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1.
The Khetri region forms a late Palaeoproterozoic igneous–metamorphic complex in NE Rajasthan, India. Seven granitoid plutons of the Khetri complex have been studied for zircon U–Pb and Pb–Pb dating along with whole-rock and Nd–Sr isotope geochemistry to provide new constraints on the Palaeoproterozoic magmatic activity in the Aravalli orogen of northwestern India. Most intrusives show evidence of moderate to extreme albitisation forming microcline–albite granite and albite granite, respectively. The rocks are metaluminous to weakly peraluminous, largely ferroan and intraplate A-type granites. The U–Pb zircon ages for four plutons cover a time span of 1732–1682 Ma, whereas Pb–Pb zircon evaporation data for three intrusives indicate minimum emplacement ages between 1671 and 1537 Ma. The Nd–Sr isotopic systematics suggest the involvement of Neoarchaean to Palaeoproterozoic crustal components in the petrogenesis of these granitoids. A regional survey of late Palaeoproterozoic ages in the Aravalli orogen provides evidence for a geographically widespread extension-related event in the northwestern Indian shield about 1720–1700 Ma ago. The record of comparable ages and the magmatic history reported in parts of North America and the North China Craton may indicate the significance of this event for the rift tectonics of the hypothetical supercontinent Columbia.  相似文献   

2.
The Palaeoproterozoic Dabla granitoid pluton of the North Khetri Copper Belt is located to the east of a NNE-SSW trending lineament with numerous albite-rich intrusives, the intraplate ‘albitite line’. The Dabla pluton is essentially made up of calcic amphibole-bearing granitoids, displaying a concentric bimodal distribution of alkali-feldspar granites, comprising a microcline-albite granite and an albite-granite. The dominant rock type is pink-coloured granite, which is characterised by quartz, microcline, albite and hastingsitic hornblende, and occurs in the marginal parts of the pluton. The volumetrically subordinate albite-granite in the central part of the pluton is invariably white in colour, non-foliated and is mainly composed of quartz, albite and amphibole of actinolite to ferro-actinolite composition. The albite-granite is characterised by low K2O (0.06-0.09%), Rb (<5 ppm) and Ba (<20 ppm), high Na2O (7.19-7.36%) and high Na/K ratios (122.4-185.2) as compared to the granite. These rocks are not subjected to any metamorphic overprint, especially the albite-granite, which shows pristine abundances of major and trace elements. The rocks are highly evolved as reflected in their high SiO2 (72 to 78%) contents and high DI (89.5-97) values. The Dabla granitoids are characterised by similar REE and spider patterns, displaying LREE enriched slopes, flat HREE profiles and strong negative Sr, P, Ti and Eu anomalies suggesting their comagmatic nature. Nevertheless, the granite is relatively more fractionated [(La/Yb)N = 3.89-8.19] and show higher REE abundances (466-673 ppm) as compared to the albite-granite [(La/Yb)N = 1.97-2.96; REE = 220-277 ppm]. Distinctive features of these rocks are their low Ca (0.21-1.53%), Mg (<0.02-0.19%), Al (11.84-12.96%) and Sr (12-46 ppm) abundances, high Zr (155-631 ppm), Y (67-156 ppm), Nb (14-91 ppm), and Ga (20-31 ppm) concentrations and high Fe*-number, high Ga/Al ratio and high agpaitic index (AI) values. These features, coupled with their ferroan, alkaline and metaluminous nature, are typical of within-plate aluminous A-type granites. The geochemical data further indicate that the Dabla magma was generated at fairly high temperature, apparently in an upper mantle region, under relatively low H2O activities and reduced conditions and emplaced at a shallow depth in an extensional tectonic environment.  相似文献   

3.
Dirk Küster  Ulrich Harms 《Lithos》1998,45(1-4):177-195
Potassic metaluminous granitoids with enrichments of HFS elements constitute part of widespread post-collisional magmatism related to the Late Neoproterozoic Pan-African orogeny in northeastern Africa (Sudan, Ethiopia, Somalia) and Madagascar. The plutons were emplaced between 580 and 470 Ma and comprise both subsolvus and hypersolvus biotite–granite, biotite–hornblende–granite, quartz–monzonite and quartz–syenite. Pyroxene-bearing granitoids are subordinate. Basic dikes and enclaves of monzodioritic composition are locally associated with the granitoid plutons. Granitoids emplaced in pre-Neoproterozoic crust have Sri-ratios between 0.7060 and 0.7236 and Nd(t) values between −15.8 and −5.6 while those emplaced in, or close to the contact with, juvenile Neoproterozoic crust have lower Sri-ratios (0.7036–0.7075) and positive Nd(t) values (4.6). However, it is unlikely that the potassic granitoids represent products of crustal melting alone. The association with basic magmas derived from subduction-modified enriched mantle sources strongly suggests that the granitoids represent hybrid magmas produced by interaction and mixing of mantle and crust derived melts in the lower crust. The most intense period of this potassic granitoid magmatism occurred between 585 and 540 Ma, largely coeval with HT granulite facies metamorphism in Madagascar and with amphibolite facies retrogression in northeastern Africa (Somalia, Sudan). Granitoid magmatism and high-grade metamorphism are probably both related to post-collisional lithospheric thinning, magmatic underplating and crustal relaxation. However, the emplacement of potassic granites continued until about 470 Ma and implies several magmatic pulses associated with different phases of crustal uplift and cooling. The potassic metaluminous granites are temporally and spatially associated with post-collisional high-K calc-alkaline granites with which they share many petrographical, geochemical and isotopical similarities, except the incompatible element enrichments. The resemblance indicates a strongly related petrogenesis of both granite associations.  相似文献   

4.
辽东半岛中生代花岗质岩浆作用的年代学格架   总被引:51,自引:4,他引:47  
辽东半岛是我国东部中生代花岗质岩石较为发育的地区。传统观点认为,该区花岗岩以三叠-早中侏罗世(印支-早燕山期)为主。采用SHRIMP、TIMS和LA—ICPMS三种方法,对60余个样品中的锆石进行了U—Pb同位素年代学测定。根据这些资料,目前可以将该区中生代花岗质岩浆作用划分为3个阶段:三叠纪(233~212Ma)、侏罗纪(180~156Ma)和早白垩世(131~117Ma)。与以前认识不同的是,区内的花岗质岩石以早白垩世为主。对比华北地台其它地区中生代岩浆作用的年代学格架发现,三叠纪一侏罗纪花岗岩主要出现在华北东部,而早白垩世花岗岩在全区均较发育,这一分布特征为探讨华北中生代地质演化提供了重要信息。  相似文献   

5.
The Sahara–Umm Adawi pluton is a Late Neoproterozoic postcollisional A-type granitoid pluton in Sinai segment of the Arabian–Nubian Shield that was emplaced within voluminous calc-alkaline I-type granite host rocks during the waning stages of the Pan-African orogeny and termination of a tectonomagmatic compressive cycle. The western part of the pluton is downthrown by clysmic faults and buried beneath the Suez rift valley sedimentary fill, while the exposed part is dissected by later Tertiary basaltic dykes and crosscut along with its host rocks by a series of NNE-trending faults. This A-type granite pluton is made up wholly of hypersolvus alkali feldspar granite and is composed of perthite, quartz, alkali amphibole, plagioclase, Fe-rich red biotite, accessory zircon, apatite, and allanite. The pluton rocks are highly evolved ferroan, alkaline, and peralkaline to mildly peraluminous A-type granites, displaying the typical geochemical characteristics of A-type granites with high SiO2, Na2O + K2O, FeO*/MgO, Ga/Al, Zr, Nb, Ga, Y, Ce, and rare earth elements (REE) and low CaO, MgO, Ba, and Sr. Their trace and REE characteristics along with the use of various discrimination schemes revealed their correspondence to magmas derived from crustal sources that has gone through a continent–continent collision (postorogenic or postcollisional), with minor contribution from mantle source similar to ocean island basalt. The assumption of crustal source derivation and postcollisional setting is substantiated by highly evolved nature of this pluton and the absence of any syenitic or more primitive coeval mafic rocks in association with it. The slight mantle signature in the source material of these A-type granites is owed to the juvenile Pan-African Arabian–Nubian Shield (ANS) crust (I-type calc-alkaline) which was acted as a source by partial melting of its rocks and which itself of presumably large mantle source. The extremely high Rb/Sr ratios combined with the obvious Sr, Ba, P, Ti, and Eu depletions clearly indicate that these A-type granites were highly evolved and require advanced fractional crystallization in upper crustal conditions. Crystallization temperature values inferred average around 929°C which is in consistency with the presumably high temperatures of A-type magmas, whereas the estimated depth of emplacement ranges between 20 and 30 km (upper-middle crustal levels within the 40 km relatively thick ANS crust). The geochronologically preceding Pan-African calc-alkaline I-type continental arc granitoids (the Egyptian old and younger granites) associated with these rocks are thought to be the crustal source of f this A-type granite pluton and others in the Arabian–Nubian Shield by partial melting caused by crustal thickening due to continental collision at termination of the compressive orogeny in the Arabian–Nubian Shield.  相似文献   

6.
Summary The Precambrian rocks in western Ethiopia consist of high- and low-grade terranes intruded by granitoids with a wide compositional spectrum. The formation ages of these granitoid rocks are, so far, poorly understood. Single-grain zircon Pb/Pb evaporation and conventional U/Pb dating conducted on four granitoids places time constraints on their emplacement and tectonothermal events. Three granitoid magmatic events were identified at 815 Ma, 700–730 Ma, and 620–625 Ma, which were marked by emplacement of the calc-alkaline Ujjukka granite and granodiorite, the anatectic Suqii-Wagga two-mica granite and the Guttin K-feldspar megacrystic granite, and the anorogenic Ganjii monzogranite, respectively. We interpret the 815 Ma age to mark a major magmatic episode in this part of Africa. A tectonothermal event at ∼ 630 Ma preceded the emplacement of the within-plate granitoids at 620–625 Ma. The decrease of ages from the calc-alkaline to anorogenic granitoids suggests a shift of magmatic styles and tectonic setting of the granitoids over a period of 200 million years. The Suqii-Wagga and Guttin granites, representing the granitoid population in the migmatitic terrane, formed as part of the successive evolution of the granitoid magmatism in the region. The presence of xenocrystic zircons of Mesoproterozoic ages in both granitoid populations emplaced into the low-grade volcanosedimentary sequence and the high-grade, often migmatitic, gneisses suggest contribution of pre-Pan-African crust to the origin and evolution of the granitoids. Conventional U/Pb studies of zircons from the Guttin K-feldspar megacrystic granite and the Ganjii monzogranite yielded upper intercept ages of ∼ 3 Ga and ∼ 2 Ga, respectively, possibly indicating the presence of reworked Archean-Proterozoic crustal material.
Zusammenfassung U/Pb und Pb/Pb Zirkonalter granitoider Gesteine aus dem Gebiet von Wallagga: Hinweise zur magmatischen und tektonischen Entwicklung pr?kambrischer Gesteine in A¨thiopien Das Pr?kambrium im westlichen ?thiopien besteht aus hoch- und niedrigmetamorphen Basement Serien, die von Granitoiden unterschiedlichster Zusammensetzung intrudiert werden. Die Bildungsalter dieser Magmatite sind bisher nur ungenügend bekannt gewesen. Neue Pb/Pb-Evaporations- und konventionelle U/Pb-Datierungen an Einzelzirkonen von vier verschiedenen Plutoniten erlauben nun Rückschlüsse auf deren Intrusionsalter und die damit verbundene tektonische Entwicklung der Region. Drei zeitlich getrennte magmatische Ereignisse lassen sich unterscheiden: Intrusion der kalk-alkalischen Ujjukka Granite um 815 Ma; Bildung der anatektischen Zweiglimmer Granite der Suqii-Wagga Suite um 700–730 Ma; Intrusion der grob porphyrischen K-Feldspat Granite von Guttin und der anorogenen Ganjii Monzogranite um 620–625 Ma. Das 815 Ma Ereignis wird als wichtige magmatische Phase in diesem Teil von Afrika interpretiert. Ein thermisches Ereignis um 630 Ma geht der Platzname von “within-plate” Granitoiden um 620–625 Ma voraus. Die beobachtete Altersabnahme von den kalk-alkalischen zu den anorogenen Granitoiden spricht für eine pr?gnante ?nderung des tektonischen Regimes über einen Zeitraum von ca. 200 Ma. Die Suquii-Wagga und Guttin Granite sind in das hochgradige, migmatische Basement intrudiert. Dies mag für eine sukzessive tektonische Entwicklung dieser Abfolgen sprechen. Ererbte, mesoproterozoische Zirkone deuten auf die Aufarbeitung pr?-panafrikanischer Gesteine hin. Obere Einstichpunkte von den U/Pb Analysen im Altersbereich von ca. 3 Ga in den Guttin Graniten und von ca. 2 Ga in den Ganjii Monzograniten sprechen ebenfalls für die Inkorporation von proterozoischen bis archaischen Krustenkomponenten.


Received June 7, 2000; accepted October 29, 2000  相似文献   

7.
Three stages of Early Proterozoic granitoid magmatism were distinguished in the southwestern margin of the Siberian craton: (1) syncollisional, including the formation of migmatites and granites in the border zone of the Tarak massif; (2) postorogenic, postcollisional, comprising numerous granitoid plutons of diverse composition; and (3) intraplate, corresponding to the development of potassic granitoids in the Podporog massif. Rocks of three petrological and geochemical types (S, I, and A) were found in the granitoid massifs. The S-type granites are characterized by the presence of aluminous minerals (garnet and cordierite), and their trace element distribution patterns and Nd isotopic parameters are similar to those of the country paragneisses and migmatites. Their formation was related to melting under varying H2O activity of aluminous and garnet—biotite gneisses at P ≥ 5 kbar and T < 850°C with a variable degree of melt separation from the residual phases. The I-type tonalites and dioritoids show low relative iron content, high concentrations of CaO and Sr, fractionated REE distribution patterns with (La/Yb)n = 11–42, and variable depletion of heavy REE. Their parental melts were derived at T ≥ 850°C and P > 10 and P < 10 kbar, respectively. According to isotopic data, their formation was related to melting of a Late Archean crustal (tonalite-diorite-gneiss) source with a contribution of juvenile material ranging from 25–55% (tonalites of the Podporog massif) to 50–70% (dioritoids of the Uda pluton). The most common A-type granitoids show high relative iron content; high concentration of high-field-strength elements, Th, and light and heavy REE; and a distinct negative Eu anomaly. Their primary melts were derived at low H2O activity and T ≥ 950°C. The Nd isotopic composition of the granitoids suggests contributions to the magma formation processes from ancient (Early and Late Archean) crustal (tonalite-diorite-gneiss) sources and a juvenile mantle material. The contribution of the latter increases from 0–35% in the granites of the Podporog and Tarak massifs to 40–50% for the rocks of the Uda and Shumikha plutons. The main factors responsible for the diversity of petrological and geochemical types of granitoids in collisional environments are the existence of various fertile sources in the section of the thickened crust of the collisional orogen, variations in magma generation conditions $(\alpha _{H_2 O} , T, and P)$ during sequential stages of granite formation, and the varying fraction of juvenile mantle material in the source region of granitoid melts.  相似文献   

8.
《Chemical Geology》2007,236(1-2):112-133
The Cida A-type granitic stock (∼ 4 km2) and Ailanghe I-type granite batholith (∼ 100 km2) in the Pan-Xi (Panzhihua-Xichang) area, SW China, are two important examples of granites formed during an episode of magmatism associated with the Permian Emeishan mantle plume activity. This is a classic setting of plume-related, anorogenic magmatism exhibiting the typical association of mantle-derived mafic and alkaline rocks along with silicic units. SHRIMP zircon U–Pb data reveal that the Cida granitic pluton (261 ± 4 Ma) was emplaced shortly before the Ailanghe granites (251 ± 6 Ma). The Cida granitoids display mineralogical and geochemical characteristics of A-type granites including high FeO/MgO ratios, elevated high-field-strength elements (HFSE) contents and high Ga/Al ratios, which are much higher than those of the Ailanghe granites. All the granitic rocks show significant negative Eu anomalies and demonstrate the characteristic negative anomalies in Ba, Sr, and Ti in the spidergrams. It can be concluded that the Cida granitic rocks are highly fractionated A-type granitoids whereas the Ailanghe granitic rocks belong to highly evolved I-type granites.The Cida granitoids and enclaves have Nd and Sr isotopic initial ratios (εNd(t) =  0.25 to + 1.35 and (87Sr/86Sr)i = 0.7023 to 0.7053) close to those of the associated mafic intrusions and Emeishan basalts, indicating the involvement of a major mantle plume component. The Ailanghe granites exhibit prominent negative Nb and Ta anomalies and weakly positive Pb anomalies in the spidergram and have nonradiogenic εNd(t) ratios (− 6.34 to − 6.26) and high (87Sr/86Sr)i values (0.7102 to 0.7111), which indicate a significant contribution from crustal material. These observations combined with geochemical modeling suggest that the Cida A-type granitoids were produced by extensive fractional crystallization from basaltic parental magmas. In contrast, the Ailanghe I-type granites most probably originated by partial melting of the mid-upper crustal, metasedimentary–metavolcanic rocks from the Paleo-Mesoproterozoic Huili group and newly underplated basaltic rocks.In the present study, it is proposed that petrogenetic distinctions between A-type and I-type granites may not be as clear-cut as previously supposed, and that many compositional and genetically different granites of the A- and I-types can be produced in the plume-related setting. Their ultimate nature depends more importantly on the type and proportion of mantle and crustal material involved and melting conditions. Significant melt production and possible underplating and/or intrusion into the lower crust, may play an important role in generating the juvenile mafic lower crust (average 20 km) in the central part of the Emeishan mantle plume.  相似文献   

9.
南秦岭勉略带北光头山花岗岩体群的成因及其构造意义   总被引:31,自引:15,他引:31  
南秦岭勉略带北部花岗岩体从闪长岩到花岗闪长岩和花岗岩变化,反映了钙碱性岩岩石组合特征,矿物组成以长石、石英、黑云母和少量角闪石为主,副矿物有锆石、磷灰石、磁铁矿和榍石,岩石化学上它们相对高K、Sr,Zr/Y比值较高,富集LEE和LILE,贫化HFSE,与后碰撞富钾钙碱性I型花岗岩特征一致。此外,它们明显亏损Nb、Ta,低Y、Yb和有较高的 LaN/YbN和Sr/Y比值,多数岩体发育淬冷岩浆结构的暗色闪长质微粒包体,包体与寄主花岗岩的稀土及微量元素存在明显差异,证明它们是地壳增厚背景下,可能由下部地壳拆沉作用导致的分别来自幔源和下部地壳熔融的二元岩浆混合演化的产物。个别高分异岩体的Fetot/Mg比值高、明显亏损Sr、Ba、Ti、P,呈现了向强分异A型花岗岩过渡的后碰撞富钾过铝偏碱性花岗岩特征。因此,结合西部岩体形成年代早于东部岩体分析,西部形成时代较早偏中基性的含有大量闪长质微粒包体的岩体代表了早期下部地壳拆沉作用的发生,东部形成较晚分异程度高的高钾钙碱性Ⅰ型花岗岩体的出现指示了南、北两大陆块碰撞汇聚后向伸展的转折,而更晚期高度分异的姜家坪富钾花岗岩体的出现则表明秦岭造山带已进入主碰撞结束期的伸展拉张演化阶段,并预示了新的板内演化期的到来。  相似文献   

10.
Summary Three distinctive metaluminous granitic suites have been identified from the Pan-African belt of the Kab Amiri area, Eastern Desert, Egypt. These are: 1) a trondhjemite-tonalite suite, 2) a calc-alkaline granodiorite suite, and 3) an alkali leucogranite suite. The trondhjemite-tonalite and the granodiorite suites resemble I-type granitoids whereas the alkali leucogranites display A-type characteristics. Geochemical attributes and field aspects indicate that three independent magmas, at different tectonic stages of the Pan-African crustal growth, are required to explain the origin of these granitoid suites. Rocks of the trondhjemite-tonalite suite correspond to granites of the arc stage and possess a narrow range of SiO2 with low K2O, Sr, Rb, Ba, Nb and Zr. Its composition is consistent with 20–30% partial melting of a primitive low-K tholeiitic source, similar to the early formed tholeiitic metavolcanics of the Egyptian basement. The granodiorite suite belongs to the collision stage and displays higher K2O, Rb, Ba, and Sr. Its magma was derived by 30–40% partial melting of LILE-enriched mafic island arc crust. The presence of abundant microdiorite enclaves in the trondhjemite-tonalite and the granodiorite suites suggests that mantle-derived mafic magma played an important role in their petrogenesis, acting as a heat source for melting via underplating and/or intrusion. The A-type leucogranites are post-collision highly fractionated granites. They exhibit low Al2O3, MgO, CaO, TiO2, Sr, and Ba and high Rb, Nb, Y. The wide chemical variations within this suite are consistent with its evolution by fractional crystallization of plagioclase, K-feldspar, amphibole, Fe–Ti oxides, and apatite from a mafic magma. The parent magma was originated in the upper mantle due to crustal attenuation associated with extension in the late stage of the Pan-African crustal evolution. Received September 13, 2000; revised version accepted May 4, 2001  相似文献   

11.
The southern Sinai Peninsula, underlain by the northernmost extension of the Arabian-Nubian Shield, exposes post-collisional calc-alkaline and alkaline granites that represent the youngest phase of late Neoproterozoic igneous activity. We report a petrographic, mineralogical and geochemical investigation of post-collisional plutons of alkaline and, in some cases, peralkaline granite. These granites intrude metamorphosed country rocks as well as syn- and post-collisional calc-alkaline granitoids. The alkaline and peralkaline granites of the southern tip of Sinai divide into three subgroups: syenogranite, alkali feldspar granite and riebeckite granite. The rocks of these subgroups essentially consist of alkali feldspar and quartz with variable amounts of plagioclase and mafic minerals. The syenogranite and alkali feldspar granite contain small amounts of calcic amphibole and biotite, often less than 3%, while the riebeckite granite is distinguished by sodic amphibole (5–10%). These plutons have geochemical signatures typical of post-collisional A-type granites and were most likely emplaced during a transition between orogenic and anorogenic settings. The parental mafic magma may be linked to lithospheric delamination and upwelling of asthenospheric mantle material. Differentiation of the underplated basaltic magma with contributions from the juvenile crust eventually yielded the post-collisional alkaline granites. Petrogenetic modelling of the studied granitic suite shows that pure fractional crystallization cannot quantitatively explain chemical variations with the observed suite, with both major oxides and several trace elements displaying trends opposite to those required by the equilibrium phase assemblage. Instead, we show that compositional variation from syenogranite through alkali feldspar granite to riebeckite granite is dominated by mixing between a low-SiO2 liquid as primitive or more primitive than the lowest-SiO2 syenogranite and an evolved, high-SiO2 liquid that might be a high-degree partial melt of lower crust.  相似文献   

12.
在岩石学研究的基础上,运用LA-ICP-MS锆石U-Pb定年和地球化学方法,研究了阿尔山地区不同时代花岗岩体的成因和构造意义。研究表明,三广山中粒碱长花岗岩形成于印支期(228.5±3.0Ma);南兴安似斑状碱长花岗岩形成于燕山期(141.7±2.6Ma),捕获锆石年龄为1847±21Ma,反映该区可能具有前寒武纪结晶基底。两岩体岩石化学以富Si、高K、低Mg、贫Ca为特点,A/CNK值为1.00~1.05;富集高场强元素和轻稀土元素,亏损重稀土元素和大离子亲石元素,稀土元素配分模式为典型的右倾海鸥型。岩相学和地球化学特征显示,三广山和南兴安花岗岩均为A型花岗岩。其中,三广山花岗岩为A2型花岗岩,南兴安花岗岩为A1型花岗岩。全岩Sr-Nd同位素组成(εNd(t)值为2.26~5.58)表明,阿尔山地区花岗岩的源区可能为显生宙-新元古代期间从亏损地幔中新增生的地壳物质,但南兴安和三广山2个岩体的形成机制不同。三广山A2型花岗岩可能是古亚洲洋在三叠纪闭合后进入造山后阶段岩石圈伸展体制下的产物,而南兴安A1型花岗岩可能形成于早白垩世大兴安岭地区板内伸展作用下的拉张减薄环境。  相似文献   

13.
The Sangan mining region, which has a proven reserve of approximately 1000 Mt of 53% iron ore, is located in the Khaf-Kashmar-Bardeskan volcano-plutonic belt in northeastern Iran. The geological units in the eastern zone of the Sangan region consist of Precambrian schists, Jurassic sedimentary rocks and Tertiary subvolcanic granitoid intrusions. Iron skarn mineralization consists of stratiform and massive bodies in the carbonate rocks that are adjacent to the granitoid intrusions. Detailed field mapping revealed that 39-Ma syenitic intrusive bodies in the western and central zones of the Sangan region were the main sources of heat and fluid for the iron mineralization.A Mid-Cenozoic biotite granite pluton is associated with the eastern anomalies. However, field relationships suggested that this pluton is not the source of the metals, heat or fluids that were responsible for the iron mineralization. This pluton is rich in silica (SiO2 contents from 66.4 to 79.1 wt%) and is characterized by high-K series with metaluminous to slightly peraluminous affinity.Geochronological (U-Pb zircon method) and geochemical data, including major and trace elements and Sr-Nd-Pb isotopes, define the complex origin of these plutons, which consist of alkaline granitoids that appear to be A-type in character but also show I-type affinity.New geochemical and isotopic data from plutons in the eastern anomalies and data from previous studies of the western and central anomalies and the southeastern intrusive rocks in the Sangan region show that these plutons have close affiliation with lower to upper crust-derived melts and were largely modified into highly fractionated I-type granite. These rocks were derived from and emplaced by varying degrees of partial melting during the Middle Eocene (Bartonian to Lutetian, 38.3–43.9 Ma) from a crustal protolith in a normal to mature volcanic continental arc setting.The Sangan granitoids were produced from crustal assimilation by a heat source from mantle melts, which are associated with the Kashmar-Neotethyan slab that subducted under Eurasia. The Khaf-Kashmar-Bardeskan igneous rocks reflect an active Cenozoic plate margin that was related to the closure of the Kashmar-Neotethyan Sea between the Lut and Eurasia blocks because of the continuous convergence between the Arabian and Iran plates during the Late Cretaceous–Early Paleocene.  相似文献   

14.
In North Xinjiang there is an alkali granite belt extending in the NW-SE direction along the southern band of the Ulungur River and running parallel to the suture zone,i.e.,Aermantai-Zhaheba Ophiolitic Melange Zone ,between the Junggar Plate and the Altay Orogenic Belt.Whole -rock Rb-Sr isochron ages of the Ulungur alkali granites are within the range of 292-309Ma, showing that they were genetically connected with the latest episode of Hercynian magmatism subsequent to the syncollision S-type and post-collision uplifting I-type granitoids in the Altay region .The alkali granites are miner-alogically characterized by the occurrence of aegirine and arfvedsonite and chemically by high silicon and alkali,low calcium and magnesium and abundant high-field elements, being typical A-type granites .The alkali granites were formed in the final stage of the Hercynian calc-alkaline magmatic cycle in a very short period of time .They are in line with the post-orogenic A-type(PA-type)granites, implying that the tectonic regime was changed from compression to extension.  相似文献   

15.
新疆拜城县波孜果尔A型花岗岩类为富含铌、钽、锆等有用元素的含矿岩体。通过偏光显微镜、电子探针(EPMA)化学成分分析、电子探针背散射(BSE)对波孜果尔A型花岗岩类的矿物学特征进行了研究,并对岩浆形成的温度条件与构造背景进行了讨论。结果表明,波孜果尔A型花岗岩类包括霓石钠闪石英碱性长石正长岩、霓石钠闪碱性长石花岗岩、黑云母碱性长石正长岩3种岩石类型。主要造岩矿物包括石英、钠长石、钾长石、霓石、钠铁闪石和铁叶云母。副矿物包括锆石、烧绿石、钍石、萤石、独居石、氟碳铈镧矿、磷钇矿等。岩浆平均温度832~839℃,形成于非造山的板内构造环境,且具高温、无水、低氧逸度的成岩特点。  相似文献   

16.
Detailed geochemical, isotope, and geochronological studies were carried out for the granitoids of the Chuya and Kutima complexes in the Baikal marginal salient of the Siberian craton basement. The obtained results indicate that the granitoids of both complexes are confined to the same tectonic structure (Akitkan fold belt) and are of similar absolute age. U–Pb zircon dating of the Kutima granites yielded an age of 2019±16 Ma, which nearly coincides with the age of 2020±12 Ma obtained earlier for the granitoids of the Chuya complex. Despite the close ages, the granitoids of these complexes differ considerably in geochemical characteristics. The granitoids of the Chuya complex correspond in composition to calcic and calc-alkalic peraluminous trondhjemites, and the granites of the Kutima complex, to calc-alkalic and alkali-calcic peraluminous granites. The granites of the Chuya complex are similar to rocks of the tonalite–trondhjemite–granodiorite (TTG) series and are close in CaO, Sr, and Ba contents to I-type granites. The granites of the Kutima complex are similar in contents of major oxides to oxidized A-type granites. Study of the Nd isotope composition of the Chuya and Kutima granitoids showed their close positive values of εNd(T) (+ 1.9 to + 3.5), which indicates that both rocks formed from sources with a short crustal history. Based on petrogeochemical data, it has been established that the Chuya granitoids might have been formed through the melting of a metabasitic source, whereas the Kutima granites, through the melting of a crustal source of quartz–feldspathic composition. Estimation of the PT-conditions of granitoid melt crystallization shows that the Chuya granitoids formed at 735–776 °C (zircon saturation temperature) and > 10 kbar and the Kutima granites, at 819–920 °C and > 10 kbar. It is assumed that the granitoids of both complexes formed in thickened continental crust within an accretionary orogen.  相似文献   

17.
This paper reports the compositions of granitoids from the Alyarmaut Uplift in the western Chukchi Peninsula, which is interpreted as a granite-metamorphic dome. A postcollisional origin was inferred for the granitoids. Their petrographic composition, petrochemical characteristics, and the compositions of their biotite allowed us to assign them to high-K I-type granites. The trace-element composition of the granitoids is comparable with that of granite types associating with both collisional and suprasubduction settings, which may reflect magma source heterogeneity generated by previous collisional processes predating dome and granite formation. The significant scatter of ɛNd(T) and 87Sr/86Sr values in the granitoids is also indicative of the heterogeneous composition of the crustal source or variable degree of magma contamination with ancient crustal material. In addition to the dominant process of the submersion of the rim of the Chukchi microcontinent beneath the active margin of the North Asian craton, the tectonic scenario of the formation of the dome structure of the Alyarmaut Uplift should involve either slab detachment or delamination of the lithospheric mantle, which causes the invasion of asthenospheric material into the base of the crust and promotes heat transfer necessary for the derivation of granitoid magmas.  相似文献   

18.
ABSTRACT

The Xilamulun Mo belt of Northeastern China, located in the southeastern segment of the Central Asia Orogenic Belt (CAOB), is composed of large deposits of porphyry Mo and quartz-vein-type Mo, which are related to Mesozoic granitoids. Previous studies led to the conclusion that all granitoids in the region formed during the Cretaceous and Triassic, but our new laser ablation inductively coupled plasma mass spectrometry U–Pb zircon dating of magmatic zircons from five samples of four mineralized plutons (Nailingou, Longtoushan, and Hashitu granites and Erbadi and Hashitu granite porphyries) reveals that these range in age from 143.8 ± 1.2 to 149.5 ± 1.0 Ma. These granites show post-collisional (A-type) geochemical characteristics (e.g. enrichment in total alkali, LILE, and LREE and depletion in Eu, Ba, P, and Nb). The Erbadi, Longtoushan, Hashitu, and Longtoushan granitoids exhibit moderately positive Hf isotopic compositions (εHf(t) = ?0.3 to 10.2), indicating that granitic magmas may reflect mixtures of mantle melts and continental crust. These mineralized granites were all emplaced along a major fault over a time span of ~6 million years during the Late Jurassic. We conclude that igneous activity and mineralization resulted from the rollback of the subducted Palaeo-Pacific plate beneath Eurasia. Confirming that the Late Jurassic granitic intrusives are related to the Mo mineralization is useful for understanding the Mesozoic tectonic evolution of the Xilamulun Mo belt and also has significant implications for the regional exploration of ores.  相似文献   

19.
由于缺少可靠的年代学资料和系统研究,阿拉善北部亚干地区的基底时代和性质尚不清楚,制约了对本区构造属性及造山带结构的进一步认识.利用亚干地区广泛出露的花岗岩锆石U-Pb年代学和Hf同位素研究,揭示源区深部物质组成特征,对探讨该地区的基底性质具有重要意义.LA-ICP-MS锆石U-Pb分析结果表明,切刀黑云母二长花岗岩体侵位于380±1 Ma,亚东花岗闪长岩体侵位于271±2 Ma,同时,原北山群中识别出大量的三叠纪花岗岩(亚干片麻状花岗岩,228±2 Ma;都热糜棱岩化花岗岩,214±2 Ma).地球化学分析表明,切刀花岗岩和都热糜棱岩化花岗岩为准铝质-弱过铝质的A型花岗岩,亚东花岗岩为钙碱性I型花岗岩.锆石Hf同位素分析显示主要的花岗岩体εHf(t)值为-2.8~+4.3,地壳模式年龄为1.0~1.5 Ga,表明源区可能以中元古代地壳物质为主.结合前人获取的前寒武纪岩石年龄,亚干地区花岗岩Hf同位素特征,以及花岗岩出现中-新元古代继承锆石等证据,亚干地区深部应具有中-新元古代基底,南戈壁微陆块范围可以延伸到阿拉善北部边境地区.   相似文献   

20.
秦亚  梁一鸿  胡兆初  冯坚  李敏 《地球科学》2013,38(4):677-688
主微量元素分析和LA-ICP-MS锆石U-Pb年龄显示吉南老岭地区的头道、老岭、上绿水桥和高台子岩体为一套早白垩世铝质A型花岗岩.主要岩性为钾长花岗岩、晶洞钾长花岗岩、花岗斑岩和花岗岩.LA-ICP-MS锆石U-Pb年龄为121~125Ma.主量元素具有富Si、alk, 贫Fe、Mg、Ca、Ti的特征; 微量元素亏损Ba、Sr、Ti、Nb、Ta、P, 富集K、Rb、Th等不相容元素; 稀土元素具有中等到强烈的负铕异常及右倾海鸥型的球粒陨石标准化稀土配分模式.元素地球化学特征表明岩体为铝质A型花岗岩(A/CNK=0.82~1.15, A/NK=1.00~1.28).岩石具有较低的不相容元素Ce/Nb、Y/Nb、Yb/Ta比值, 为A1型非造山花岗岩.研究表明吉南老岭地区早白垩世时处于非造山的伸展构造环境, 是华北板块东部早白垩世伸展地球动力学背景在吉林南部地区的岩浆活动体现.   相似文献   

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