递增变质作用过程中化学元素的演化规律———以山西五台群变质同位地层为例

山西五台群文溪组和柏枝岩组岩石学特征和岩石化学、微量元素及稀土元素特征研究表明，这两个组中相应层位地球化学特征基本一致。递增变质作用使岩石贫Ｎａ２Ｏ、Ｋ２Ｏ及大离子亲石元素和相对富集ＦｅＯ、ＭｇＯ及铁族元素。由于变质作用仅使稀土元素总量发生微小变化，而不改变其总体分布型式，所以稀土元素是指示岩石形成与演化的良好指示剂     

东秦岭松树沟高压变质基性岩石及其退变质作用的PTt演化轨迹

在北秦岭商南松树沟出露的高压变质基性岩石，包括高压基性麻粒岩和石榴单斜辉石岩，遭受了从中压麻粒岩相、高角闪岩相到绿帘角闪岩相的连续的退变质作用的改造。这些岩石形成的温度为８２６℃～８８７℃，压力约为１．４０～１．５８ＧＰａ，其不同退变质阶段的温压条件依次分别是７６５℃～８２５℃和约１．０３～１．１４ＧＰａ、６５０℃～７５０℃和约０．９ＧＰａ以及４００℃～５００℃和约０．５～０．６ＧＰａ。它们共同构成一个早期近等温降压（ＩＴＤ）和晚期降温降压的顺时针ＰＴｔ演化轨迹。结合高压岩石９８３±１４０Ｍａ的退变质年龄和松树沟残存的蛇绿岩片考虑，这些高压岩石的形成和抬升与秦岭造山带中、晚元古宙时期洋壳的俯冲、消减和陆块碰撞伴随的快速构造上升作用有关。     

High-Pressure and Ultrahigh-Pressure Metamorphic Belt in Tongbai-Dabie Mountains,Central China

There are four units of high-pressure to ultrahigh-pressure metamorphism extending from south to north across the Tongbai-Dabie Mountains: the epidote-blueschist-facies unit, the low-temperature eclogite facies unit , the ultrahigh-pressure eclngite facies unit and the medium-temperature eclogite facies unit . The later two units were formed during the Caledonian subduction between the Tongbai-Dabie microplate and the North China plate ,the former two units are the products of Indosinian continental-continental subduction and collision between the Yangtze and the North China plates.     

北秦岭官坡地区高压—超高压榴辉岩岩相学及变质作用研究

北秦岭官坡地区的榴辉岩及含柯石英榴辉岩产在帮岭岩群的北侧，主要由绿辉石和石榴石组成，部分石榴石和绿辉石中含柯石英包体。此外还含有退变质的多硅白云母、角闪石、黝帘石和纳长石等矿物，根据变质矿物之间的替代关系及共生组合规律，榴辉岩退变质作用可划分为四个阶段，各阶段代表性矿物组合依次为：柯石英＋绿辉石＋石榴石；石英＋绿辉石＋石榴石；多硅白云母＋绿辉石＋石榴石＋石英；角闪石＋斜长石＋白云母＋黑云母。这四个     

冀东太古宙高级变质岩区若干地质问题的研究

在1∶5万区域地质填图及专题研究的基础上探讨了变质岩石中的岩浆侵位变形构造、褶皱构造及变形与变质作用的关系等三个方面的问题。研究表明冀东太古宙高级区变质岩石中不同程度地发育岩浆岩构造,包括在不同类型片麻岩之间所表现的穿切构造、基性岩墙中的矿物定向构造以及基性岩体边缘及其围岩的变形构造等,褶皱构造可分为表壳岩褶皱及片麻岩褶皱,高级区可能不存在大型的片麻岩褶皱,通过镜下特征矿物相的研究并结合野外变质基性岩墙的产状及特征,建立区域变质与变形作用的关系,从而为区域地质事件表的建立提供依据。     

Geodynamic significance of ophiolites within the Calabrian Arc

Abstract Slices of oceanic lithosphere belonging to the neo‐Tethys realm crop out discontinuously in the northern Calabrian Arc, Southern Apennines. They consist of high‐pressure–low‐temperature metamorphic ophiolitic sequences formed from metaultramafics, metabasites and alternating metapelites, metarenites, marbles and calcschist. Ophiolites occupy an intermediate position in the northern Calabrian Arc nappe pile, situated between overlying Hercynian continental crust and the underlying Apenninic limestone units. In the literature, these ophiolitic sequences are subdivided into several tectonometamorphic units. Geochemical characteristics indicate that metabasites were derived from subalkaline basalts with tholeiitic affinity (transitional mid‐oceanic ridge basalt type), and a harzburgitic‐lherzolitic protolith is suggested for the serpentinites. The pressure–temperature‐deformation paths of the metabasites from different outcrops display similar features: (i) the prograde segment follows a typical Alpine geothermal gradient up to a metamorphic climax at 350°C and 0.9 GPa and crystallization of the high‐pressure mineral assemblage occurs along a pervasive foliation developed during a compressive tectonic event; and (ii) the retrogression path can be subdivided in two segments, the first is characterized by nearly isothermal decompression to approximately 400°C and 0.3 GPa and the second follows a cooling trajectory. During low‐pressure conditions, a second deformation event produces millimetric to decametric scale asymmetric folds that describe west‐verging major structures. The third deformation event is characterized by brittle extensional structures. The tectonometamorphic evolution of the ophiolitic sequences from the different outcrops is similar. Both thermobarometric modeling and tectonic history indicate that the studied rocks underwent Alpine subduction and exhumation processes as tectonic slices inside a west‐verging accretionary wedge. The subduction of oceanic lithosphere was towards the present east; therefore, the Hercynian continental crust, overthrusted on the ophiolitic accretionary wedge after the neo‐Tethys closure, was part of the African paleomargin or a continental microplate between Africa and Europe.     

On the origin of oriented rutile needles in garnet from UHP eclogites

Although oriented rutile needles in garnet have been reported from several ultrahigh‐pressure (UHP) rocks and considered to be important UHP indicators, their crystallographic features including growth habit and lattice correspondences with garnet host have never been properly characterized. This paper presents a detailed analytical electron microscopic (AEM) study on evenly distributed oriented rutile needles in garnet of two eclogitic rocks from Sulu. Some garnet in one UHP diamondiferous quartzofeldspathic rock from the Saxonian Erzgebirge, and in one high‐pressure (HP) felsic granulite from Bohemia also contain a few unevenly distributed oriented rutile needles. They have also been studied for the purpose of comparison. Despite different distribution patterns, AEM revealed that all rutile needles are oriented along the 〈111〉 directions of garnet with their lateral sides surrounded by the {110} planes of garnet, and that the growth directions of most needles are close to the normal of the {101} planes of rutile. No other specific crystallographic orientation relationships between rutile and garnet host were observed, and there is no pyroxene associated with rutile, as necessitated by the precipitation reaction of rutile in garnet as previously proposed. A simple solid‐state precipitation scenario for the formation of the rutile needles in garnet in these two eclogitic rocks is not justified. Three alternative mechanisms are considered for the formation of oriented rutile needles: (i) the rutile needles may be inherited from precursor minerals; (ii) the rutile needles may be formed by a dissolution–reprecipitation mechanism; and (iii) the rutile needles may be formed by cleaving and healing of garnet with rutile deposition. None of these mechanisms can fully explain the observations, although the first one is less likely and the third one is preferred. This study presents an example where the presence of oriented/aligned inclusions in minerals does not necessarily imply a precipitation origin.     

Accessory phase petrogenesis in relation to major phase assemblages in pelites from the Nelson contact aureole, southern British Columbia

Monazite petrogenesis in the Nelson contact aureole is the result of allanite breakdown close to, but downgrade and therefore independent of, major phase isograds involving cordierite, andalusite and staurolite. The development of garnet downgrade of the staurolite and andalusite isograds does not appear to affect the onset of the allanite-to-monazite reaction but does affect the textural development of monazite. In lower pressure, garnet-absent rocks, allanite breakdown results in localized monazite growth as pseudomorphous clusters. In higher pressure, garnet-bearing rocks, allanite breakdown produces randomly distributed, lone grains of monazite with no textural relationship to the original reaction site. Fluids liberated from hydrous phases (chlorite, muscovite) during garnet formation may have acted as a flux to distribute light rare earth elements more widely within the rock upon allanite breakdown, preventing the localized formation of monazite pseudomorphs. Despite these textural differences, both types of monazite have very similar chemistry and an indistinguishable age by electron microprobe chemical dating (157 ± 6.4 Ma). This age range is within error of isotopic ages determined by others for the Nelson Batholith. Garnet from the garnet, staurolite and andalusite zones shows euhedral Y zoning typified by a high-Y core, low-Y collar and moderate-Y annulus, the latter ascribed to allanite breakdown during garnet growth in the garnet zone. The cause of the transition from high-Y core to low-Y collar, traditionally interpreted to be due to xenotime consumption, is unclear because of the ubiquitous presence of xenotime. Accessory phase geothermometry involving monazite, xenotime and garnet returns inconsistent results, suggesting calibration problems or a lack of equilibration between phases.     

陕西略阳铜厂铜矿成矿时代及地质意义

根据铜厂铜矿床辉钼矿ＲｅＯｓ同位素模式年龄和黄铜矿ＲｂＳｒ同位素等时线年龄分别为８８９Ｍａ和３５９Ｍａ,并依据其地质特征和与铜厂岩体之间时空关系,认为早期铜矿化发生在８８９Ｍａ左右,与铜厂岩体岩浆期后热液有关;晚期铜矿化则发生在３５９Ｍａ左右,是伴随区域动力变质作用发生的;其矿质来源研究表明既有来自围岩的,又有来自岩体本身的;包裹体测温资料表明成矿温度集中在两个区间：高温大于３００℃,低温１５０～２００℃。该矿床为多期、复源、多种成矿作用叠加复合的产物。