Alpine metamorphism of low-grade schists from the Slavonian Mountains (Croatia): new P-T and geochronological constraints

Low-grade schists from the Slavonian Mountains (Tisia Mega-Unit, Mt Papuk, Croatia), previously assigned to Precambrian to Lower Palaeozoic metamorphism, have been subjected to geochemical investigations, P-T modelling, and in situ age dating of monazite. The studied fine-grained metasediments consist of chlorite (5–15 vol.%), K white-mica (40–55 vol.%), quartz (20–35 vol.%), feldspar (albite 15–20 vol.%), opaques (<2 vol.%), and accessory minerals. According to their whole-rock geochemistry, the detritus of the former sediments came from upper crustal felsic rocks as they occur, for instance, at Mt Papuk. The schists show a complex microtectonic fabric, including well-developed schistosity systems. P-T pseudosections in the system MnNCKFMASHTO, constructed for typical schists of the study area, resulted in peak P-T conditions of 445–465 °C and 4.6–6.0 kbar for a sample from Kutjevo (eastern part of the study area) and 450–460 °C and 5.2–6.0 for a Vranovo sample (western part). Electron microprobe (EMP) dating of monazite in the schists gave a weighted average age of 109.0 ± 13.1 Ma (2σ) eventually with three subgroups of ages at 225 ± 63 (two analyses), 114 ± 24 and 83 ± 22 Ma. We conclude that the metamorphism of the studied schists at depths of c. 20 km is due to an Alpine collisional event.     

关于巴罗式变质带的最新研究及其对研究秦岭杂岩的意义

本文对苏格兰高地Grampian造山运动中产生的经典巴罗变质带进行了讨论,重点介绍了近年来关于其变质作用的特征及发生机制认识方面的重大变化。强调巴罗变质作用仅发生在整个造山运动过程中的部分时段,纪录了短暂的加热过程,时空上与区域内大规模的双峰式岩浆活动有关。经典的巴罗变质系列并非形成于地壳增厚及其热弛豫,而是代表了中地壳内大规模的接触变质作用。参考经典地区的变质特征,对发育巴罗式变质作用的秦岭杂岩进行了初步对比分析,指出其中与夕线石有关的变质P-T-t轨迹可能是等压冷却过程,而不是等温降压的顺时针演化模式。秦岭杂岩的变质作用时间仍需要进一步准确厘定。结合其它相关地质特征的分析和对比,得出如下推论:巴罗式变质带发育地区的变质作用、混合岩与花岗岩均属于同一动力系统作用的结果,花岗质岩体不是变质作用的原因;基性岩浆可能提供了巴罗式变质作用发生所需要的热能,但不是必要条件;巴罗式变质作用可以发生在正常地壳厚度情况下,不是碰撞构造的标志;伴随热异常的变形过程中产生了变质带的梯度分布(巴罗式变质带)和一些花岗岩,形成类似于底辟的冲起构造。     

阿尔金南缘金鸿山-俄博梁地区石墨矿化特征及找矿前景分析

素有"黑金子"称谓的石墨,是传统工业和战略性新兴产业必须的矿物原料。文章以阿尔金南缘金鸿山—俄博梁地区的晶质石墨矿床为研究对象,通过成矿地质条件、控矿因素研究,分析了矿床成因。认为金鸿山—俄博梁地区具备较好的晶质石墨矿找矿潜力。     

玄武质陨石NWA8545的岩石地球化学特征以及对其母体岩浆过程的启示

NWA 8545 是一块玄武质无球粒陨石,它与碳质陨石(CC)NWA 011 成对.CC 被认为是来自于外太阳系的一类物质,由于同位素异常,它们区别于来自内太阳系的非碳质陨石(NC).NWA 011 及其成对陨石作为CC中稀有的玄武质无球粒陨石,其记录的岩浆过程可以被用来研究外太阳系早期行星母体的岩浆活动.本文利用扫描电镜、电子探针和激光剥蚀电感耦合等离子质谱仪(LA-ICP-MS)对NWA 8545 中的辉石、斜长石和陨磷钙钠石进行岩相学以及原位主微量元素的分析,并根据矿物模式丰度计算全岩稀土元素含量.电子探针结果显示NWA 8545 与 HED族陨石Eucrite(钙长辉长无球粒陨石)具有相似的主量元素特征,同时其岩相学与5 型Eucrite类似.激光微量数据表明辉石、斜长石和陨磷钙钠石的稀土元素配分都表现出略微的Ce异常,但其辉石的Ba、Sr等元素并未出现明显的富集现象,即该陨石受地球风化作用影响不明显.利用辉石和斜长石的稀土元素含量,计算平衡熔体的成分,显示其平衡熔体的成分都与全岩的成分比较接近,可以认为两者是在封闭的体系下接近同时结晶.结合变质过程和母体岩浆的成分,本文认为NWA 8545 是由其母体岩浆在经历分离结晶过程后喷发到母体行星表面冷却形成的.     

福建凤山矿区石墨矿地质特征及控矿因素分析

通过对福建省漳平市凤山矿区石墨矿近年来硐探、钻探等地质资料系统的梳理,在分析矿区地质特征和矿体特征的基础上,深入研究了石墨矿的控矿因素。研究认为该区石墨矿是由赋存于中二叠统童子岩组的无烟煤经过高温、高压作用进一步变质而成的。煤层受到岩浆热变质作用使碳物质(煤)分解,重新富集形成以隐晶质(土状)为主的隐晶质石墨矿,因此本区石墨矿的控矿因素是温度和构造。由于过往对福建煤系石墨资源的研究程度不够深入,造成大部分煤系石墨矿划归煤矿,致使石墨矿资源被浪费,本次通过野外地质勘查、采样样品测试等工作,确定了凤山矿区为煤系石墨矿,为下一步勘探工作提供有力依据,为合理开发利用矿产资源指明新的方向。     

Fluid fluxes during low-temperature alteration: implications of multi-style alteration assemblages from the Welsh Borderland,UK

Localized (domainal) low-temperature alteration may indicate variations in the chemistry of alteration fluids and/or discrete fluid flow paths during metamorphism. Occurrences of epidote- and pumpellyite-dominated domains are often used as evidence for large fluxes of Ca-rich fluids. However, comparative studies of two domainal alteration styles from basaltic to andesitic lavas and volcaniclastic rocks at Builth Wells, Wales, UK suggest that such interpretations cannot be applied universally. Here, only one set of domains can be attributed to large fluxes of Ca-rich fluids. In contrast, the second set of domains formed where the host rock supplied the necessary Ca, and fluid/rock ratios were relatively low. These domains are hosted by rocks which show a Caledonian regional metamorphic imprint, characterized by the alteration assemblage albite+chlorite+titanite±prehnite±pumpellyite±calcite±muscovite±quartz (considered to have formed at c. 200°C and ≤2.5 kbar). Type 1 domains lie along fluid channelways, such as veins. Pumpellyite is the dominant secondary mineral, but the alteration assemblage is variable with pumpellyite±prehnite±calcite±titanite±chlorite (±quartz). The domains formed at temperatures of 130–230°C during Ordovician hydrothermal activity, before the peak of regional metamorphism. In contrast, Type 2 domains are not associated with obvious fluid channelways. A central prehnite-dominated zone typically has a rim with the assemblage pumpellyite+calcite±prehnite±chlorite±titanite±K-rich phyllosilicate. These domains probably formed from pelitic xenoliths which contained a volcaniclastic component at temperatures of 130–230°C and at relatively low fluid/rock ratios. However, the timing of domain formation is uncertain. Pyrobitumen, in veins and disseminated throughout the rock, may have influenced the formation of both types of domain by stabilizing pumpellyite in preference to epidote and causing metamorphic calcite formation through the release of CO₂ to the alteration fluids. © 1996 John Wiley & Sons, Ltd.     

四川丹巴穹状变质地体

四川西部丹巴地区最为引人注目的地质构造是穹状变质地体的发育。华北、扬子和羌塘三个板块之间的南北向和东西向双向收缩,引起区内发育了大小不等的十几个穹状变质地体,自北而南有马奈、春牛场、丹巴、公差、格宗等变质穹隆。多数穹隆的核部出露的是前寒武纪的片麻岩和混合岩,例如春牛场侵入体。其中的片麻岩原岩、黑云母和角闪石质片麻岩均属本区最老的岩石。它不整合于志留纪地层之下,年代学研究证明其年代属新元古代(大约865~785Ma)。混合岩从形态上说,多为条带状,偶见角砾状的角闪石质混合岩。但是也有不少穹隆,核部是花岗岩类。岩石化学研究证明,它们大多属于S型花岗岩,仅个别为I型。穹状变质地体的外围变质带可分三类:(1)巴罗带型区域递增变质带,有的显示变质带的倒转;(2)巴肯型变质带;(3)低级区域变质带,多数是中压绿片岩相。巴罗带变质的泥质岩,多数变晶矿物如黑云母、十字石、石榴石均具早期低级变质矿物的定向包裹物,显示明显叠加变质的信息。变质泥质岩的∑REE=(195~274)×10-6,(La/Yb)n=0·811~1·917。稀土配分曲线和微量元素蛛网图具Nb、P、Ti负异常,显示大陆地壳的特征,是陆缘碎屑物质区域变质产物。巴肯带出露于丹巴以北,主要变质泥质岩是夕线石片麻岩类,常见铁铝榴石而少见堇青石,说明原岩富铁贫镁,局部出现锌铁尖晶石。由北侧的巴肯带到巴罗型变质的公差穹隆到南部的格宗穹隆变质带是从高温到低温连续变化的。因之,我们倾向于认为松潘—甘孜造山带的东南缘是一个规模较大的、呈NE向分布的低—中压区域变质带,总体是一条热轴,垂直走向,向东南温度逐步降低。据前人同位素年龄资料:M1巴罗型区域变质发生于约210~205Ma,马奈花岗岩U-Pb锆石年龄为(197±6)Ma。M2巴肯型变质与岩体侵入有关,年龄约为164Ma。M3喜马拉雅期重结晶的黑云母年龄约为30Ma。总之,丹巴变质穹隆的形成是青藏高原东北部地质构造演化中重要的一幕,其主要活动期起于印支晚期最后结束于喜马拉雅期的隆升和挤出。依据低压高温变质带的空间分布,推测本区印支末期存在一NE向的热轴,同时也是S型花岗岩体的出露区。至于木里一带穹隆与丹巴穹隆在变质程度上的差异,应当归因于印支晚期的陆壳增厚过程中,北倾南倒逆冲剪切造成区域热流的不均一性。也说明了青藏高原东北缘在喜山期隆升之前具有复杂的构造变质历史。     

应用P-T-t理论再认识辽河群变质作用

辽河群是出露于辽宁省东部的独具特色的古元古代变质岩系,赋存丰富的矿产资源,研究历史悠久.但对有关辽河群变质作用的一些重要问题上看法诸多,很难取得一致意见.本文应用P-T-t轨迹理论重新认识这些问题,认为引起辽河群变质作用的根本原因是大陆碰撞造山带使辽河群俯冲到地下深处;辽河群变质作用在时间上和空间上有独特的演化特征;辽河群变质作用与不同规模的构造或不同层次的构造的关系是不一样的.     

The boyndie syncline,a D1 structure in the Dalradian of Scotland

The structure of the Dalradian rocks of the Banffshire coast has been re-examined. It is shown that D₁ structures face upwards along the entire section and the major Boyndie Syncline (Sutton and Watson 1956) must also be of D₁, age and not D₃ as proposed by Johnson (1962). D₂ structures are developed in the west, most strongly in the Portsoy Group and Cowhythe Gneiss where they may be related to the Portsoy Thrust (Elles 1931). East of the Cowhythe Gneiss D₂ structures are not developed but D₃ structures are of local importance. Porphyroblast growth is considered to be post-D₁, pre-D₃ related to the ‘active’ D₂ deformation in the west (Barrovian) and to the ‘static’ D₂ interval in the east (Buchan). The wider implications of these conclusions for Dalradian structure are briefly considered.     

变质作用、板块构造及超级大陆旋回

麻粒岩相超高温变质作用（GUHTM）主要发育于新太古代至寒武纪岩石中;推测在深部较年轻的,特别是新生代造山带岩石中也会有GUHTM存在。岩石中最初出现GUHTM记录意味着产生瞬时极高热流处的地球动力学发生了改变。许多GUHTM带可能发育于类似现代大陆弧后的构造背景中。在较热的地球上,超大陆及其裂解形成的循环组合,尤其是经岩石圈减薄的洋盆卷入到其外翻过程中可能产生比现代太平洋边缘更热的大陆弧后。中温榴辉岩 高压麻粒岩相变质作用（EHPGM）也是最先发现于新太古代岩石记录中,并发育于从元古宙至古生代岩石中。EHPGM带是对GUHTM带的补充,并经常认为是记录了从俯冲至碰撞造山作用的过程。在元古宙岩石记录中的蓝片岩明显记录了与现代俯冲作用相关的低热流梯度。以发育柯石英(±硬柱石)或金刚石为特征的硬柱石蓝片岩和榴辉岩（高压变质作用,HPM）及超高压变质岩（UHPM）主要是在显生宙形成。HPMUHPM记录了显生宙俯冲碰撞造山带早期碰撞过程中的低热流梯度及陆壳的深俯冲作用。尽管与直觉不同,在超级大陆聚敛期（Wilson旋回洋盆打开和关闭）的大陆地块增生过程,许多HPMUHPM带看来确实是通过小洋盆关闭而发育起来的,反映双重热体制的双重变质带仅发育于新太古代以来的岩石记录中。双重热体制是现代板块构造的特点,而双重变质作用则是板块构造在岩石记录中的特征性标志。尽管构造样式很可能不同,新太古代以来GUHTM和EHPGM带的发育证明“元古宙板块构造体制”的开始。以冷俯冲和大陆地壳深俯冲至地幔,以及其中的部分又从深达300 km处发生折返为标志,“元古宙板块构造体制”在新元古代进化为“现代板块构造体制”,这个转变可由岩石中的HPMUHPM证明。记录这种极端条件的变质带年龄是不一致的,而变质作用发生时间与各大陆岩石圈聚合到超级克拉通（如Superia/Sclavia）或超级大陆（如Nuna (Columbia), Rodinia, Gondwana, 和Pangea）的时间却是一致的。