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1.
The first data on the age of detrital zircons are given for Late Precambrian terrigenous rocks of the Baikal Group and Ushakovka Formation of the southern flank of the Siberian Craton. The ages obtained for 348 zircons cover the Paleoarchean to Late Ediacaran period, demonstrate the dynamics of change of sources of the clastic material in the sedimentation basin, and mark the changes of the Late Precambrian tectonic regimes. The age of the youngest group of detrital zircons extracted from the rocks of the Kachergat Formation allows us to restrict the upper age limit of accumulation of the rocks of the Baikal Group to the Late Ediacaran (Late Vendian).  相似文献   

2.
中生代华北克拉通破坏是目前引人关注的研究课题。鉴于目前一些文章在表达克拉通状态时引用的地质图件不准确,忽略了华北克拉通从古至今的不同阶段的演化,不能正确的表达克拉通在破坏之前或之后的状态,本文强调华北克拉通破坏前的状态是研究的重要基础。华北克拉通是经历过多期克拉通化形成的。  相似文献   

3.
The Rb-Sr age of metasomatic rocks from four gold deposits and occurrences localized in Archean granite-greenstone belts of the western, central, and southern Karelian Craton of the Baltic Shield has been determined. At the Pedrolampi deposit in central Karelia, the dated Au-bearing beresite and quartz-carbonate veins are located in the shear zone and replace Mesoarchean (~2.9 Ga) mafic and felsic metavolcanic rocks of the Koikar-Kobozero greenstone belt. At the Taloveis ore occurrence in the Kostomuksha greenstone belt of western Karelia, the dated beresite replaces Neoarchean (~2.7 Ga) granitoids and is conjugated with quartz veins in the shear zone. At the Faddeinkelja occurrence of southern Karelia, Aubearing beresite in the large tectonic zone, which transects Archean granite and Paleoproterozoic mafic dikes, has been studied. At the Hatunoja occurrence in the Jalonvaara greenstone belt of southwestern Karelia, the studied quartz veins and related gold mineralization are localized in Archean granitoids. The Rb-Sr isochrons based on whole-rock samples and minerals from ore-bearing and metasomatic wall rocks and veins yielded ~1.7 Ga for all studied objects. This age is interpreted as the time of development of ore-bearing tectonic zones and ore-forming hydrothermal metasomatic alteration. New isotopic data in combination with the results obtained by our precursors allow us to recognize the Paleoproterozoic stage of gold mineralization in the Karelian Craton. This stage was unrelated to the Archean crust formation in the Karelian Block and is a repercussion of the Paleoproterozoic (2.0–1.7 Ga) crust-forming tectonic cycle, which gave rise to the formation of the Svecofennian and Lapland-Kola foldbelts in the framework of the Karelain Craton. The oreforming capability of Paleoproterozoic tectonics in the Archean complexes of the Karelian Craton was probably not great, and its main role consisted in reworking of the Archean gold mineralization of various genetic types, including the inferred orogenic mesothermal gold concentrations.  相似文献   

4.
First finds of microfossils from the silicified microphytolitic carbonates of the Uluntui Formation in the southwestern Baikal region are described. They are represented by remains of the cyanobacterial community that formed microphytolites. These microfossils are accompanied by acritarchs probably belonging to green algae. The silicified microfossils are sufficiently well preserved despite complete and repeated recrystallization of host primary carbonate rocks. Main phases of secondary mineralization are related to hydrothermal-metasomatic processes, which were likely provoked by collisional events on the southern flank of the Siberian Craton in the Silurian.  相似文献   

5.
Despite representing one of the largest cratons on Earth, the early geological evolution of the Amazonia Craton remains poorly known due to relatively poor exposure and because younger metamorphic and tectonic events have obscured initial information. In this study, we investigated the sedimentary archives of the Carajás Basin to unravel the early geological evolution of the southeastern Amazonia Craton. The Carajás Basin contains sedimentary rocks that were deposited throughout a long period spanning more than one billion years from the Mesoarchean to the Paleoproterozoic. The oldest archives preserved in this basin consist of a few ca. 3.6 Ga detrital zircon grains showing that the geological roots of the Amazonia Craton were already formed by the Eoarchean. During the Paleoarchean or the early Mesoarchean (<3.1 Ga), the Carajás Basin was large and rigid enough to sustain the formation and preservation of the Rio Novo Group greenstone belt. Later, during the Neoarchean, at ca. 2.7 Ga, the southeastern Amazonia Craton witnessed the emplacement of the Parauapebas Large Igneous Province (LIP) that probably covered a large part of the craton and was associated with the deposition of some of the world largest iron formations. The emplacement of this LIP immediately preceded a period of continental extension that formed a rift infilled first by iron formations followed by terrigenous sediments. This major change of sedimentary regime might have been controlled by the regional tectonic evolution of the Amazonia Craton and its emergence above sea-level. During the Paleoproterozoic, at ca. 2.1 Ga, the Rio Fresco Group, consisting of terrigenous sediments from the interior of the Amazonia Craton, was deposited in the Carajás Basin. At that time, the Amazonian lithosphere could have either underwent thermal subsidence forming a large intracratonic basin or could have been deformed by long wavelength flexures that induced the formation of basins and swells throughout the craton under the influence of the growing Transamazonian mountain belt.  相似文献   

6.
小秦岭地区是华北克拉通南缘早前寒武纪基底重要分布区,可见大量构造抬升剥露的基底结晶杂岩带。太华杂岩是小秦岭出露最古老的地质体,对于探讨华北克拉通南缘早期地壳形成和演化及其构造归属等问题具有重要意义。在小秦岭地区,太华杂岩被划分为正片麻岩系和以孔兹岩系为主的表壳岩。利用LA-ICP-MS锆石U-Pb定年方法测得小秦岭地区太华杂岩表壳岩中黑云斜长片麻岩碎屑锆石的源区物质主要形成于2.40~2.11 Ga,经历了两期的古元古代晚期变质事件(~2.04 Ga和~1.91 Ga),限定该套表壳岩的沉积时代介于2.11~1.91 Ga。结合锆石Hf同位素特征,我们认为该表壳岩的碎屑物质可能主要来自中条山的涑水杂岩体及绛县杂岩体、熊耳花岗岩体、小秦岭古元古代花岗岩体等,其初始的源区物质可能为太华杂岩的新太古代正片麻岩系。此外,本研究揭示华北中部造山带可能记录了一个长达约250 Ma(~2.05~1.8 Ga)持续的俯冲-碰撞过程。  相似文献   

7.
Following terrane amalgamation of early oceanic lithosphere, the southern and central parts of the Kaapvaal Craton were a coherent unit by 3.1 Ga. Juxta-position of the northern and western granitoid-greenstone terranes including the Murchison Island Arc was the result of terrane accretion that started at 3.1 Ga. The culmination of these events was the collision of the Kaapvaal Craton, the pre-cratonic Zimbabwe block and the Central Zone to generate the Limpopo granulite gneiss terrane. Coeval with these orogenic events the central Kaapvaal Craton underwent extension to accommodate the development of the Dominion, Witwatersrand/Pongola and Ventersdorp basins. The craton scale Thabazimbi-Murchison Lineament development during the 3.1 Ga accretion event and continued to influence the tectonic evolution of the Kaapvaal block throughout the period under review as indicated by the syn-sedimentary tectonics of the > 2.64 Ga Wolkberg Group, overlying Black Reef Formation and the Transvaal Sequence. The Transvaal and Griqualand West basins developed in the Late Archaean (> 2.55 Ga) with basin dynamics influenced by far field stresses related to the Limpopo Orogeny. During this period the Thabazimbi-Murchison Lineament lay close to the northern margin of the depository. Reactivation of the Lineament between 2.4 and 2.2 Ga resulted in inversion of the Transvaal Basin and formation of the northward verging Mhlapitsi fold and thrust belt. The half-graben setting envisaged for the deposition of the Pretoria Group was influenced by the Thabazimbi-Murchison Lineament as was the emplacement and subsequent deformation of the Bushveld Complex.  相似文献   

8.
The western flank of the Paleoproterozoic Imandra-Varzuga rift zone consists of three volcanogenic-sedimentary series and layered mafic-ultramafic intrusions of different age (2.50–2.45 Ga). The earliest Monchegorsk and Monche Tundra layered massifs were formed about 2.50 Ga during the prerift stage of the evolution of the Imandra-Varzuga zone. The early rift stage (~2.45 Ga) produced layered intrusions of the Imandra complex and volcanic rocks of the Strelna Group, consisting of the Kuksha and Seidorechka formations. In terms of chemical composition, the volcanic rocks of the Seidorechka Formation belong to a single basalt-rhyolite series, mostly of normal alkalinity and both tholeiitic and calc-alkaline affinity. The rocks of the Imandra Complex are characterized by moderate LREE enrichment, relatively flat HREE patterns, and a positive Eu anomaly. Similar REE distribution patterns were observed in the volcanic rocks of the Seidorechka Formation, which show a gradual increase in REE content with increasing SiO2. The upper part of the Seidorechka Formation in the southern Khibiny region is composed of metarhyodacites. They terminate the sequence of the Strelna Group and have a U-Pb zircon age of 2448 ± 8 Ma. This age presumably reflects the upper age boundary of the rocks of the Seidorechka Formation and the end of the early stage of the evolution of the Imandra-Varzuga zone. Xenogenic zircon from the same sample yielded a U-Pb zircon age of 2715 ± 42 Ma. A U-Pb age of 2202 ± 17 Ma was obtained for titanite and rutile and interpreted as the metamorphic age of the Seidorechka Formation. The metavolcanic rocks of the Seidorechka Formation have negative ?Nd (T) varying from ?2.84 to ?2.32, and ISr values of 0.7041–0.7038, which are higher than those of the depleted mantle and suggest their derivation from an enriched mantle reservoir (EM1). The spatial association of the volcanic rocks of the Seidorechka Formation and the rocks of the Imandra Complex, similarity in the behavior of most major elements, similar REE distribution patterns, and close formation ages and isotope signatures give grounds to combine them in a single volcanoplutonic association.  相似文献   

9.
华北中部造山带南缘华山地区太华变质杂岩中锆石U-Pb定年   总被引:11,自引:0,他引:11  
华山太华变质杂岩出露于华北克拉通中部造山带最南缘,区内斜长角闪片麻岩呈"透镜状"或"似层状"产出于黑云斜长片麻岩或TTG片麻岩中。大多数含有石榴子石变斑晶的变质岩中,保留了至少3期变形形迹和3个阶段的变质矿物组合。本文对斜长角闪片麻岩和黑云斜长片麻岩中的锆石,进行了SIMS和LA-ICP-MSU-Pb定年。斜长角闪片麻岩的岩浆锆石年龄为2.29Ga,表明其原岩形成于古元古代。斜长角闪片麻岩、黑云斜长片麻岩中的变质锆石及锆石变质增生边年龄为1.94~1.82Ga,表明华山地区比华北克拉通中部造山带中段及北段其他地区普遍记录的约1.85Ga的变质事件,不仅早了约0.1Ga,且变质事件持续达0.1Ga之久。这说明华北中部造山带前寒武纪期间的构造-变质事件是一个比较漫长的复杂过程。  相似文献   

10.
Geological data on the Precambrian basic complexes of the Siberian Craton and their isotopic age are considered. The three main episodes of Precambrian basic magmatism of Siberia correspond to certain stages of the geodynamic evolution of the craton and the Earth as a whole. In the Late Paleoproterozoic, largely in the south and the north of the craton, the basic rocks were emplaced against the background of post-collision extension, which followed the preceding collision-accretion stage responsible for the formation of the craton. In the Mesoproterozoic, primarily in the north of the craton, basic magmatism was controlled by dispersed within-plate extension apparently caused by the impact of a mantle plume. Neoproterozoic basic magmatism widespread in the southern and southeastern parts of the craton was caused by rifting, which accompanied breakdown of the Rodinia supercontinent and opening of the Paleoasian ocean along the southern margin of the Siberian Craton.  相似文献   

11.
The U-Pb age of the manganotantalite from rare-metal pegmatites of the Vishnyakovskoe deposit (East Sayan Belt) has been assessed at 1838 ± 3 Ma. The acquired data indicate the pegmatites of this deposit and associated granites of the Sayan complex belong to the postcollision South Siberian igneous belt (1.88–1.84 Ga), which stretches along the southwestern frame of the Siberian Craton by more than 2500 km, from the Yenisei Ridge to the Aldan Shield. Formation of this igneous belt is related to joining (starting from about 1.9 Ga BP) of the series of continental microplates and island arcs to the Siberian Craton; this led to final stabilization of the craton at about 1.8 Ga BP.  相似文献   

12.
The autonomous (massif-type) anorthosite massifs of the Kalar Complex (2623 ± 23 Ma) intrude high-grade metamorphic rocks of the Kurulta tectonic block at the junction of the Aldan and Dzhugdzhur-Stanovoi fold area. These rocks belong to the most ancient anorthosite-mangerite-charnockite-granite (AMCG) magmatic association, whose origin was constrained to the Mesoproterozoic (1.8–1.1 Ga). The charnockites are typical high-potassium reduced granites like rapakivi, which affiliate with the A type. The Nd and Pb isotopic composition of these rocks suggests their predominantly crustal genesis, whereas the anorthosites were most probably produced by a mantle magma that was significantly contaminated by crustal material at various depth levels. The intrusions of the Kalar Complex were emplaced in a postcollision environment, with the time gap between the collisional event and the emplacement of these massifs no longer than 30 m.y. The southern Siberian Platform includes two definitely distinguished and spatially separated AMCG associations, which have different ages and tectonic settings: (i) the Late Archean (2.62 Ga) postcollision Kalar plutonic complex and (ii) the Early Proterozoic (1.74–1.70 Ga) anorogenic Ulkan-Dzhugdzhur volcano-plutonic complex.  相似文献   

13.
The Archean Wyoming Craton is flanked on the south and east by belts of Paleoproterozoic supracrustal successions whose correlation is complicated by lack of geochronologic constraints and continuous outcrop. However, carbonate units in these successions may be correlated by integrating carbon isotope stratigraphy with lithostratigraphy. The 10 km thick Paleoproterozoic Snowy Pass Supergroup in the Medicine Bow Mountains was deposited on the present-day southern flank of the Wyoming Craton; it contains three discrete levels of glacial diamictite correlative with those in the Huronian Supergroup, on the southern margin of the Superior Craton. The Nash Fork Formation of the upper Snowy Pass Supergroup is significantly younger than the uppermost diamictite and was deposited after the end of the Paleoproterozoic glacial epoch. Carbonates at the base of the Nash Fork Formation record remarkable 13C-enrichment, up to +28‰ (V-PDB), whereas those from overlying members of the lower Nash Fork Formation have δ13C values between +6 and +8‰. Carbonates from the upper Nash Fork Formation above the carbonaceous shale have carbon isotope values ranging between 0 and +2.5‰. The transition from high carbon isotope values to those near 0‰ in the Nash Fork Formation is similar to that at the end of the ca. 2.2–2.1 Ga carbon isotope excursion in Fennoscandia. This chemostratigraphic trend and deposition of BIFs, Mn-rich lithologies, carbonaceous shales and phosphorites at the end of the global ca. 2.2–2.1 Ga carbon isotope excursion are likely related to ocean overturn associated with the final breakup of the Kenorland supercontinent. Correlative carbonates from the Slaughterhouse Formation in the Sierra Madre, WY, and from the Whalen Group in the Rawhide Creek area in the Hartville Uplift, WY, have highly positive carbon isotope values. In contrast, carbonates from other exposures of the Whalen Group in the Hartville Uplift and all carbonate units in the Black Hills, SD, have carbon isotope values close to 0‰. Combined with existing geochronologic and stratigraphic constraints, these data suggest that the Slaughterhouse Formation and the succession exposed in the Rawhide Creek area of the Hartville Uplift are correlative with the lower and middle Nash Fork Formation and were deposited during the ca. 2.2–2.1 Ga carbon isotope excursion. The Estes and Roberts Draw formations in the Black Hills and carbonates from other exposures in the Hartville Uplift postdate the ca. 2.2–2.1 Ga positive carbon isotope excursion and are most likely correlative with the upper Nash Fork Formation. The passive margin, on which the carbonates with highly positive carbon isotope values were deposited, extended around the southern flank of the Wyoming Craton through the Sierra Madre, Medicine Bow Mountains and Hartville Uplift. The presence of carbonates with carbon isotope values close to 0‰ in the upper Nash Fork Formation and the Whalen Group indicates that the passive margin persisted on the southern flank of the Wyoming Craton after the carbon isotope excursion. Rifting in the Black Hills, likely related to the final breakup of the Kenorland, succeeded the carbon isotope excursion, since the Estes and Roberts Draw formations, deposited during rifting and ocean opening on the eastern flank of the Wyoming Craton, postdate the carbon isotope excursion.  相似文献   

14.
华北克拉通怀安杂岩中早前寒武纪变质表壳岩具有变质程度深(麻粒岩相)、连续性差、变形及构造置换强烈等特征,地层划分及形成时代一直存在较大争议.通过详细的地质调查、岩石学及年代学研究,新厘定出新太古代桑干岩群铁英岩岩组、石榴黑云片麻岩岩组以及古元古代集宁岩群黄土窑岩组石榴高压基性麻粒岩-大理岩岩段和含石墨矽线石榴片麻岩-变粒岩-大理岩岩段4套变质表壳岩单元,并建立了相应的岩石学识别标志.新太古代变质表壳岩一般呈透镜体或带状体产出于新太古代变质深成岩中,且锆石年龄存在~2.5 Ga和~1.8 Ga两个峰值.铁英岩岩组原岩为一套基性火山岩夹磁铁石英岩建造,产出阿尔戈马型BIF铁矿,形成年龄为2 489±19 Ma;石榴黑云片麻岩岩组主体岩石为条带状石榴黑云斜长片麻岩,原岩为杂砂岩建造,物源来自新太古代TTG岩石.古元古代石榴高压基性麻粒岩-大理岩岩段原岩为一套基性火山岩夹大理岩建造,形成年龄早于~2.03 Ga;含石墨矽线石榴片麻岩-变粒岩-大理岩岩段野外呈带状构造岩片体产出,连续性较好,为一套"有层无序"的孔兹岩组合,碎屑锆石年龄介于2.30~1.99 Ga,与区域上孔兹岩年龄结构一致,形成时代为古元古代晚期(1.99~1.95 Ga).新太古代和古元古代变质表壳岩均卷入古元古代末期的造山过程(1.95~1.80 Ga),遭受麻粒岩相变质与变形作用.区内孔兹岩可能是造山过程卷入的构造岩片.本研究进一步明确了晋冀蒙交界地区存在与孔兹岩不同的新太古代陆源碎屑岩和古元古代洋壳残片,这对重新认识本区早前寒武纪地质演化具有重要意义.   相似文献   

15.
Located in the middle segment of the Trans-North China Orogen, the Fuping Complex is considered as a critical area in understanding the evolution history of the North China Craton (NCC). The complex is composed of various high-grade and multiply deformed rocks, including gray gneiss, basic granulite, amphibolite, fine-grained gneiss and marble, metamorphosed to upper amphibolite or granulite facies. It can be divided into four rock units: the Fuping TTG gneisses, Longquanguan augen gneisses, Wanzi supracrustals, and Nanying granitic gneisses. U-Pb age and Hf isotope compositions of about 200 detrital zircons from the Wanzi supracrustals of the Fuping Complex have been analyzed. The data on metamorphic zircon rims give ages of 1.82-1.84 Ga, corresponding to the final amalgamation event of the NCC, whereas the data for igneous zircon cores yield two age populations at -2.10 and -2.51 Ga, with some inherited ages scattering between 2.5 and 2.9 Ga. These results suggest that the Wanzi supracrustals were derived from the Fuping TTG gneisses (-2.5 Ga) and the Nanying granitic gneisses (2.0-2.1 Ga) and deposited between 2.10 and 1.84 Ga. All zircons with -2.51 Ga age have positive initial εHf values from +1.4 to +10.9, suggesting an important crustal growth event at -2.5 Ga through the addition of juvenile materials from the mantle. The Hf isotope data for the detrital zircons further imply that the 2.8 Ga rocks are important components in the lower crust, which is consistent with a suggestion from Nd isotope data for the Eastern Block. The zircons of 2.10 Ga population have initial εHf values of-4.9 to +6.1, interpreted as mixing of crustal re-melt with minor juvenile material contribution at 2.1 Ga. These results are distinct from that for the Western Block, supporting that the Fuping Complex was emplaced in a tectonic active environment at the western margin of the Eastern Block.  相似文献   

16.
Studies of gneisses from the Yenisei regional shear zone (YRSZ) provide the first evidence for Mesoproterozoic tectonic events in the geologic history of the South Yenisei Ridge and allowed the recognition of several stages of deformation and metamorphism spanning from Late Paleoproterozoic to Vendian. The first stage (~ 1.73 Ga), corresponding to the period of granulite-amphibolite metamorphism at P = 5.9 kbar and T = 635 °C, marks the final amalgamation of the Siberian craton to the Paleo-Mesoproterozoic Nuna supercontinent. During the second stage, corresponding to a hypothesized breakup of Nuna as a result of crustal extension, these rocks underwent Mesoproterozoic dynamic metamorphism (P = 7.4 kbar and T = 660 °C) with three peaks at 1.54, 1.38, and 1.25 Ga and the formation of high-pressure blastomylonite rocks in shear zones. Late-stage deformations during the Mesoproterozoic tectonic activity in the region, related to the Grenville-age collision processes and assembly of Rodinia, took place at 1.17-1.03 Ga. The latest pulse of dynamic metamorphism (615–600 Ma) marks the final stage of the Neoproterozoic evolution of the Yenisei Ridge, which is associated with the accretion of island-arc terranes to the western margin of the Siberian craton. The overall duration of identified tectonothermal processes within the South Yenisei Ridge during the Riphean (~ 650 Ma) is correlated with the duration of geodynamic cycles in the supercontinent evolution. A similar succession and style of tectonothermal events in the history of both the southern and the northern parts of the Yenisei Ridge suggest that they evolved synchronously within a single structure over a prolonged time span (1385–600 Ma). New data on coeavl events identified on the western margin of the Siberian craton contradict the hypothesis of a mantle activity lull (from 1.75 to 0.7 Ga) on the southwestern margins of the Siberian craton during the Precambrian. The synchronous sequence and similar style of tectonic events on the periphery of the large Precambrian Laurentia, Baltica, and Siberia cratons suggest their spatial proximity over a prolonged time span (1550–600 Ma). The above conclusion is consistent with the results of modern paleomagnetic reconstructions suggesting that these cratons represented the cores of Nuna and Rodinia within the above time interval.  相似文献   

17.
赵国春 《岩石学报》2009,25(8):1772-1792
华北克拉通基底可分为三个太古宙微陆块(东部陆块、阴山陆块和鄂尔多斯陆块)和三个早元古宙活动带(孔兹岩带、华北中部带和胶-辽-吉带).这些构造单元具有不同的变质作用时间和P-T演化特征.东部陆块和阴山陆块晚太古宙基底岩系的变质作用发生在~2.5Ga,变质演化以等压冷却(IBC)逆时针P-T轨迹为特征,反映变质作用的成因与大规模地幔岩浆底侵有关.孔兹岩带主期变质作用发生在~1.95Ga,变质演化以近等温减压(ITD)顺时针P-T轨迹为特征,反映阴山陆块与鄂尔多斯陆块碰撞形成西部陆块的热构造过程.华北中部带变质作用发生在~1.85Ga,变质演化同样以近等温减压(ITD)顺时针P-T轨迹为特征,反映了西部陆块和东部陆块最终碰撞形成统一的华北克拉通基底的构造过程.早元古宙胶-辽-吉带变质作用表现‘双变质带'特征:西北带的北辽河群、老岭群和粉子山群的变质作用以中压顺时针P-T轨迹为特征,而东南带的南辽河群、吉安群和荆山群的变质作用以低压逆时针P-T演化为特征.华北克拉通基底变质作用演化地质图能更好地反映上述不同构造单元的变质作用演化特征.尽管岩浆弧、大陆裂谷和地幔柱模式都能解释东部陆块晚太古宙基底变质作用所具有的近等压冷却(IBC)逆时针P-T演化特征,地幔柱模式能够更合理解释东部陆块所存在的宽达800千米而时代近于相同的晚太古代火成岩带、大量科马提质超镁铁质岩石和双峰式火山岩、广泛发育的穹窿构造等.华北克拉通变质基底中具有石榴石-单斜辉石-斜长石-石英组合的高压基性麻粒岩和具有蓝晶石-钾长石组合的高压泥质麻粒岩的出露只局限在早元古宙华北中部带的北段和胶-辽-吉带的南端;这些高压麻粒岩形成在俯冲和陆-陆碰撞的构造环境中.西部陆块孔兹岩带含假蓝宝石麻粒岩是碰撞后(~1.92Ga)拉伸引发地幔岩浆底侵导致局部地带发生超高温(UHT)变质作用的产物.  相似文献   

18.
吕梁地区古元古代岩浆作用非常强烈,其成因与构造环境对客观恢复华北克拉通早期地质演化具有重要意义。本文选择了杜家沟长石斑岩、吕梁群近周峪组中基性火山岩和恶虎滩片麻岩进行了较系统研究。2个杜家沟长石斑岩的SHRIMP锆石U-Pb年龄分别为2189±6Ma和2186±3Ma,恶虎滩闪长质片麻岩的SHRIMP锆石U-Pb年龄为2182±5Ma。杜家沟长石斑岩为A型花岗岩,具有造山后花岗岩特征;吕梁群近周峪组中基性火山岩具有岛弧火山岩的地球化学特征;恶虎滩片麻岩也具有岛弧岩浆岩特征。综合分析华北克拉通2.2~2.0Ga的岩浆岩构造性质认为,吕梁地区岩浆性质的复杂性可能与所处的构造位置有关。古元古代吕梁地区可能位于华北克拉通古陆块边缘,其2.2~2.1Ga的岩浆岩可能经历岛弧和裂谷两种体制的共同制约。  相似文献   

19.
The geological position, composition, and age of detrital zircons of sedimentary deposits of the Nugan Formation of the Western Baikal region underlying the Golousta Formation of the Baikal series of Ediacaran age have been studied. The formation of both stratigraphic units due to the same sources of detrital material, located within the southern flank of the Siberian Craton, has been proved. The deposits of the Nugan Formation have been demonstrated to mark the rifting stage of the formation of the passive margin of the Paleo-Asiatic Ocean: their accumulation occurred in the Late Cryogenian during the interval 720–640 Ma.  相似文献   

20.
Although the presence of post-Hamersley Group mafic intrusive and extrusive rocks in the southern Hamersley province of Western Australia has been known since the area was first mapped in the early 1960s, details of the age, tectonic setting and significance of these rocks have only recently been determined, and are still controversial. These rocks are most commonly interpreted as the products of two temporally distinct periods of continental extension, separated by a hiatus of ~370 m.y. represented by the unconformity at the base of the Wyloo Group. However, the integration of published geochronological and geochemical data with detailed field observations documented in this study shows that ca 2.2 Ga dolerite sills pre- and post-date this unconformity, and were intruded during Ophthalmian orogenesis in a retroarc foreland basin. Furthermore, ca 2.2 Ga mafic magmatism is interpreted to include the Cheela Springs Basalt and is related to subduction beneath the southern Hamersley province, most likely resulting in accretion of part of the Gascoyne Province to the Pilbara Craton.  相似文献   

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