西藏冈底斯带始新世曲水岩基的岩浆混合作用:来自斜长石阴极发光特征和成分变化的证据

斜长石作为主要造岩矿物,是研究岩石成因、示踪岩浆演化和岩浆混合过程的有效工具.对冈底斯带曲水岩基始新世花岗闪长岩、二长花岗岩、闪长岩脉和暗色包体中的斜长石进行了阴极发光图像结构特征、电子探针主量元素和LA-ICP-MS微量元素成分的分析,揭示了斜长石复杂环带的成因和相关的岩浆过程.该区斜长石的阴极发光图像呈现出多种颜色且与其An值相对应,随着An值降低依次为绿色、蓝色和暗灰色或暗红色等,并发育补丁状环带、筛状环带、韵律环带等.花岗闪长岩、二长花岗岩中斜长石的An值具有相似的变化范围(20~55),而闪长岩脉和暗色包体中An值的变化范围较大(25~85),表明曲水岩基经历了复杂的开放过程.微量元素结果表明:花岗闪长岩与闪长岩脉和暗色微粒包体具有相同的Sr含量范围(600×10^-6~1 100×10^-6);而二长花岗岩的Sr含量(1 000×10^-6~2 400×10^-6)整体高于前者.以上研究表明,花岗闪长岩中阴极发光呈现绿色的核部或幔部是偏中性岩浆注入寄主岩岩浆混合的结果;具有高Sr含量的二长花岗岩认为是高Sr含量的岩浆结晶形成的;闪长岩脉和暗色微粒包体中的筛状结构斜长石为寄主岩捕掳晶.     

Mineralogy, whole-rock and Sr-Nd isotope geochemistry of mafic microgranular enclaves in Cretaceous Dagbasi granitoids, Eastern Pontides, NE Turkey: Evidence of magma mixing, mingling and chemical equilibration

Rocks of the Late Cretaceous Dagbasi Pluton (88-83 Ma), located in the eastern Pontides, include mafic microgranular enclaves (MMEs) ranging from a few centimetres to metres in size, and from ellipsoidal to ovoid in shape. The MMEs are composed of gabbroic diorite, diorite and tonalite, whereas the felsic host rocks comprise mainly tonalite, granodiorite and monzogranite based on both mineralogical and chemical compositions. MMEs are characterized by a fine-grained, equigranular and hypidiomorphic texture. The common texture of felsic host rocks is equigranular and also reveals some special types of microscopic textures, e.g., oscillatory-zoned plagioclase, poikilitic K-feldspar, small lath-shaped plagioclase in large plagioclase, blade-shaped biotite, acicular apatite, spike zones in plagioclase and spongy-cellular plagioclase textures and rounded plagioclase megacrysts in MMEs. Compositions of plagioclases (An₃₃-An₆₀), hornblendes (Mg#=0.77-1.0) and biotites (Mg#=0.61-0.63) of MMEs are slightly distinct or similar to those of host rocks (An_12-57; hbl Mg#=0.63-1.0; Bi Mg#=0.50-0.69), which suggest partial to complete equilibration during mafic-felsic magma interactions.The felsic host rocks have SiO₂ between 60 and 76 wt% and display low to slightly medium-K tholeiitic to calc-alkaline and peraluminous to slightly metaluminous characteristics. Chondrite-normalized rare-earth element (REE) patterns are fractionated (La_cn/Lu_cn=1.5-7.3) with pronounced negative Eu anomalies (Eu/Eu*=0.46-1.1). Initial ε_Nd(i) values vary between −3.1 and 1.6, initial ⁸⁷Sr/⁸⁶Sr values between 0.7056 and 0.7067.Compared with the host rocks, the MMEs are characterized by relatively high Mg-number of 22-52, low contents of SiO₂ (53-63 wt%), low ASI (0.7-1.1) and low to medium-K tholeiitic to calc-alkaline, metaluminous to peraluminous composition. Chondrite-normalized REE patterns are relatively flat [(La/Yb)_cn=1.4-3.9; (Tb/Yb)_cn=0.9-1.5] and show small negative Eu anomalies (Eu/Eu*=0.63-1.01). Isotope signatures of these rocks (⁸⁷Sr/⁸⁶Sr_(i)=0.7054-0.7055; ε_Nd(i)=-1.0 to 1.9) are largely similar to the host rocks. Gabbroic diorite enclaves have relatively low contents of SiO₂, ASI; high Mg#, CaO, Al₂O₃, TiO₂, P₂O₅, Sr and Nb concentrations compared to dioritic and tonalitic enclaves.The geochemical and isotopic similarities between the MMEs and their host rocks indicate that the enclaves are of mixed origin and are most probably formed by the interaction between the lower crust- and mantle-derived magmas. All the geochemical data suggest that a basic magma derived from an enriched subcontinental lithospheric mantle, interacted with a crustal melt that originated from dehydration melting of the mafic lower crust at deep crustal levels. The existence of compositional and textural disequilibrium and the nature of chemical and isotopic variation in these rock types indicate that magma mixing/mingling between an evolved mafic and a granitic magma was involved in their genesis. Microgranular enclaves are thus interpreted to be globules of a more mafic magma probably from an enriched lithospheric mantle source. Al-in-amphibole estimates the pluton emplacement at ca. 0.3-3.8 kbar, and therefore, magma mixing and mingling must have occurred at 3.8 kbar or below this level.     

内蒙古沙德盖花岗岩岩浆混合作用:岩相学、矿物化学和年代学证据

华北地台北缘乌拉山地区的沙德盖钾长花岗岩体中普遍发育以二长岩为主的暗色微粒包体,包体具塑性流变特征,与寄主岩的接触界线或为截然或为渐变过渡。岩相学观察表明,包体中发育多种反映岩浆混合作用的典型组构,如石英眼斑、环斑长石、镁铁质团块、钾长石巨晶的溶蚀、磷灰石的针柱状形貌、长石中的包体带以及钙长石的"针尖"结构等。造岩矿物的电子探针分析表明,岩浆混合在沙德盖岩体的形成中起了重要作用,寄主花岗岩浆主要来自下地壳,而暗色包体岩浆则主要为地幔来源。锆石LA-ICP-MS U-Pb同位素定年结果显示,沙德盖花岗岩及其暗色微粒包体的形成时代基本一致,分别为233.4±2.3Ma和229.7±1.5Ma(中三叠世),进一步佐证了该岩体是岩浆混合作用的产物。研究认为,当铁镁质岩浆与长英质岩浆混合时,早期基性岩浆的快速淬冷形成了边界清楚、具明显冷凝边且暗色矿物含量较高的包体;随着两种不同成分岩浆之间温差的减小以及组分的交换,进一步形成了颜色较浅、边界渐变过渡和无明显冷凝边的包体。     

岩浆混合作用与火成岩多样性的耦合关系:以东昆仑造山带白日其利长英质岩体为例

壳-幔岩浆相互作用如何影响长英质火成岩的岩石学多样性是当前岩石学研究的焦点问题之一.以岩石类型丰富的东昆仑白日其利长英质岩体和暗色微粒包体为研究对象,开展系统的锆石U-Pb年代学、矿物学、全岩元素地球化学和Sr-Nd-Hf同位素研究,探讨和解析这一重要科学问题.LA-ICPMS锆石U-Pb年代学研究表明,暗色微粒包体（247.8±2.0 Ma）与二长花岗岩（247.5±1.4 Ma）、花岗闪长岩（248.8±2.1 Ma）和石英闪长岩（248.8±1.5 Ma）均侵位结晶于早三叠世.岩相学和矿物学研究表明,白日其利长英质岩石与包体的成因机制与壳-幔岩浆的机械或化学混合作用密切相关.元素地球化学和Sr-Nd-Hf同位素组成研究揭示,幔源镁铁质岩浆端元起源于受俯冲板片流体交代的富集地幔熔融,而壳源长英质岩浆端元则起源于东昆仑古老的变质杂砂岩基底.岩石成因分析揭示,幔源镁铁质岩浆侵入长英质晶粥岩浆房,促使长英质晶粥发生活化,随后壳-幔岩浆端元以不同比例和不同方式发生机械和化学混合等相互作用,从而形成镁铁质岩墙、包体、石英闪长岩和花岗闪长岩等多种岩石类型.晶粥状态下壳-幔岩浆相互作用是控制东昆仑长英质火成岩多样性和大陆地壳生长演化的重要方式.      

北拉萨块体唐江穷果岩体中由同源岩浆不同期次之间混合产生的暗色包体:一种新的暗色包体岩石成因

在西藏北拉萨块体中段唐江穷果岩体中发现了一种新的岩石成因的暗色包体.唐江穷果岩体中暗色包体呈椭球状,与寄主岩之间呈不紧密胶结,在暗色包体和寄主岩的接触面上通常形成一个明显的风化间隙面.暗色包体为角闪闪长斑岩,寄主岩为花岗闪长岩,暗色包体明显较寄主岩更基性,更富Na₂O、CaO、MgO和Fe₂O₃T.暗色包体和寄主岩具有明显不同的稀土元素,暗色包体的稀土元素除La、Ce元素外,整体含量较寄主岩高,且轻重稀土分异弱.两者都具有弧岩浆岩的特征,富集Rb、Cs、K等大离子亲石元素和Th、U,而亏损Nb、Ta、Ti等高场强元素.暗色包体成岩年龄为113.9±1.0 Ma,寄主岩的成岩年龄为110±1.1 Ma,暗色包体成岩年龄较寄主岩早约4 Ma.此外,两者具有一致的锆石原位Lu-Hf同位素特征.以上岩相学、年代学、元素地球化学和同位素地球化学证据表明,唐江穷果暗色包体和寄主岩来源于同源母岩浆,暗色包体在二次岩浆房中经历了较弱的斜长石结晶分离作用,寄主岩在二次岩浆房中经历了较强的角闪石结晶分离作用.经过结晶分离作用的寄主岩岩浆在侵位过程中将较早形成处于半塑性状态下的暗色包体裹挟至近地表.唐江穷果暗色包体最可能的成因模式可以解释为同源岩浆不同期次间的物理混合.      

Zircon U–Pb geochronology,major-trace elements and Sr–Nd isotope geochemistry of Mashhad granodiorites (NE Iran) and their mafic microgranular enclaves: evidence for magma mixing and mingling

ABSTRACT

Mashhad granitoids and associated mafic microgranular enclaves (MMEs), in NE Iran record late early Mesozoic magmatism, was related to the Palaeo-Tethys closure and Iran-Eurasia collision. These represent ideal rocks to explore magmatic processes associated with Late Triassic closure of the Palaeo-Tethyan ocean and post-collisional magmatism. In this study, new geochronological data, whole-rock geochemistry, and Sr–Nd isotope data are presented for Mashhad granitoids and MMEs. LA–ICP–MS U–Pb dating of zircon yields crystallization ages of 205.0 ± 1.3 Ma for the MMEs, indicating their formation during the Late Triassic. This age is similar to the host granitoids. Our results including the major and trace elements discrimination diagrams, in combination with field and petrographic observations (such as ellipsoidal MMEs with feldspar megacrysts, disequilibrium textures of plagioclase), as well as mineral chemistry, suggest that MMEs formed by mixing of mafic and felsic magmas. The host granodiorite is a felsic, high K calc-alkaline I-type granitoid, with SiO₂ = 67.5–69.4 wt%, high K₂O (2.4–4.2 wt%), and low Mg# (42.5–50.5). Normalized abundances of LREEs and LILEs are enriched relative to HREEs and HFSEs (e.g. Nb, Ti). Negative values of whole-rock εNd_(t) (?3 to ?2.3) from granitoids indicate that the precursor magma was generated by partial melting of enriched lithospheric mantle with some contributions from old lower continental crust. In the MMEs, SiO₂ (53.4–58.2 wt%) is lower and Ni (3.9–49.7 ppm), Cr (0.8–93.9 ppm), Mg# (42.81–62.84), and εNd_(t) (?2.3 to +1.4) are higher than those in the host granodiorite, suggesting a greater contribution of mantle-derived mafic melts in the genesis of MMEs.     

普朗斑岩铜矿岩浆混合作用：岩石学及元素地球化学证据

普朗斑岩铜矿花岗闪长斑岩中存在大量的随机分布的镁铁质微粒包体,包体与寄主岩存在渐变接触关系。包体成分为闪长质,具有岩浆结构,存在针状磷灰石,显示了快速冷却结晶的特征。包体内可见具有暗色矿物镶边的眼球状石英,表明存在岩浆混合作用。寄主岩岩体规模较小,呈岩枝状产出,包体和寄主岩均为似斑状结构,说明两种岩浆侵位和发生岩浆混合作用的深度较浅。元素地球化学特征显示包体与寄主岩的之间有成分交换。包体和寄主岩强不相容元素均富集,高场强元素Nb、Ta、Ti均表现出显著的负异常,具有典型的岛弧岩浆岩的微量元素特征,包体和寄主岩Mg＃较高,在同等Si条件下比玄武岩部分熔融体富K2O和MgO,意味着源区必须有幔源岩浆的贡献。普朗斑岩铜矿蚀变矿化模式反映了其成矿环境偏基性,暗示镁铁质岩浆的加入对成矿具有贡献。     

西秦岭金厂石英闪长岩的岩浆混合成因：岩相学和锆石U-Pb年代学证据及其构造意义

位于西秦岭南部的金厂石英闪长岩岩体内含有大量镁铁质暗色微粒包体,包体大多呈浑圆状和水滴状,部分呈不规则拉长状,与寄主岩的接触界线截然或呈渐变过渡关系。石英闪长岩中的磷灰石呈短柱状,而包体中的磷灰石则呈细长针状,反映基性岩浆的快速冷凝结晶。石英闪长岩中的斜长石发育振荡环带,核部的斜长石An低,而边部斜长石An先急剧上升,复又下降;核部与边部之间存在明显的间断,同时斜长石边部包裹有暗色矿物,指示其形成时可能有更基性的岩浆注入。寄主岩中的角闪石大多为普通角闪石和镁普通角闪石,属SiO2饱和型,而包体中角闪石一部分为镁普通角闪石,属SiO2饱和型,一部分为韭闪石、韭闪石质普通角闪石,属SiO2不饱和类型。包体中的角闪石自核部到边部,Al2O3与TiO2含量急剧下降,说明核部和幔部相对于边部形成于更高温的环境。寄主岩中黑云母部分为铁质黑云母,部分为镁质黑云母,而包体中黑云母均为镁质黑云母,在∑FeO/(∑FeO+MgO)对MgO图解上寄主岩与包体中黑云母均落入壳-幔混源区。寄主岩和包体中的锆石均为典型的岩浆锆石,LA-ICP-MS锆石U-Pb定年表明它们的形成年龄分别为212±2Ma及215±1Ma(2σ),在误差范围内基本一致,证明二者同时形成。综合以上岩相学和年代学证据认为,金厂石英闪长岩和镁铁质暗色微粒包体是幔源基性岩浆和壳源酸性岩浆混合作用的产物,形成于秦岭造山带中三叠世造山后伸展环境。结合区域上的研究结果认为,中—晚三叠世时期的幔源岩浆底侵和下地壳部分熔融在西秦岭广泛存在。     

东昆仑沟里地区暗色包体及其寄主岩石地球化学特征及成因

通过青海东昆仑东部沟里地区阿斯哈岩体中寄主闪长岩和暗色微粒包体的岩相学、全岩地球化学研究,确定了岩石成因及其构造属性。阿斯哈岩体中暗色包体广泛分布,包体岩性主要为角闪辉长岩。包体具有岩浆结构,部分包体具有塑性流变特征,包体中可见寄主岩石矿物的捕掳晶和针状磷灰石,表现出岩浆混合的岩相学特征。主岩及暗色包体同属准铝质、高钾钙碱性-钾玄岩系列过渡岩石,主量元素在Harker图解及Al₂O₃/K₂O-CaO/K₂O和SiO₂/CaO-K₂O/CaO的共分母协变图上具良好的线性关系,反映两者成分的变化与岩浆混合作用有关。两者的稀土元素配分模式总体一致,显示二者密切的成因联系。两者都富含大离子亲石元素（Rb、K）,相对亏损高场强元素（Nb、Ta、P、Ti）。暗色包体具有贫硅（w(SiO₂)=50.70%~53.88%）和富镁、铁、钙的地球化学特征,其Mg^#值较高（Mg^#=0.52~0.59）,暗示其来源于俯冲带流体交代地幔楔的部分熔融。主岩的Rb/Sr值为0.22~0.27,接近地壳平均值,Nb/Ta值为14.5~15.2,介于地幔平均值与地壳平均值之间,表明寄主岩石岩浆具有壳源岩浆的性质并经历了幔源岩浆的混合作用。结合区域构造演化及构造判别,认为阿斯哈岩体形成于安第斯型活动大陆边缘的构造环境。早三叠世,阿尼玛卿洋向北俯冲,俯冲带流体交代地幔楔,导致其部分熔融形成基性岩浆,底侵的幔源基性岩浆诱发下地壳部分熔融并与之发生混合形成本区闪长岩,而其中的暗色包体为幔源岩浆混合不彻底的产物。     

西藏曲水碰撞花岗岩的混合成因：来自成因矿物学证据

西藏曲水碰撞花岗岩地处冈底斯构造-岩浆带中部,呈东西向平行雅鲁藏布缝合带分布.该岩体以花岗闪长岩、石英闪长岩为主,其次为石英二长闪长岩.岩体内普遍发育微粒镁铁质包体.对花岗闪长岩、石英闪长岩及微粒镁铁质包体的成因矿物学研究结果显示：（1）斜长石发育环带且边缘和核部偏基性,幔部酸性;（2）斜长石斑晶边缘常含有角闪石、黑云母等暗色矿物包体;（3）钾长石X射线结构分析显示自核部向边缘温度呈现逐渐升高的特点;（4）长石矿物中普遍含有较高的Cr、Ni、Co元素,明显不同于壳熔花岗岩;（5）角闪石、黑云母矿物MgO含量高于典型壳熔花岗岩;（6）包体中发育针状磷灰石和角闪石,显示为岩浆淬冷的结果.上述特征不可能用正常岩浆分异作用来解释,而更可能是壳-幔岩浆混合作用的结果.采用矿物温压计所得到的结果也符合混合后的岩浆演化特征.     

西准噶尔克拉玛依岩体的成因:年代学、岩石学和地球化学证据

西准噶尔地区克拉玛依岩体主要由闪长岩和花岗岩组成,锆石SHRIMP法给出的岩体结晶年龄为(315.5±2.8)Ma,为晚石炭世侵入岩.克拉玛依岩体具岛弧岩石的元素地球化学特征:总体上岩石富钠.A/CNK=0.57～0.84,富集LREE,(La/Yb)N=4.7～6.1,Eu显示弱负异常(δEu=0.76～0.91),...     

湘中紫云山岩体暗色微粒包体的成因:岩相学、全岩及矿物地球化学证据

暗色微粒包体广泛分布于湘中紫云山岩体中的似斑状角闪石黑云母花岗闪长岩中,但其研究程度较低.对具有火成结构的暗色微粒包体及其寄主岩进行了岩相学、全岩及长石、辉石、黑云母的矿物地球化学研究,探讨其岩石成因及构造意义.寄主岩的全岩主量、微粒元素较为均一,而暗色微粒包体变化较大,且后者相对贫SiO₂而富Na₂O,但总体上二者均具有准铝质、钙碱性、镁质的特征,均富集轻稀土和大离子亲石元素,而亏损重稀土和高场强元素.寄主岩和暗色微粒包体的斜长石、辉石和黑云母均分别属于中长石、次透辉石－低铁次透辉石和铁质黑云母的范畴,显示相似的矿物地球化学特征.详尽的岩相学和地球化学特征表明,寄主岩属于I型和ACG型花岗岩,具有明显壳幔混合的特点;而暗色微粒包体形成时处于液态并具有流动性,与寄主岩间存在明显的机械和化学混合作用,并具有早期为骤冷快速结晶、晚期缓慢结晶这两期过程.因此,紫云山岩体中出现大量暗色微粒包体,是印支晚期湘中地区在强烈挤压之后的松弛阶段,由于软流圈物质上涌,并与其诱发的壳源酸性岩浆混合作用的产物.      

塔里木南缘布雅花岗岩和暗色包体的锆石U-Pb年代学及地球化学特征

塔里木西南缘铁克里克地区广泛发育早古生代中酸性侵入岩,本文对其中布雅岩体及其暗色包体进行系统的岩石学、年代学及岩石地球化学研究,确定了岩石成因及其构造属性。LA-MC-ICP-MS锆石U-Pb年代学研究表明,寄主石英二长闪长岩结晶年龄为432.6±2.5 Ma(MSWD=1.5),暗色包体结晶年龄为432.4±6.4 Ma(MSWD=0.031),二者形成时代相同,均为志留纪早期岩浆活动的产物。地球化学特征表明,布雅暗色包体应来源于地幔的部分熔融,而寄主岩石岩浆具有壳源岩浆的性质并经历了幔源岩浆不均匀的混合。野外及岩相学特征均显示暗色包体为铁镁质岩浆注入长英质岩浆快速冷凝形成的,是幔源岩浆底侵下地壳形成的岩浆混合作用的产物。它们是塔里木南缘早古生代碰撞造山作用晚期的岩浆记录。     

Magma mixing/mingling in the Eocene Horoz (Nigde) granitoids, Central southern Turkey: evidence from mafic microgranular enclaves

Mafic microgranular enclaves (MMEs) are widespread in the Horoz pluton with granodiorite and granite units. Rounded to elliptical MMEs have variable size (from a few centimetres up to metres) and are generally fine-grained with typical magmatic textures. The plagioclase compositions of the MMEs range from An₁₈?CAn₆₄ in the cores to An₁₇?CAn₂₉ in the rims, while that of the host rocks varies from An₁₇ to An₅₅ in the cores to An₀₇ to An₃₃ in the rims. The biotite is mostly eastonitic, and the calcic-amphibole is magnesio-hornblende and edenite. Oxygen fugacity estimates from both groups?? biotites suggest that the Horoz magma possibly crystallised at fO₂ conditions above the nickel?Cnickel oxide (NNO) buffer. The significance of magma mixing in their genesis is highlighted by various petrographic and mineralogical characteristics such as resorption surfaces in plagioclases and amphibole; quartz ocelli rimmed by biotite and amphibole; sieve and boxy cellular textures, and sharp zoning discontinuities in plagioclase. The importance of magma mixing is also evident in the amphiboles of the host rocks, which are slightly richer in Si, Fe³⁺ and Mg in comparison with the amphiboles of MMEs. However, the compositional similarity of the plagioclase and biotite phenocrysts from MMEs and their host rocks suggests that the MMEs were predominantly equilibrated with their hosts. Evidence from petrography and mineral chemistry suggests that the adakitic Horoz MMEs could be developed from a mantle-derived, water-rich magma (>3 mass%) affected by a mixing of felsic melt at P >2.3?kbar, T >730°C.     

Double injection events of mafic magma into supersolidus Yucheon granites to produce two types of mafic enclaves in the Cretaceous Gyeongsang Basin,SE Korea

Petrographic and geochemical features of the Cretaceous Yucheon granites and their mafic microgranular/magmatic enclaves (MMEs), SE Korea, reveal that the MMEs originated from magma mixing. Mesoscopic and microscopic features indicate that mechanical mixing operated heterogeneously to produce the MMEs with a wide range of sizes and textures. Chemical compositions of amphibole, biotite, and plagioclase rims of both the MMEs and host granites are almost identical, indicating that chemical homogenization took place to some extent after the mechanical mixing. Plagioclase cores, however, have various compositions depending on the host rocks and/or sampling locations, suggesting their sluggish re-equilibration. The MMEs are divided into Type A (low TiO₂, very fine-grained, chilled margins) and Type B (high TiO₂, fine- to medium-grained, no chilled margins). The lower TiO₂ MMEs cooled more rapidly and interacted with granitic magma for a shorter period of time than the higher TiO₂ MMEs. Additionally, the former are less enriched in HREEs than the latter. Zoned plagioclase has two zones of increased An content. These features are indicative of double injection events of mafic magma. A previous model explains the magma mixing as resulting from the generation of a slab window due to Kula-Pacific ridge subduction. The model cannot, however, explain the eastward younging of the granites in Korea, necessitating a new, more elaborate model of Cretaceous geodynamics and magmatism in East Asia.     

Petrogenesis of mafic microgranular enclaves (MMEs) in the oligocene-miocene granitoid plutons from northwest Anatolia,Turkey

Mafic microgranular enclaves (MMEs) in host granitoids can provide important constraints on the deep magmatic processes. The Oligocene-Miocene granitoid plutons of the NW Anatolia contain abundant MMEs. This paper presents new hornblende Ar-Ar ages and whole-rock chemical and Sr-Nd isotope data of the MMEs from these granitic rocks. Petrographically, the MMEs are finer-grained than their host granites and contain the same minerals as their host rocks (amphibole + plagioclase + biotite + quartz + K-feldspar), but in different proportions. The Ar-Ar ages of the MMEs range from 27.9 ± 0.09 Ma to 19.3 ± 0.01 Ma and are within error of their respective host granitoids. The MMEs are metaluminous and calc-alkaline, similar to I-type granites. The Sr-Nd isotopes of MMEs are 0.7057 to 0.7101 for ⁸⁷Sr/⁸⁶Sr and 0.5123 to 0.5125 for ¹⁴³Nd/¹⁴⁴Nd, and are similar to their respective host granitoids. These lithological, petrochemical and isotopic characteristics suggest that the MMEs in this present study represent chilled early formed cogenetic hydrous magmas produced during a period of post-collisional lithospheric extension in NW Anatolia. The parental magma for MMEs and host granitoids might be derived from partial melting of underplated mafic materials in a normally thickened lower crust in a post-collisional extensional environment beneath the NW Anatolia. Delamination or convective removal of lithospheric mantle generated asthenospheric upwelling, providing heat and magma to induce hydrous re-melting of underplated mafic materials in the lower crust.     

同源岩浆不同期次之间混合产生的暗色包体——以北拉萨地块中部晚白垩世桑心日岩体为例

本文在研究西藏北拉萨块体中段桑心日岩体中的暗色包体时发现了一种具有特殊岩石成因的暗色包体。暗色包体呈椭球状,在暗色包体和寄主岩的接触面上通常形成一个明显的可能由风化作用造成的间隙面。暗色包体为二长玢岩-花岗闪长玢岩,寄主岩为花岗岩,暗色包体明显较寄主岩更基性,更富Na_2O、CaO、MgO和Fe_2O_3~T。暗色包体和寄主岩具有明显不同的稀土元素特征,暗色包体的稀土元素含量变化较大,最基性样品具有最高的稀土含量,随着基性程度的降低稀土元素含量明显下降。随着岩浆的进一步演化,岩浆向花岗岩方向演化,稀土含量又逐步升高。寄主岩和暗色包体具有基本一致的微量元素组成,具有典型的弧岩浆岩的特征,富集Rb、Cs、K等大离子亲石元素和Th、U,亏损Nb、Ta、Ti等高场强元素。此外,暗色包体和寄主岩具有明显的Ba、Sr的负异常。暗色包体成岩年龄为75. 6±1. 2Ma,寄主岩的成岩年龄为71. 8±0. 6Ma,暗色包体成岩年龄较寄主岩早约4Myr。两者具有一致的锆石原位Lu-Hf同位素特征。综合以上岩相学、年代学、元素地球化学和同位素地球化学证据,我们认为桑心日暗色包体和寄主岩来源于同源母岩浆,初始岩浆在母岩浆房中经历了不同程度的含钾角闪石结晶分离作用,并沿早期较弱的构造裂隙侵入到地壳的某一层位,随着构造活动进一步加剧,经过进一步分异母岩浆大规模上侵,并将早先侵位处于半塑性状态的暗色包体侵吞、裹挟至近地表。桑心日暗色包体最可能的成因模式可以解释为同源岩浆不同期次间的物理混合。     

东昆仑东段哈拉尕吐花岗岩基岩浆混合作用:来自岩石学和矿物学约束

哈拉尕吐花岗岩基位于东昆仑东段,其中花岗闪长岩岩浆混合作用明显,是研究岩浆混合作用的良好对象.从岩石学、岩相学和矿物化学等方面对哈拉尕吐花岗岩基进行了详细研究.电子探针结果显示:寄主岩斜长石的An值同相对应包体中斜长石捕掳晶近似;包体中基质斜长石大部分具核边结构,核部和边部An值存在间断;部分包体中浅色基质斜长石的An值与具核边结构斜长石的边部近似;辉长闪长岩中斜长石具较高的An值.寄主岩角闪石同相对应包体中角闪石捕掳晶的结晶温度、压力和氧逸度较为接近;包体中基质角闪石的结晶温度和压力低于寄主岩角闪石,氧逸度稍高于寄主岩角闪石;辉长闪长岩角闪石具有最高的结晶温度和压力及最低的氧逸度.哈图沟剖面和德福胜剖面寄主岩中的斜长石和角闪石的成分具有一定差别.岩浆不同期次侵入结晶和岩浆自身演化,使不同地点斜长石和角闪石的成分和物理化学特征具有一定变化.镁铁质岩浆位于地壳深部,氧逸度较低,使结晶的角闪石具有较高的形成压力和较低的氧逸度,斜长石具较高An值;随着镁铁质岩浆注入寄主岩,由于环境突变,使斜长石受到熔蚀;由于岩浆上侵以及两种岩浆物理化学性质差别较大,导致温度、压力和水饱和度降低,氧逸度升高,使包体中残留岩浆快速结晶,形成具核边结构、浅色均一的斜长石,以及结晶程度较差、较高氧逸度的角闪石.      

浙江雁荡山火山-侵入杂岩的岩浆混合作用——暗色包体中长石环带的证据

浙江雁荡山是中国东南部燕山晚期巨型火山-侵入杂岩带的重要组成部分。对其中央侵入相石英正长斑岩的暗色微粒包体中的斑晶和基质斜长石进行了详细的内部结构和成分分析,揭示了斜长石复杂环带的成因和相关的岩浆作用过程。斑晶斜长石由熔蚀的核部和表面干净的幔部组成,边部包裹有钾长石膜。核部斜长石呈浑圆状或港湾状,内部发育筛状结构,An成分显著低于幔部斜长石,代表来自酸性岩浆房中早期结晶的斜长石捕掳晶。同时,幔部斜长石与自形、表面干净的基质斜长石具有类似的An含量,且两者均含有针状磷灰石的包裹体,应结晶自与暗色微粒包体相应的基性岩浆。长石的复杂结构记录了雁荡山火山-侵入杂岩形成过程中的岩浆混合作用和岩浆演化过程。岩浆混合之后的火山喷发活动,造成岩浆房的压力突然减小,温压条件达到钾长石结晶的区域,在石英正长斑岩的斑晶斜长石和暗色包体中的斑晶与基质斜长石外均形成钾长石膜,构成反环斑结构。     

西秦岭德乌鲁岩体成因及地质意义——来自岩石地球化学的证据

西秦岭德乌鲁岩体位于夏河-合作断裂和力士山-围当山断裂之间,寄主岩石以花岗闪长岩为主,石英闪长岩和石英二长闪长岩次之,并含有大量暗色微粒包体(MMEs)。对德乌鲁岩体开展了年代学研究,获得的花岗闪长岩的LA-ICP-MS锆石U-Pb年龄为225.9±1.3 Ma,表明该岩体形成于晚三叠世早期,可能与扬子板块与华北板块陆陆碰撞有关。岩石地球化学研究表明,寄主岩石具有高K2O,低Y、MgO的特点,而暗色微细粒包体(MMEs)具低K2O,高Y、MgO的特点,在微量元素蛛网图解和稀土元素配分模式上它们具有类似的曲线,在Al_2O_3/MgOSiO_2/MgO图上呈现明显的线性关系,表明这些岩石之间发生了明显的物质交换,说明德乌鲁岩体中的石英闪长岩、石英二长闪长岩和花岗闪长岩是由镁铁质岩浆和长英质岩浆混合产生的,可能与扬子板块和华北板块陆陆碰撞后伸展环境下发生的强烈壳-幔相互作用有关。MMEs可能是镁铁质岩浆的残余物,地球化学特征显示可能有幔源物质的加入,并带来了Au、Cu等成矿元素,在岩体形成演化过程中生成富含Cu和Au的含矿热液,从而在德乌鲁岩体中形成了热液型铜金矿床。