博茨瓦纳赛莱比-皮奎铜镍硫化物矿床研究进展          下载免费PDF全文

任军平  许康康  刘晓阳  王杰  左立波  孙凯  何胜飞  贺福清 《地质找矿论丛》2015,30(S1):129-136

文章对博茨瓦纳铜镍硫化物矿床的研究成果进行了总结,概括了赛莱比-皮奎铜镍硫化物矿床的区域地质背景、岩石地层划分,较系统地分析了矿床的地质特征和矿床成因;认为铜镍硫化物矿床的成矿物质来源多样,并且矿床形成后经历了强烈的褶皱和剪切作用。  相似文献   

钦-杭结合带硅质岩的分布特征及其地质意义   总被引：3，自引：0，他引：3  

李红中  周永章  杨志军  高乐  何俊国  梁锦  曾长育  吕文超 《地学前缘》2015,22(2):108-117

钦州—杭州(钦-杭)结合带位于中国东南部地区,跨越浙江、江西、湖南、广东和广西5省(区)。大致以南岭为界,该带可划分为北、中、南三段。中段与南岭带重合,大致分布在北纬24°~27°范围,以北为北段,包括江西、浙江及安徽南部,以南为南段,包括粤西桂东南地区。钦-杭结合带跨带内沉积硅质岩广泛发育,地质和地球化学证据展示它们主要为热水成因。硅质岩相关的热水活动分布偏向于靠近结合带的两侧。钦-杭结合带"北、中、南"三段的硅质岩时空分布存在明显差异:南段及两侧邻区大规模热水活动集中于晚古生代,中段及两侧邻区的集中于早古生代,北段及邻区的热水活动集中于元古宙。这种大规模热水活动自北向南逐渐变新的特点与钦-杭结合带分段演化具有较好的对应关系。作为热水活动地质遗迹的硅质岩,其形成与大地构造与地球动力学背景的演化有密切的关系,特别是与钦-杭结合带的几个拉张阶段存在较好的对应关系。富含硅质的热水活动伴随了丰富的成矿作用,热水喷流沉积型块状硫化物矿床和热水沉积型金矿在该构造带内均较为典型。  相似文献   

西准噶尔蛇绿混杂岩中洋岛玄武岩研究新进展   总被引：2，自引：0，他引：2  

杨高学  李永军  佟丽莉  杨宝凯  张胜龙  沈锐  段丰浩 《地质学报》2015,89(2):392-405

洋岛玄武岩(OIB)起源研究是当代固体地球岩石学及地球化学最基本问题之一,通常被认为源于地幔柱。西准噶尔位于中亚造山带的西南缘,该地区发育多条蛇绿混杂岩带,主要包括唐巴勒、玛依勒、达尔布特及克拉玛依蛇绿混杂岩带,它们组成相似,主要为蛇纹岩、蛇纹石化方辉橄榄岩、二辉橄榄岩、纯橄岩、铬铁矿、辉石岩、辉长岩、辉绿岩、玄武岩(拉斑质和碱性)、硅质岩及斜长花岗岩。随着研究的不断深入,在西准噶尔蛇绿混杂岩带中不断有不同时代OIB被识别。这些玄武岩属于碱性玄武岩系列,具有高TiO2和FeOt,低MgO,强烈富集轻稀土元素特征,没有明显Nb、Ta负异常,与日喀则及夏威夷洋岛玄武岩地球化学特征极为相似,可能形成于大洋板内的海山或洋底高原,认为其成因与地幔柱相关,表明在西准噶尔(洋)的演化过程中,不仅是洋内俯冲系统,还伴有地幔柱活动。结合前人研究,认为中亚造山带可能是洋内俯冲+地幔柱复合的演化模型。同时,对中亚造山带中的OIB及OIB型玄武岩形成时代进行系统总结发现,它们不仅时代宽度大,并且具有连续发育的特点。对正确认识地幔柱活动在显生宙中亚造山带地壳增生过程中的贡献提供新的资料和证据。  相似文献   

Continental growth and reworking on the edge of the Columbia and Rodinia supercontinents; 1.86–0.9 Ga accretionary orogeny in southwest Fennoscandia     

Nick M.W. Roberts  Trond Slagstad 《International Geology Review》2015,57(11-12):1582-1606

Geological history from the late Palaeoproterozoic to early Neoproterozoic is dominated by the formation of the supercontinent Columbia, and its break-up and re-amalgamation into the next supercontinent, Rodinia. On a global scale, major orogenic events have been tied to the formation of either of these supercontinents, and records of extension are commonly linked to break-up events. Presented here is a synopsis of the geological evolution of southwest Fennoscandia during the ca. 1.9–0.9 Ga period. This region records a protracted history of continental growth and reworking in a long-lived accretionary orogen. Three major periods of continental growth are defined by the Transscandinavian Igneous Belt (1.86–1.66 Ga), Gothian (1.66–1.52 Ga), and Telemarkian (1.52–1.48 Ga) domains. The 1.47–1.38 Ga Hallandian–Danopolonian period featured reorganization of the subduction zone and over-riding plates, with limited evidence for continental collision. During the subsequent 1.38–1.15 Ga interval, the region is interpreted as being located inboard of a convergent margin that is not preserved today and hosted magmatism and sedimentation related to inboard extensional events. The 1.15–0.9 Ga period is host to Sveconorwegian orogenesis that marks the end of this long-lived accretionary orogen and features significant crustal deformation, metamorphism, and magmatism. Collision of an indenter, typically Amazonia, is commonly inferred for the cause of widespread Sveconorwegian orogenesis, but this remains inconclusive. An alternative is that orogenesis merely represents subduction, terrane accretion, crustal thickening, and burial and exhumation of continental crust, along an accretionary margin. During the Mesoproterozoic, southwest Fennoscandia was part of a much larger accretionary orogen that grew on the edge of the Columbia supercontinent and included Laurentia and Amazonia amongst other cratons. The chain of convergent margins along the western Pacific is the best analogue for this setting of Proterozoic crustal growth and tectonism.  相似文献   

Discovery of a binary Centaur     

Keith S. Noll  Harold F. Levison 《Icarus》2006,184(2):611-618

We have identified a binary companion to (42355) 2002 CR₄₆ in our ongoing deep survey using the Hubble Space Telescope's High Resolution Camera. It is the first companion to be found around an object in a non-resonant orbit that crosses the orbits of giant planets. Objects in orbits of this kind, the Centaurs, have experienced repeated strong scattering with one or more giant planets and therefore the survival of binaries in this transient population has been in question. Monte Carlo simulations suggest, however, that binaries in (42355) 2002 CR₄₆-like heliocentric orbits have a high probability of survival for reasonable estimates of the binary's still-unknown system mass and separation. Because Centaurs are thought to be precursors to short period comets, the question of the existence of binary comets naturally arises; none has yet been definitively identified. The discovery of one binary in a sample of eight observed by HST suggests that binaries in this population may not be uncommon.  相似文献   

Centaurs from the Oort cloud and the origin of Jupiter-family comets     

V. V. Emel'yanenko  D. J. Asher  M. E. Bailey 《Monthly notices of the Royal Astronomical Society》2005,361(4):1345-1351

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Evolution of regional metamorphism in the Cape Smith Thrust Belt (northern Quebec, Canada): interaction of tectonic and thermal processes     

M. R. ST-ONGE  S. B. LUCAS 《Journal of Metamorphic Geology》1991,9(5):515-534

Abstract Syn-metamorphic re-imbrication of the internal part of thrust belts can result in distinct pressure–temperature–time–deformation ( P–T–t–d ) pathways for different structural–metamorphic domains. In the early Proterozoic Cape Smith Thrust Belt (Canada), an external (piggyback-sequence thrusting) domain is characterized by thermal peak metamorphism occurring after deformation. In contrast, thermal peak metamorphism in an internal domain occurred during re-imbrication by out-of-sequence thrusting. The interactions of tectonic and thermal processes have been studied using three methods: (i) qualitative evaluation of the timing between mineral growth and deformation; (ii) analytical P–T paths from growth-zoned garnet porphyroblasts; and (iii) numerical modelling of vertical heat conduction. Derived P–T–t–d pathways suggest that uplift in the external domain resulted in part from erosion and isostatic unloading. In contrast, paths for the internal domain indicate that the out-of-sequence portion of the thrust belt may have experienced faster unroofing relative to the external domain. This is attributed to thickening by out-of-sequence thrusting and possibly to extensional faulting at (now eroded) higher structural levels. Observations on the timing of metamorphism, coupled with numerical modelling, suggest that the thermal peak metamorphism documented in the external domain is a consequence of the emplacement of the out-of-sequence thrusts stack in the internal portion of the thrust belt.  相似文献   

P–T–fluid evolution in the Mahalapye Complex, Limpopo high-grade terrane, eastern Botswana     

K. HISADA  L. L. PERCHUK  T. V. GERYA  D. D. VAN REENEN  B. K. PAYA 《Journal of Metamorphic Geology》2005,23(5):313-334

Metapelites, migmatites and granites from the c. 2 Ga Mahalapye Complex have been studied for determining the P–T–fluid influence on mineral assemblages and local equilibrium compositions in the rocks from the extreme southwestern part of the Central Zone of the Limpopo high‐grade terrane in Botswana. It was found that fluid infiltration played a leading role in the formation of the rocks. This conclusion is based on both well‐developed textures inferred to record metasomatic reactions, such as Bt ? And + Qtz + (K₂O) and Bt ± Qtz ? Sil + Kfs + Ms ± Pl, and zonation of Ms | Bt + Qtz | And + Qtz and Grt | Crd | Pl | Kfs + Qtz reflecting a perfect mobility (Korzhinskii terminology) of some chemical components. The conclusion is also supported by the results of a fluid inclusion study. CO₂ and H₂O ( = 0.6) are the major components of the fluid. The fluid has been trapped synchronously along the retrograde P–T path. The P–T path was derived using mineral thermobarometry and a combination of mineral thermometry and fluid inclusion density data. The Mahalapye Complex experienced low‐pressure granulite facies metamorphism with a retrograde evolution from 770 °C and 5.5 kbar to 560 °C and 2 kbar, presumably at c. 2 Ga.  相似文献   

The eruptive history of the Tequila volcanic field, western Mexico: ages, volumes, and relative proportions of lava types     

Catherine B. Lewis-Kenedi  Rebecca A. Lange  Chris M. Hall  Hugo Delgado-Granados 《Bulletin of Volcanology》2005,67(5):391-414

The eruptive history of the Tequila volcanic field (1600 km²) in the western Trans-Mexican Volcanic Belt is based on ⁴⁰Ar/³⁹Ar chronology and volume estimates for eruptive units younger than 1 Ma. Ages are reported for 49 volcanic units, including Volcán Tequila (an andesitic stratovolcano) and peripheral domes, flows, and scoria cones. Volumes of volcanic units 1 Ma were obtained with the aid of field mapping, ortho aerial photographs, digital elevation models (DEMs), and ArcGIS software. Between 1120 and 200 kyrs ago, a bimodal distribution of rhyolite (~35 km³) and high-Ti basalt (~39 km³) dominated the volcanic field. Between 685 and 225 kyrs ago, less than 3 km³ of andesite and dacite erupted from more than 15 isolated vents; these lavas are crystal-poor and show little evidence of storage in an upper crustal chamber. Approximately 200 kyr ago, ~31 km³ of andesite erupted to form the stratocone of Volcán Tequila. The phenocryst assemblage of these lavas suggests storage within a chamber at ~2–3 km depth. After a hiatus of ~110 kyrs, ~15 km³ of andesite erupted along the W and SE flanks of Volcán Tequila at ~90 ka, most likely from a second, discrete magma chamber located at ~5–6 km depth. The youngest volcanic feature (~60 ka) is the small andesitic volcano Cerro Tomasillo (~2 km³). Over the last 1 Myr, a total of 128±22 km³ of lava erupted in the Tequila volcanic field, leading to an average eruption rate of ~0.13 km³/kyr. This volume erupted over ~1600 km², leading to an average lava accumulation rate of ~8 cm/kyr. The relative proportions of lava types are ~22–43% basalt, ~0.4–1% basaltic andesite, ~29–54% andesite, ~2–3% dacite, and ~18–40% rhyolite. On the basis of eruptive sequence, proportions of lava types, phenocryst assemblages, textures, and chemical composition, the lavas do not reflect the differentiation of a single (or only a few) parental liquids in a long-lived magma chamber. The rhyolites are geochemically diverse and were likely formed by episodic partial melting of upper crustal rocks in response to emplacement of basalts. There are no examples of mingled rhyolitic and basaltic magmas. Whatever mechanism is invoked to explain the generation of andesite at the Tequila volcanic field, it must be consistent with a dominantly bimodal distribution of high-Ti basalt and rhyolite for an 800 kyr interval beginning ~1 Ma, which abruptly switched to punctuated bursts of predominantly andesitic volcanism over the last 200 kyrs.Electronic Supplementary Material Supplementary material is available in the online version of this article at Editorial responsility: J. Donnelly-NolanThis revised version was published online in January 2005 with corrections to Tables 1 and 3.An erratum to this article can be found at  相似文献   

Evolution of a complex isolated dome system,Cerro Pizarro,central México     

Nancy?RiggsEmail author  Gerardo?Carrasco-Nunez 《Bulletin of Volcanology》2004,66(4):322-335

Cerro Pizarro is an isolated rhyolitic dome in the intermontane Serdán-Oriental basin, located in the eastern Trans-Mexican Volcanic Belt. Cerro Pizarro erupted ~1.1 km³ of magma at about 220 ka. Activity of Cerro Pizarro started with vent-clearing explosions at some depth; the resultant deposits contain clasts of local basement rocks, including Cretaceous limestone, ~0.46-Ma welded tuff, and basaltic lava. Subsequent explosive eruptions during earliest dome growth produced an alternating sequence of surge and fallout layers from an inferred small dome. As the dome grew both vertically and laterally, it developed an external glassy carapace due to rapid chilling. Instability of the dome during emplacement caused the partial gravitational collapse of its flanks producing various block-and-ash-flow deposits. After a brief period of repose, re-injection of magma caused formation of a cryptodome with pronounced deformation of the vitrophyric dome and the underlying units to orientations as steep as near vertical. This stage began apparently as a gas-poor eruption and no explosive phases accompanied the emplacement of the cryptodome. Soon after emplacement of the cryptodome, however, the western flank of the edifice catastrophically collapsed, causing a debris avalanche. A hiatus in eruptive activity was marked by erosion of the cone and emplacement of ignimbrite derived from a caldera to the north of Cerro Pizarro. The final growth of the dome growth produced its present shape; this growth was accompanied by multiple eruptions producing surge and fallout deposits that mantle the topography around Cerro Pizarro. The evolution of the Cerro Pizarro dome holds aspects in common with classic dome models and with larger stratovolcano systems. We suggest that models that predict a simple evolution for domes fail to account for possibilities in evolutionary paths. Specifically, the formation of a cryptodome in the early stages of dome formation may be far more common than generally recognized. Likewise, sector collapse of a dome, although apparently rare, is a potential hazard that must be recognized and for which planning must be done.Editorial responsibility: J. Gilbert  相似文献