拉萨地体内低速异常成因的探讨--壳内局部熔融的地震层析证据

青藏高原南部天然地震体波的层析反演图像描绘出拉萨地体内在15～90km深度内低速异常的分布特征。在研究速度结构的基础上，根据熔融程度与纵波波速呈倒数衰减的特性，论证了拉萨地体中低速体的出现与壳内的局部熔融有关。壳内局部熔融则来源于板块俯冲、地壳增厚产生的热而非幔源侵入所造成。同时，也发现了在拉萨以东中下地壳低速体有向东发展的趋势。大面积部分熔融层分布的深度范围约在15～35km处。另外，据藏南地区的SKS波分裂时间延迟很小的特点，推测藏南地幔中可能不存在各向异性，也就是没有足够的热源使各向异性矿物的品格重新定位。这从另一方面佐证了部分熔融仅存在于地壳内而不是地幔中。     

Origin of Exceptionally Abundant Phonolites on Ua Pou Island (Marquesas, French Polynesia): Partial Melting of Basanites Followed by Crustal Contamination

On the basis of the first systematic mapping of Ua Pou, longknown for its exceptionally abundant phonolites, we estimatethat these rocks cover 65% of the surface of the island whereasmafic lavas cover 27% and intermediate ones 8%. The silica-undersaturatedsuite was erupted in a restricted time span (2·9–2·35Myr), following the emplacement of tholeiites derived from ayoung HIMU-type source at c. 4 Ma. Primitive basanites, derivedfrom a heterogeneous mantle source with a dominant EM II + HIMUsignature, represent likely parental magmas. The series is characterizedby a Daly gap defined by a lack of phonotephrites. We considerthat the most likely model for the origin of evolved lavas ispartial melting at depth of primitive basanites, leaving anamphibole-rich residuum and producing tephriphonolitic magmas.These tephriphonolitic magmas may have evolved by closed-systemfractional crystallization towards Group A phonolites. Threeother groups of phonolites could have been derived from tephriphonoliticmagmas by open-system fractional crystallization processes,characterized respectively by seawater contamination (GroupB), assimilation of nepheline syenite-type materials (GroupC) and extreme fractionation coupled with assimilation of theunderlying oceanic crust (Group D). The prominence of evolvedlavas is a consequence of their origin from partial meltingof mafic precursors followed by crustal contamination. KEY WORDS: Marquesas; French Polynesia; phonolite; partial melting; contamination     

辽西义县晚白垩世大兴庄组流纹岩的地球化学特征及其成因

辽西义县晚白垩世大兴庄组流纹岩具有埃达克质火山岩的特征.这些流纹岩SiO₂≥68.62%、Al₂O₃≥14.40%、MgO < 1.2%(Mg# < 0.45)、Sr＞360μg/g、Yb < 1.1μg/g、Y < 12μg/g、La/Yb＞40、Sr/Y≥39和Nb/Ta＞17.5;轻稀土元素富集, 重稀土元素和高场强元素(如Nb、Ta、Ti)明显亏损, 轻重稀土元素强烈分馏, 具有弱的负铕异常; Nd、Sr同位素具有较低的143Nd/144Nd(0.511376~0.511441, ε_Nd(t)=-23.45~-22.16)和适中的87Sr/86Sr(0.7073~0.7074, ε_Sr(t)=32.38~32.8)比值, 具有富集地幔端员(EMI)特点.这些特征表明, 大兴庄组流纹质岩浆起源于较厚下地壳榴辉岩部分融熔, 也说明中生代晚期局部仍残留较厚的下地壳, 这为进一步理解燕山造山带中生代到新生代岩石圈减薄提供了重要信息.      

Geodynamic Information in Peridotite Petrology

Systematic differences are observed in the petrology and majorelement geochemistry of natural peridotite samples from thesea floor near oceanic ridges and subduction zones, the mantlesection of ophiolites, massif peridotites, and xenoliths ofcratonic mantle in kimberlite. Some of these differences reflectvariable temperature and pressure conditions of melt extraction,and these have been calibrated by a parameterization of experimentaldata on fertile mantle peridotite. Abyssal peridotites are examplesof cold residues produced at oceanic ridges. High-MgO peridotitesfrom the Ronda massif are examples of hot residues producedin a plume. Most peridotites from subduction zones and ophiolitesare too enriched in SiO₂ and too depleted in Al₂O₃ to be residues,and were produced by melt–rock reaction of a precursorprotolith. Peridotite xenoliths from the Japan, Cascades andChile–Patagonian back-arcs are possible examples of arcprecursors, and they have the characteristics of hot residues.Opx-rich cratonic mantle is similar to subduction zone peridotites,but there are important differences in FeO_T. Opx-poor xenolithsof cratonic mantle were hot residues of primary magmas with16–20% MgO, and they may have formed in either ancientplumes or hot ridges. Cratonic mantle was not produced as aresidue of Archean komatiites. KEY WORDS: peridotite; residues; fractional melting; abyssal; cratonic mantle; subduction zone; ophiolite; potential temperature; plumes; hot ridges     

Silica depleted melting of pelites. Petrogenetic grid and application to the Susqueda Aureole, Spain

Metapelitic rocks in the low pressure contact metamorphic aureole around the Susqueda igneous complex, Spain show a number of features that make them an ideal testing ground for the modelling of silica‐undersaturated melting. Rocks in the aureole experienced localized depletion in silica by the segregation of quartz veins during a pre‐anatectic, regional cordierite‐andalusite grade metamorphic event. These rocks were then intruded by gabbroic to dioritic rocks of the Susqueda igneous complex that formed a migmatitic contact metamorphic aureole in the country rocks. This migmatisation event caused quartz‐saturated hornfels and restite formation in rocks that had experienced no quartz vein segregation in the previous regional metamorphic event, but silica‐undersaturated melting in those rocks that were previously depleted in silica. Silica‐undersaturated melting is investigated using a new petrogenetic P–T projection and equilibrium pseudosections calculated in the KFMASH and NCKFMASH systems, respectively. The grid considers quartz absent equilibria and a range of phases that form typically in silica‐undersaturated bulk compositions, for example corundum. It is shown that the quartz‐rich precursors in the Susqueda contact aureole produced about 10% melt during contact metamorphism. However, most of this melt was extracted leaving behind rocks with restitic bulk compositions and minor leucosome segregation. It is suggested that the melt mixed with the host igneous rocks causing an apparent magmatic zoning from diorite in the centre of the complex to tonalite at the margins. In contrast, the quartz‐poor precursors (from which the quartz veins segregated) melted in the silica‐undersaturated field producing a range of assemblages including peritectic corundum and spinel. Melting of the silica‐undersaturated rocks produced only negligible melt and no subsequent melt loss.     

Archaean high-K granitoids produced by remelting of earlier Tonalite–Trondhjemite–Granodiorite (TTG) in the Sangmelima region of the Ntem complex of the Congo craton,southern Cameroon

We present a geochemical and isotopic study that, consistent with observed field relations, suggest Sangmelima late Archaean high-K granite was derived by partial melting of older Archaean TTG. The TTG formations are sodic-trondhjemitic, showing calcic and calc-alkalic trends and are metaluminous to peraluminous. High-K granites in contrast show a potassic calc-alkaline affinity that spans the calcic, calc-alkalic, alkali-calcic and alkalic compositions. The two rock groups (TTG and high-K granites) on the other hand are both ferroan and magnesian. They have a similar degree of fractionation for LREE but a different one for HREE. Nd model ages and Sr/Y ratios define Mesoarchaean and slab-mantle derived magma compositions respectively, with Nb and Ti anomalies indicating a subduction setting for the TTG. Major and trace element in addition to Sr and Nd isotopic compositions support field observations that indicate the derivation of the high-K granitic group from the partial melting of the older TTG equivalent at depth. Geochemical characteristics of the high-K granitic group are therefore inherited features from the TTG protolith and cannot be used for determining their tectonic setting. The heat budget required for TTG partial melting is ascribed to the upwelling of the mantle marked by a doleritic event of identical age as the generated high-K granite melts. The cause of this upwelling is related to linear delamination along mega-shear zones in an intracontinental setting.     

辽宁后仙峪硼矿区混合岩的LA-MC-ICP-MS锆石U-Pb年龄：对硼矿成矿演化的制约

辽东硼矿赋存于辽吉裂谷带的古元古代火山—沉积岩系之中,属沉积—变质型硼矿床,主矿区包括有后仙峪硼镁矿、翁泉沟硼铁矿和砖庙—杨木杆硼镁矿,一直以来是我国硼矿石的主产地。本次研究在后仙峪硼矿区采集了矿区外围的条痕状混合花岗岩(DSQ-08)和矿体上盘侵位于电英岩之中的含电气石混合花岗岩(HXY-19),挑选出其中的锆石单矿物进行LA-MC-ICP-MS测年。条痕状混合花岗岩中锆石的核部具有岩浆振荡环带,Th/U值为0.64~0.96,~(207)Pb/~(206)Pb年龄为2240±4Ma;含电气石混合花岗岩中锆石的内核和边部均具有极为清晰的岩浆振荡环带,Th/U值分别为0.12~1.05和0.41~1.08,~(207)Pb/~(206)Pb年龄分别记录了2157±6Ma和1932±26Ma两次锆石生长事件。含电气石的混合花岗岩的锆石边部形成于混合岩化过程之中,记录了辽河群下部岩石在1.9Ga左右发生的部分熔融作用事件,具有重要的地质意义。矿区外围的条痕状混合花岗岩和矿体周缘含电气石混合花岗岩的核部岩浆年龄较为接近,说明两种岩石可能均由古元古代的火山—沉积岩,在1.9Ga左右经部分熔融作用形成。因此,结合前人在后仙峪硼矿区内进行的硼同位素地球化学和岩相学方面的研究成果,我们认为后仙峪硼矿区混合花岗岩的锆石核部U-Pb年龄可基本确定辽吉裂谷早期的超基性火山岩和酸性火山岩的喷发、海相蒸发沉积事件均发生于2240~2157Ma左右,该时期的蒸发沉积作用初步形成硼酸盐矿;后期强烈的部分熔融和混合岩化作用发生在1932±26Ma,在超基性火山岩保护下,硼矿发生变质和小规模的迁移,形成了硼镁矿、硼镁铁矿及矿体周缘的电英岩和含电气石混合花岗岩。     

富氟花岗岩中萤石岩浆成因的新证据

通过富氟花岗岩-HF-H2O体系的熔化-结晶实验,在620～700℃、1×108Pa条件下获得了石英+碱性长石+黄玉+云母+萤石的矿物组合.在该实验体系中首次发现了八面体萤石.实验结果表明,在岩浆条件下可以形成萤石,从而为富氟花岗岩中萤石的岩浆成因提供了新证据.     

1.0GPa和常温至1100 ℃条件下角闪石斜长片麻岩的V_p变化:实验测量与理论计算

在1．0GPa、常温至1100℃条件下测量了角闪石斜长片麻岩的纵波速度（Vp）,并统计了不同温度实验产物中各种矿物的体积百分含量。结果显示,1．0GPa下,角闪石斜长片麻岩的Vp首先随温度升高（室温至700℃）缓慢降低约6％,然后（700—850℃）快速降低约6％,再（850～950℃）转而急剧升高15％～25％,最后（T〉950℃）又快速下降。实验产物分析表明在高温高压下α-石英-β石英相变和岩石部分熔融是岩石Vp异常变化的主要因素。由取样产物的矿物含量和弹性参数,计算了各温度条件下岩石的Vp得出与实验测量相同的波速-温度变化趋势,即Vp随温度升高先缓慢降低,接着快速降低后又急剧升高,最后又快速减小。实验测量和理论计算对比研究表明,通过高温高压下岩石中的物相变化观测结果进行岩石波速的计算,是检验岩石弹性波速测量结果和研究地球内部地震波结构的一种有效方法。     

胶北晚中生代煌斑岩的岩石地球化学特征及其成因研究

胶北煌斑岩分别采自龙口、烟台和威海地区，包括拉辉煌斑岩、斜闪正煌岩和角闪煌斑岩，煌斑岩K—Ar全岩年龄变化于89．3～169．5Ma，为晚中生代岩浆活动的产物。在岩石化学组成上，SiO2=42．02％～54．95％，以钙碱性系列为主．岩石以富集大离子亲石元素（LILE）（Ba，U，K，Th）和LREE，亏损高场强元素（HFSE）（Nb，Ta和Ti）为特征，Mg^#=33．9～53．9，Eu／Eu^＊=0．71～0．89，^87Sr／^86Sr初始比值0．707642～0．709791，εNd（t）为-17．6～-10．4，^206Pb／^204Pb=37．588～38．431，^207Pb／^204Pb=15．423～15．531，^206Pb／^204Pb=17．204～18．179。表明煌斑岩源自俯冲陆壳（扬子下地壳）在地幔源区发生交代作用时形成的富集型地幔的部分熔融体．考虑到煌斑岩具有大陆边缘弧玄武岩的特征，我们认为煌斑岩在成因上同样与古大洋板块的俯冲作用有关，为碰撞后弧岩浆作用形成的脉岩。