星地碰撞的板块构造效应

板块构造是一种全球大地构造理论.它以洋底扩张、洋壳边缘俯冲及转换断层为主要构造活动形式,配以地幔对流为原动力,建立一套颇具魅力的板块构造机制理论,被受到广泛认同.但也存在一些重要问题,主要是其地幔对流理念难以令人信服和对海陆格局变迁问题没提出明确的动力机制.在阐明造成板块构造理论这两方面困难问题的主要理由之后,介绍了星地碰撞事件的存在状况及其动力作用,着重论述了大规模星地碰撞的动力作用强大,对全球地质构造活动都有重要影响,板块构造也难以避免;星地碰撞的强烈冲击作用,有能力造成洋底开裂或使大陆裂解.据此设想,可用"星地撞击成缝,减压诱发岩浆上侵"的模式,取代与地球内部层圈结构相抵触的"地幔对流"模式来解释洋底扩张;并以星地碰撞发生地点的随机变化性作为大规模海陆格局变迁的主控原因.如此,则可有助于上述板块构造理论中存在的两大难题的解决.     

“全新特提斯洋”概念与广义特提斯构造域

特提斯最初是指欧亚大陆南缘的古海洋,后逐渐引申出从元古宙、古生代到中生代的一系列位于劳亚大陆与冈瓦纳大陆之间的古大洋,如原特提斯洋、古特提斯洋和新特提斯洋,不同大洋在时间上前后交叠。如今横亘在冈瓦纳大陆(南极洲)和欧亚大陆之间的是印度洋,是新特提斯洋的继承者,可以另称为“全新特提斯洋”。这一概念的引申直接体现了印度洋与特提斯构造域一脉相承的关系,有助于将今论古、由此及彼,更直观地了解特提斯构造域的演化过程。本文按时间序列梳理了印度洋的大地构造演化和岩浆作用过程,识别了印度洋在155 Ma、120 Ma、90～84 Ma、76 Ma、65 Ma、52 Ma、45 Ma、38 Ma等关键时期的异常海底扩张记录,这些扩张事件将为标定新特提斯构造域的演化提供参照。其中155 Ma可能指示了新特提斯洋的鼎盛期,90 Ma指示了新特提斯洋的洋中脊俯冲,76～52 Ma是非洲-阿拉伯大陆与欧亚大陆初始碰撞-主碰撞(即新特提斯洋西部关闭)的时期,65～45 Ma是印度次大陆与欧亚大陆初始碰撞-主碰撞(即新特提斯洋中部关闭)的时期,38 Ma是澳大利亚北部大洋开始净俯冲(即新提斯洋东部开始消减)的时间。...     

文登南部陆—陆碰撞与流体成矿

本文通过对胶南－文荣碰撞带东段,即文登南部陆－陆碰撞带地质特征研究,探讨了Ａｇ→Ａｕ,Ａｇ→Ａｕ→Ａｕ,Ｐｂ,Ｚｎ→Ａｕ,Ｃｕ这一明显的矿化分带性与碰撞机制的关系,详细研究了碰撞带中石英包裹体特征,尤其是深入研究了石英包裹体中Ｈ２Ｏ和ＣＯ２含量变化特征与碰撞带中挤压构造及伸展构造耦合关系,提出了碰撞驱动流体与成矿的认识。     

大陆碰撞造山带的两类橄榄岩——以柴北缘超高压变质带为例

论述了大陆俯冲碰撞带中地幔橄榄岩的基本特征和成岩类型,并重点讨论柴北缘超高压变质带中不同性质的橄榄岩及其成因。根据岩石学特征,我们确定柴北缘超高压带中发育有两种类型的橄榄岩:(1)石榴橄榄岩,岩石类型包括石榴二辉橄榄岩、石榴方辉橄榄岩、纯橄岩和石榴辉石岩,是大陆型俯冲带的标志性岩石。金刚石包裹体、石榴石和橄榄石的出溶结构、温压计算等均反映其来源深度大于200km。地球化学特征表明该橄榄岩的原岩是岛弧环境下高镁岩浆在地幔环境下堆晶的产物。(2)大洋蛇绿岩型地幔橄榄岩,与变质的堆晶杂岩(包括石榴辉石岩、蓝晶石榴辉岩)和具有大洋玄武岩特征的榴辉岩构成典型的蛇绿岩剖面,代表大洋岩石圈残片。这两类橄榄岩的确定对了解柴北缘超高压变质带的性质和构造演化过程有重要意义。     

Early Eocene leucocratic sill/dike swarms in the Gangdese belt,southern Tibet: Tectonic implications for Indo-Asian collision

The timing of the initial Indo-Asian collision is a subject of debate for a long time. Besides, the magmatic trace of the collisional process is also unclear. In the present study, the authors report Early Eocene leucocratic sill/dike swarms in the northern edge of the Nymo intrusive complex of the Gangdese belt, southern Tibet. The Nymo intrusive complex was emplaced at ca. 50 –47 Ma and surrounded by the metamorphosed Jurassic-aged Bima Formation volcano-sedimentary sequence along its northern side. At outcrops, the leucocratic sills/dikes intruded along or truncated the deformed foliations of the host Bima Formation, which has been subject to high-temperature amphibolite-facies metamorphism at ca. 50 –47 Ma. Detailed cathodoluminescence image analyses reveal that the zircon grains of the leucocratic sills/dikes have core-mantle textures. The cores yield the Jurassic ages comparable to the protolith ages of the Bima Formation. In contrast, the mantles of zircon grains yield weighted mean ages of ca. 49–47 Ma, representing the crystallization timing of these leucocratic sills/dikes. The coeval ages for the Nymo intrusive complex, the high-temperature metamorphism, and the leucocratic sills/dikes indicate that a close relationship exists among them. The authors tentatively suggest that these leucocratic sills/dikes were generated from partial melting of the Jurassic-aged Bima Formation volcanic rocks, triggered by the high heat from the magma chamber of the Nymo intrusive complex. This Early Eocene tectono-thermal event of coeval magmatism, metamorphism and partial melting was most likely formed during the Indo-Asian collisional setting.©2021 China Geology Editorial Office.     

Element mobility during continental collision: insights from polymineralic metamorphic vein within UHP eclogite in the Dabie orogen

Metamorphic dehydration and partial melting are two important processes during continental collision. They have significant bearing on element transport at the slab interface under subduction‐zone P–T conditions. Petrological and geochemical insights into the two processes are provided by a comprehensive study of leucocratic veins in ultrahigh‐pressure (UHP) metamorphic rocks. This is exemplified by this study of a polymineralic vein within phengite‐bearing UHP eclogite in the Dabie orogen. The vein is primarily composed of quartz, kyanite, epidote and phengite, with minor accessory minerals such as garnet, rutile and zircon. Primary multiphase solid inclusions occur in garnet and epidote from the both vein and host eclogite. They are composed of quartz ± K‐feldspar ± plagioclase ± K‐bearing glass and exhibit irregular to negative crystal shapes that are surrounded by weak radial cracks. This suggests their precipitation from solute‐rich metamorphic fluid/melt that involved the reaction of phengite breakdown. Zircon U–Pb dating for the vein gave two groups of concordant ages at 217 ± 2 and 210 ± 2 Ma, indicating two episodes of zircon growth in the Late Triassic. The same minerals from the two rocks give consistent δ¹⁸O and δD values, suggesting that the vein‐forming fluid was directly derived from the host UHP eclogite. The vein is much richer in phengite and epidote than the host eclogite, suggesting that the fluid is associated with remarkable concentration of such water‐soluble elements as LILE and LREE migration. Garnet and rutile in the vein exhibit much higher contents of HREE (2.2–5.7 times) and Nb–Ta (1.8–2.0 times) than those in the eclogite, indicating that these normally water‐insoluble elements became mobile and then were sunken in the vein minerals. Thus, the vein‐forming agent would be primarily composed of the UHP aqueous fluid with minor amounts of the hydrous melt, which may even become a supercritical fluid to have a capacity to transport not only LILE and LREE but also HREE and HFSE at subduction‐zone metamorphic conditions. Taken together, significant amounts of trace elements were transported by the vein‐forming fluid due to the phengite breakdown inside the UHP eclogite during exhumation of the deeply subducted continental crust.     

Active tectonics of the Himalaya

The Himalayan mountains are a product of the collision between India and Eurasia which began in the Eocene. In the early stage of continental collision the development of a suture zone between two colliding plates took place. The continued convergence is accommodated along the suture zone and in the back-arc region. Further convergence results in intracrustal megathrust within the leading edge of the advancing Indian plate. In the Himalaya this stage is characterized by the intense uplift of the High Himalaya, the development of the Tibetan Plateau and the breaking-up of the central and eastern Asian continent. Although numerous models for the evolution of the Himalaya have been proposed, the available geological and geophysical data are consistent with an underthrusting model in which the Indian continental lithosphere underthrusts beneath the Himalaya and southern Tibet. Reflection profiles across the entire Himalaya and Tibet are needed to prove the existence of such underthrusting. Geodetic surveys across the High Himalaya are needed to determine the present state of the MCT as well as the rate of uplift and shortening within the Himalaya. Paleoseismicity studies are necessary to resolve the temporal and spatial patterns of major earthquake faulting along the segmented Himalayan mountains.     

内蒙古乌拉山金矿带中大桦背花岗岩与金矿床成因联系探讨

乌拉山金矿带大体背花岗岩成因属陆壳（改造）重熔型。花岗岩在成矿作用中的贡献，不仅能直接提供矿源，而且更重要的是间接提供矿源，花岗岩与金矿床在成因上、空间上、时间上有着密切联系，是形成（花岗岩）与被形成（矿床）的关系。指明乌拉山金矿具有三位一体成矿地质条件，即大古代变质岩系是金等成矿元素的提供者──—成矿基础，中生代构造──—岩浆活动是金等成矿元素的地质营力──—关键成矿作用，随之而进行的是金沿着构造裂隙（与之配套的断裂构造）集中、沉淀的成矿作用。     

Metamorphism and granite genesis in the Hidaka Metamorphic Belt, Hokkaido, Japan

The Main Zone of the Hidaka Metamorphic Belt is an uplifted crustal section of island-arc type. The crust was formed during early Tertiary time, as a result of collision between two arc–trench systems of Cretaceous age. The crustal metamorphic sequence is divided into four metamorphic zones (I–IV), in which zone IV is in the granulite facies. A detailed study of the evolution of the Hidaka Belt, based on a revised P–T–t analysis of the metamorphic rocks, notably a newly found staurolite-bearing granulite, confirms a prograde isobaric heating path, after a supposed event of tectonic thickening of accretionary sedimentary and oceanic crustal rocks. During the peak metamorphic event (c. 53 Ma), the regional geothermal gradient attained 33–40° C km^?1, and the highest P–T condition obtained from the lowest part of the granulite unit is 830° C, 7 kbar. In this part, X_H2O of Gt–Opx–Cd gneiss is about 0.15 and that of Gt–Cd–Bt gneiss is 0.4. The P–T–X_H2O condition of the granulite unit is well within a field where fluid-present partial melting of pelitic and greywacke metamorphic rocks takes place. This is in harmony with the restitic nature of the Gt–Opx–Cd gneiss in the lowest part of the granulite unit. The possibility that partial melting took place in the Main Zone is significant for the genesis of the peraluminous (S-type) granitic rocks within it. The S-type granitic rocks in this zone are Opx–Gt–Bt tonalite in the granulite zone, Gt–Cd–Bt tonalite in the amphibolite zone, and Cd–Bt–Mus tonalite in the Bt–Mus gneiss zone. The mineralogical and chemical nature of these strongly peraluminous tonalitic rocks permit them to be regarded as having been derived from S-type granitic magma generated by crustal anatexis of pelitic metamorphic rocks in deeper crust.     

陆内碰撞体制流体作用及成矿作用研究的意义和现状

陆内碰撞作用和流体作用都是８０年代以来的研究前沿，它们的研究必然会大大促进成矿作用研究的发展，也是跟踪和超越世界地球科学先进水平的重要途径。中国拥有最多最复杂的陆内碰撞带，为中国学者开发有关研究并取得高水平成果提供了得天独厚的条件。对陆内碰撞、流体作用和成矿作用研究现状的分析表明，三者之间研究的相互结合是薄弱环节，限制了有关问题的深入，但为我国学者开发该方向的研究，取得领先于国家水平的成果，提供了