk of the pluton and grades upwards to alkali-feldspar granites. The latters form two horizontal subzones, an albite–alkali feldspar (Ab–Afs) granite and an uppermost perthite granite. These two varieties are chemically indistinguishable. Syenogranite, as compared with alkali-feldspar granites, is richer in Ca, Sr, K, Ba and contains less SiO₂, Rb, Y, Nb and U; Eu/Eu* values are 0.22–0.33 for syenogranite and 0.08–0.02 for alkali-feldspar granites. The δ¹⁸O (Qtz) is rather homogeneous throughout the pluton, 8.03–8.55‰. The δ¹⁸O (Afs) values in the syenogranite are appreciably lower relative to those in the alkali–feldspar granites: 7.59–8.75‰ vs. 8.31–9.12‰. A Rb–Sr isochron (n = 9) yields an age of 593 ± 16 Ma for the Katharina Ring Complex (granite pluton and ring dikes).

The alkali–feldspar granites were generated mainly by fractional crystallization of syenogranite magma. The model for residual melt extraction and accumulation is based on the estimated extent of crystallization ( 50 wt.%), which approximates the rigid percolation threshold for silicic melts. The fluid-rich residual melt could be separated efficiently by its upward flow through the rigid clusters of crystal phase. Crystallization of the evolved melt started with formation of hypersolvus granite immediately under the roof. Fluid influx from the inner part of the pluton to its apical zone persisted and caused increase of P_H2O in the magma below the perthite granite zone. Owing to the presence of F and Ca in the melt, P_H2O of only slightly more than 1 kbar allows crystallization of subsolvus Ab–Afs granite. Abundance of turbid alkali feldspars and their ¹⁸O/¹⁶O enrichment suggest that crystallization of alkali-feldspar granites was followed by subsolvus fluid–rock interaction; the δ¹⁸O (Fsp) values point to magmatic origin of fluids.

The stable and radiogenic isotope data [δ¹⁸O (Zrn) = 5.82 ± 0.06‰, I_Sr = 0.7022 ± 0.0064, ε_Nd (T) values are + 3.6 and + 3.9] indicate that the granite magma was generated from a ‘juvenile’ source, which is typical of the rocks making up most of the Arabian–Nubian shield.