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1.
村前铜多金属矿床位于钦杭成矿带东段,为一具有矽卡岩型矿化和斑岩型矿化的铜多金属矿床,含矿岩体为燕山早期花岗闪长斑岩,岩石具有富硅、富铝、富碱的特点,属于偏铝-过铝质钙碱性花岗岩类。岩体具有从深部向浅部蚀变增强,大部分组分活动性不明显,而成矿元素Cu-Mo-Fe-Pb-Zn-Au-Ag含量明显增加,Na2O、Sr含量降低,REE元素除Eu少量丢失外,其余均呈一致的迁入特征。岩体属Ⅰ型花岗质岩石,由具角闪石+石榴子石残留相的火成岩部分熔融形成的熔浆,混合或混染了地壳重熔型岩浆上侵就位而成。钦杭结合带东段,燕山期中酸性岩浆活动具有从176~150Ma的埃达克岩或具岛弧花岗岩特征的Ⅰ型花岗岩,至150~140Ma的S型花岗岩,向140~110Ma的A型花岗岩演化趋势,显示了地壳由厚减薄的过程,暗示其大地构造背景为岩石圈的伸展减薄环境,而形成于169.3±1.1Ma的村前斑岩体正处于伸展阶段早期。综合岩体成矿特征表明,钦杭成矿带东段及邻近地区,176~160Ma主要形成与Ⅰ型花岗质岩石有关的以Cu为主的多金属矿床;160~150Ma主要形成与Ⅰ型花岗质岩石有关的Cu-Mo矿床与W-Sn矿床;150~140Ma主要形成与S型花岗质岩石有关的以W-Sn-Mo为主的多金属矿床,以及以Ag-Pb-Zn为主的多金属矿床;140~110Ma主要形成与A型花岗质岩石有关的以W-Sn-Mo为主的多金属矿床,少量与Ⅰ型花岗质岩石有关的Pb-Zn矿床。 相似文献
2.
David Orejana Carlos Villaseca Pablo Valverde-Vaquero Elena A. Belousova Richard A. Armstrong 《International Journal of Earth Sciences》2012,101(7):1789-1815
The Spanish Central System (SCS) batholith, located in the Central Iberian Zone, is one of the largest masses of granite in the European Variscan Belt. This batholith is a composite unit of late- and post-kinematic granitoids dominated by S- and I-type series granite, with subordinate leucogranite and granodiorite. Zircon trace element contents, from two representative S-type and three I-type granitoids from the eastern portion of the SCS batholith, indicate a heterogeneous composition due to magma differentiation and co-crystallisation of other trace element-rich accessory phases. In situ, U–Pb dating of these zircons by SHRIMP and LA-ICP-MS shows 479–462-Ma inherited zircon ages in the I-type intrusions, indicating the involvement of an Ordovician metaigneous protolith, while the S-type intrusions exclusively contain Cadomian and older zircon ages. The zircon crystallisation ages show that these granites have been emplaced at ca. 300?Ma with a time span between 303?±?3?Ma and 298?±?3?Ma. Precise dating by CA-ID-TIMS reveals a pulse at 305.7?±?0.4?Ma and confirms the major pulse at 300.7?±?0.6?Ma. These ages match the Permo-Carboniferous age for granulite-facies metamorphism of the lower crust under the SCS batholith and coincide with a widespread granitic event throughout the Southern Variscides. Ti-in zircon thermometry indicates temperatures between 844 and 784°C for both the S- and I-type granites, reinforcing the hypothesis that these granites are derived from deep crustal sources. 相似文献
3.
B.L. Narayana J. Mallikharjuna Rao M.V. Subba Rao N.N. Murthy V. Divakara Rao 《Gondwana Research》2000,3(4):507-520
Early Proterozoic Dongargarh granite complex of Central India, intruding the tonalitic to granodioritic Amgaon gneisses and the Nandgaon Group bimodal volcanic suite, comprises three different textural and compositional types, viz., porphyritic granodiorite (PG), coarse equigranular granite (EG) and microgranite (MG). Synplutonic mafic dykes are common in the granite complex. The PG is characterised by rapakivi texture and the EG is the dominant facies and exhibits sporadically developed rapakivi texture. Microgranular enclaves are common in the EG while they are rare in PG. Major and trace element geochemistry of PG shows marked I- type and some occasional A-type granite characters unusual for a rapakivi granite while the EG shows A-type granite signatures. The field, petrographic, chemical and isotopic data of these granites suggest their derivation by mixing of mantle derived basic magma with a crustal-derived partly crystalline granitic magma. Episodic mafic magma underplating caused the anatexis of the Archaean lower continental crust in a continental margin tectonic setting resulting first in the formation of the I-type granodiorite followed by A-type granite. The I-type granodiorite is mixed with the basic magma (synplutonic dykes) while the EG is formed by mingling of A- type granite magma and the intruding basic magma. 相似文献
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5.
The country rock in southern Finland formed mainly during the Svecofennian orogeny ca. 1.9 Ga ago. The middle and lower crust was partially melted 1.83 Ga ago due to crustal thickening and subsequent extension. During this event, S-type migmatites and granites were formed along a 100×500 km zone. This Late Svecofennian Granite–Migmatite zone (LSGM zone) is a large crustal segment characterised by roughly E–W trending sub-horizontal migmatites and granites. Combined ductile E–W shear movements and NNW–SSE compressional movements defined a transpressional tectonic regime during the emplacement. Partial melts that moved through the crust pooled as granite sheets or froze as migmatites. Major transpressive shear zones border the LSGM zone, which forms a tectonic and metamorphic zone that crosscuts the earlier Svecofennian granitoids. Based on field observations and geochemical data from two sets of outcrops, we show that the great volumes of late-orogenic granites and migmatites in southern Finland were transported and emplaced as small chemically variable batches, possibly extracted from different protoliths. These melt batches were transported along repeatedly activated channels and collected at some horizontal level in the crust. In the Nagu area, the melt batches were trapped under a roof-layer of amphibolite and the whole complex was synchronously folded into open folds with steep axial surfaces and E–W trending fold axes. The sheets of microcline granite are, in places, strongly sheared; the microcline phenocrysts are imbricated and subsequent deformation of the microcline phenocrysts indicates syn-tectonic movements of the layers as well as a syn-tectonic mechanism for the late-magmatic fractionation. Depending on the degree of crystallisation of the individual melt batches during shearing at different intensities, the granites have slightly different appearances. Some sheared zones show a cumulate-like trace element geochemistry, indicating that melt fractions were expelled from the system, producing layers of deformation enhanced fractionated granites and cumulate layers. Our interpretation is that the Nagu area shows shear-assisted fractionation mechanisms in granitic melts, and that similar processes are responsible for the fractionation trends seen in the sub-horizontal sheeted granites in Hämeenlinna at higher levels in the crust. 相似文献
6.
北山花岗岩S型/I型空间变化规律及含矿性 总被引：3，自引：0，他引：3
北山地区花岗岩十分发育, 出露面积接近总面积的30%, 形成时代以华力西期为主, 约占80%以上。笔者根据岩石化学判别统计, 本区花岗岩的S型/I型个数比例, 北带0.33, 中带0.54, 南带0.59, 说明从北向南, I型花岗岩逐渐减少, S型花岗岩逐渐增多。区内花岗岩类为重要的含矿岩石, 其中典型斑岩铜矿床与I型花岗质斑岩有关, 当出现铜铅组合时则与S型花岗质斑岩有关; 钼矿床有关花岗岩一般属I型, 当出现钨钼组合时则向S型花岗岩过渡; 钨锡矿床主要与S型花岗岩有关; 金矿床有关的花岗岩既有I型, 也有S型, 专属性不明显。 相似文献
7.
Robert Bolhar Uwe Ring Charlotte M. Allen 《Contributions to Mineralogy and Petrology》2010,160(5):719-742
We use 369 individual U–Pb zircon ages from 14 granitoid samples collected on five islands in the Cyclades in the Aegean Sea,
Greece, for constraining the crystallisation history of I- and S-type plutons above the retreating Hellenic subduction zone.
Miocene magmatism in the Cyclades extended over a time span from 17 to 11 Ma. The ages for S-type granites are systematically
~2 million years older than those for I-type granites. Considering plutons individually, the zircon data define age spectra
ranging from simple and unimodal to complex and multimodal. Seven of the 14 investigated samples yield more than one distinct
zircon crystallisation age, with one I-type granodiorite sample from Mykonos Island representing the most complex case with
three resolvable age peaks. Two samples from S-type granites on Ikaria appear to have crystallised zircon over 2–3 million
years, whereas for the majority of individual samples with multiple zircon age populations the calculated ages deviate by
1–1.5 million years. We interpret our age data to reflect a protracted history involving initial partial melting at deeper
lithospheric levels, followed by crystallisation and cooling at shallower crustal levels. Our study corroborates published
research arguing that pluton construction is due to incremental emplacement of multiple magma pulses over a few million years.
Assuming that multiple age peaks of our 14 samples can indeed serve to quantify time spans for magmatic emplacement, our data
suggest that Aegean plutons were constructed over a few million years. Our tectonic interpretation of the U–Pb ages is that
the S-type granites resulted from partial melting and migmatisation of the lower crust, possibly starting at ~23 Ma. The I-type
granites and associated mafic melts are interpreted to reflect the magmatic arc stage in the Cyclades starting at ~15 Ma. 相似文献
8.
东天山红柳河地区分布着大量的海西期花岗岩体，从早到晚，依次为河西站岩体、红柳河岩体、河西岩体和天湖岩体，主要岩石类型为花岗闪长岩、二长花岗岩和斜长花岗岩，河西站和红柳河花岗岩的岩相学和地球化学具有S型花岗岩的特征，而河西岩体和天湖岩体显示出I型花岗岩特征，河西花岗岩微量元素含量最低，具Eu弱正异常，类似于adakite岩地球化学特点；其他花岗岩微量元素含量高，具Eu负异常，与洋脊花岗岩相比，该区花岗岩不同程度地富集K2O、Rb、Ba、Th和Ce，亏损Ta、Nb、Zr、Hf、Y、Yb等，河西花岗岩、河西站和红柳河花岗岩、天湖花岗岩分别具有火山弧、同碰撞才碰撞后花岗岩特点，河西花岗岩和其他花岗岩分别起源于先前存在的大洋拉斑玄武岩残片和古老地壳岩石的部分熔融，这些花岗岩均形成于陆内造山环境，与东天山海西晚期地壳-岩石圈的挤压和伸展作用有关。 相似文献
9.
拉地贡玛地区花岗岩处于金沙江缝合带内,区域上隶属西金乌兰—金沙江缝合带的物质组成部分,在研究区属通天河构造岩浆岩带。据出露岩石类型,将其划分为3个单元: 拉地贡玛花岗闪长岩(T3γδ)、日阿日曲石英闪长岩(T3δο)、缅切英云闪长岩(T3δi)。岩浆侵位时代为晚三叠世; 侵入岩体是以高硅富铝、多碱质和挥发组分为特征的兼具I型和S型花岗岩,属过铝质花岗岩; 轻重稀土分馏程度明显,轻稀土富集,Eu、Ce呈弱负异常,Rb、Th、Ba等元素富集,Y、Yb、Cr等元素亏损,具I型和S型花岗岩的特点,与火山弧钙碱性花岗岩特征相似。研究区花岗岩形成构造环境与晚三叠世多彩—当江构造混杂带的俯冲作用有关,是与俯冲汇聚构造环境有关的大陆碰撞弧型花岗岩。 相似文献
10.
L. P. Black J. L. Everard M. P. McClenaghan C. R. Calver A. M. Fioretti 《Australian Journal of Earth Sciences》2013,60(7):933-968
Devonian–Carboniferous granites are widespread in Tasmania. In eastern Tasmania, Devonian granites intrude Ordovician–Early Devonian quartz-rich turbidites of the Mathinna Supergroup. The earliest (～400 Ma) I-type granodiorites may be arc-related. Following the Tabberabberan Orogeny (～389 Ma), more felsic and, finally, strongly fractionated I- and S-type granites were emplaced until ～373 Ma. In contrast, western Tasmania granites intrude a more diverse terrane of predominantly marine shelf successions, with depositional ages as old as Late Mesoproterozoic. They are mostly felsic and fractionated I- and S-types emplaced from ～374–351 Ma, possibly in response to post-collisional crustal extension following juxtaposition of the eastern and western Tasmanian terranes. Granites from the two terranes are readily distinguishable by the age spectra of their inherited zircon, which are noticeably similar to those of the detrital zircon from sedimentary successions in their respective terranes. Furthermore, within each terrane, both I and S-types yield similar inheritance patterns. This suggests a pivotal role for the sedimentary successions in the petrogenesis of both types. Western Tasmanian granites are also enriched in ～1600 Ma zircon, which is essentially unrepresented in the exposed supracrustal succession. Subtle differences between the inheritance and detrital age spectra in eastern Tasmania probably relate to unrepresentative sampling of the supracrustal rocks. Nd, Sr and Pb isotopic characteristics of the granites are consistent with their derivation by mixing of magmas derived from the mantle, possibly the lower crust, and from supracrustal rocks. Systematic isotopic trends in some eastern Tasmanian I-types, particularly in the Scottsdale Batholith, correlate well with major and trace element geochemistry and age. The isotopes are inconsistent with simple restite unmixing or crystal fractionation in a closed magma chamber, and indicate progressive contamination by the Mathinna Supergroup, or similar rocks. The isotopic characteristics of late, strongly fractionated granites, although sometimes obscured by hydrothermal alteration, are also consistent with concurrent assimilation-fractional crystallisation processes. Together with the close association of some strongly fractionated I- and S-types, this suggests that such granites were generated directly in the lower crust, and were not derived from unfractionated parental granite magmas. 相似文献
11.
永福岩体位于永梅晚古生代拗陷带中部。利用LA-ICP-MS锆石U-Pb定年法测得永福岩体中YF-1样品的年龄为133±1 Ma(MSWD=0.50)、YF-2样品的年龄为143±1 Ma(MSWD=0.59),说明其形成于早白垩世,与燕山期岩浆活动有关。该岩体富硅、碱,里特曼指数σ=0.96~2.43,铝饱和指数(A/CNK)=0.98~1.66,属高钾钙碱性系列,准铝质到过铝质范围。稀土元素总量较高,LREE相对富集,HREE相对亏损;具中-弱Eu负异常,弱Ce负异常到无异常,轻重稀土的分馏较微弱;微量元素表现为亏损元素Ba、Sr、K、P和Ti,富集Th、U、Zr、Hf等元素。样品YF-2~YF-7具有S型花岗岩特征,为永福岩体主体,源岩可能来自古-中元古代下地壳沉积岩;而样品YF-1具有Ⅰ型花岗岩特征,源岩可能来自古-中元古代下地壳火成岩。锆石的εHf(t)值除一颗来自残留基底为正值外,其他锆石全部为负值(-4.30~-11.82),Hf同为素二阶段模式年龄tDM2为1.45~1.92 Ga,表明永福岩体可能形成于古老地壳物质的重融。岩体形成于燕山期地壳的伸展背景下,在岩石圈伸展作用下幔源岩浆底侵促使古-中元古代下地壳沉积岩先发生部分熔融,形成永福岩体早期的S型花岗岩,岩浆作用后期,古-中元古代下地壳火成岩部分熔融,形成永福岩体晚期的I型花岗岩。 相似文献
12.
Tectonic implications from Re-Os dating of Mesozoic molybdenum deposits in the East Qinling-Dabie orogenic belt 总被引：34，自引：0，他引：34
J.W. Mao G.Q. Xie W.J. Qü H.S. Ye H.M. Li Y.F. Li 《Geochimica et cosmochimica acta》2008,72(18):4607-4626
The East Qinling-Dabie molybdenum belt is part of a larger East-West trending metallogenic belt in eastern China. Most of the molybdenum deposits occur as porphyry or porphyry-skarn type, but there are also some vein type deposits. Following systematic Re-Os dating of molybdenite from 13 deposits and comparisons with two previously dated deposits, we have recognized that the molybdenum mineralization in the East Qinling-Dabie belt was developed during hydrothermal activity linked to magmatism and the emplacement of granitoid stocks. Three pulses of granitoid magmatism and Mo mineralization are recognized corresponding to significant tectonic events in the East Qinling-Dabie belt. Vein type deposits dated at 233-221 Ma were formed in detachment fractures, indicating localized extension within the collisional setting of the North China and Yangtze Cratons. I-type and transitional I- and S-type granites and related mineralization dated at 148-138 Ma may have formed part of a continental magmatic arc, with widespread magmatism and back-arc extension caused by subduction of the Izanagi or Paleopacific plate beneath the Eurasian continent in a WNW-ESE direction in the Late Jurassic-Early Cretaceous. Both S-type and transitional S- and I-type granite-associated porphyry molybdenum deposits dated at 131-112 Ma are part of an extensive mineralization event throughout East China that can be ascribed to regional large-scale lithospheric thinning, delamination and thermal erosion. 相似文献
13.
14.
Malihe Shahzeidi Mohsen Moayyed Mamoru Murata Tzen-Fu Yui Shoji Arai Fukun Chen 《International Geology Review》2017,59(7):793-811
The aim of this article is to examine the geochemistry and geochronology of the Cadomian Mishu granites from northwest Iran, in order to elucidate petrogenesis and their role in the evolution of the Cadomian crust of Iran. The Mishu granites mainly consist of two-mica granites associated with scarce outcrops of tonalite, amphibole granodiorite, and diorite. Leucogranitic dikes locally crosscut the Mishu granites. Two-mica granites show S-type characteristics whereas amphibole granodiorite, tonalities, and diorites have I-type signatures. The I-type granites show enrichment in large-ion lithophile elements (e.g. Rb, Ba and K) and depletion in high field strength elements (e.g. Nb, Ti and Ta). These characteristics show that these granites have been formed along an ancient, fossilized subduction zone. The S-type granites have high K, Rb, Cs (and other large ion lithophile elements) contents, resembling collision-related granites. U–Pb zircon dating of the Mishu rocks yielded 238U/206Pb crystallization ages of ca. 550 Ma. Moreover, Rb–Sr errorchron shows an early Ediacaran age (547 ± 84 Ma) for the Mishu igneous rocks. The two-mica granites (S-type granites) show high 87Sr/86Sr(i) ratios, ranging from 0.7068 to 0.7095. Their ?Nd values change between ?4.2 and ?4.6. Amphibole granitoids and diorites (I-type granites) are characterized by relatively low 87Sr/86Sr(i) ratios (0.7048–0.7079) and higher values of ?Nd (?0.8 to ?4.2). Leucogranitic dikes have quite juvenile signature, with ?Nd values ranging from +1.1 to +1.4 and Nd model ages (TDM) from 1.1 to 1.2 Ga. The isotopic data suggests interaction of juvenile, mantle-derived melts with old continental crust to be the main factor for the generation of the Mishu granites. Interaction with older continental crust is also confirmed by the presence of abundant inherited zircon cores. The liquid-line of descend in the Harker diagrams suggests fractional crystallization was also a predominant mechanism during evolution of the Mishu I-type granites. The zircon U–Pb ages, whole rock trace elements, and Sr–Nd isotope data strongly indicate the similarities between the Mishu Cadomian granites with other late Neoproterozoic–early Cambrian (600–520 Ma) granites across Iran and the surrounding areas such as Turkey and Iberia. The generation of the Mishu I-type granites could be related to the subduction of the Proto-Tethyan Ocean during Cadomian orogeny, through interaction between juvenile melts and old (Mesoproterozoic or Archaean) continental crust. The S-type granites are related to the pooling of the basaltic melts within the middle–upper parts of the thick continental crust and then partial melting of that crust. 相似文献
15.
门巴区晚白垩世花岗岩主要分布于冈底斯中段的扎雪、金达和桑巴附近,由黑云母钾长花岗岩、钾长花岗岩和二云母钾长花岗岩及花岗闪长岩等组成。其中花岗闪长岩SHRIMP 锆石U--Pb 年龄为68. 8 ± 1. 6 Ma; 钾长花岗岩黑云母K--Ar 年龄为78. 2 ± 1. 2 Ma 和81. 5 ± 1. 4 Ma; 黑云母钾长花岗岩和二云母钾长花岗岩的黑云母K--Ar 分别为90. 8 ± 1. 81 Ma 和91. 2 ± 1. 8 Ma。岩石学和地球化学分析结果表明,S 型和低Sr 低Yb 特征的黑云母钾长花岗岩和二云母钾长花岗岩形成于拉萨地块与羌塘地块碰撞造山过程中的地壳加厚背景; S 型和总体低Sr、高Yb 特征的钾长花岗岩形成于造山带晚期阶段的伸展背景; I 型花岗闪长岩应是新特提斯洋俯冲作用的结果,形成于岛弧构造环境。 相似文献
16.
Despite extensive geochemical study and their importance to granite studies, the geochronology of Silurian to early-Devonian granitic rocks of southeastern Australia is poorly understood. In order to provide an improved temporal framework, new ion microprobe U–Pb zircon ages are presented from these rocks, and previous work is critically reviewed. Geochronological control is best in the Berridale Batholith, where S- and I-type granites have a close spatial relationship. In this region, there is a small volume of I-type granite that crystallised at 436 Ma, followed closely by a large volume of S-type granite at 432 Ma. I-type granite is abundant in a second peak at ca 417 Ma, although the Jindabyne pluton from the Kosciuszko Batholith is slightly older, at 424 Ma. A broader survey of S-type granite throughout the eastern Lachlan Orogen shows that the 432 Ma event is ubiquitous. There is no temporal overlap between S- and I-type granites in the Kosciuszko and Berridale Batholiths, which suggests that factors other than variations in degree of crustal contamination (which may include variation in tectonic setting, heat-flow, mass transfer across the crust–mantle boundary and/or availability in source materials) contribute to the diversity in granite types. The S-type granitic rocks occupy an aerial extent of greater than 28 000 km2, and geochronological constraints suggest that the crystallisation of these granites took place over a relatively small interval, probably less than 10 m.y. This implies a magmatic flux of over 64 km3/Ma per km strike length, comparable to other high-flux granitic belts. Previous work has linked the Benambran Orogeny to the generation of the S-type granites, and so the age of these granites constrains the age of Benambran Orogenesis 相似文献
17.
黑龙江宝山一带海西晚期强过铝花岗岩地质地球化学及岩石成因 总被引：4，自引：0，他引：4
黑龙江宝山地区在构造上位于兴蒙造山带东部的松嫩地块和佳木斯地块之间的伊春-延寿花岗岩带北段,区内分布大面积的古生代-中生代花岗岩.其中海西晚期花岗岩,岩性主要为碱长花岗岩、二长花岗岩和花岗闪长岩等,锆石U-Pb法 LA-ICP MS测年结果为252.6±3 Ma.其主量元素表现出富Si、略富Al、富碱质和低Mg、低Ca的特点;微量元素表现出富集Rb、Nd、K、Pb、U和亏损Nb、Ta、P、Ti等高场强元素的特点,并且Sr、Ba呈明显的负异常;稀土元素具有明显的轻稀土元素富集、重稀土元素相对亏损的特征,轻重稀土元素分馏程度较高.岩石总体上属于高钾钙碱性花岗岩,是岩浆经历了高度结晶分异作用的产物.矿物化学和岩石地球化学特征表明其特征类似于S型花岗岩,源岩物质来自于地壳. 相似文献
18.
勐养花岗闪长岩体位于滇西腾冲地块梁河县南勐养镇一带。用LA-ICP-MS技术测得花岗闪长岩锆石U-Pb年龄为115.2±1.0Ma,该年龄被解释为花岗闪长岩的形成年龄,表明该区花岗闪长岩体的形成时代为早白垩世。岩石地球化学特征表明,花岗闪长岩中SiO_2含量为62.39%~67.97%,Na_2O+K_2O为6.26%~7.80%,K_2O为1.98%~4.11%,具有贫钾(K_2O/Na_2O值为0.45~1.11)、低P2O5(0.09%~0.38%)的特征;MgO为1.78%~1.98%,Mg~#为34.90~48.40,属于准铝质-弱过铝质钙碱性系列。微量元素具有相对富集大离子亲石元素(U、Th、Rb、Ba)、亏损高场强元素(Tb、Nb、Zr、Hf)的特点。该花岗闪长岩具有I型花岗岩的特征,同时兼有S型花岗岩之特点,具有明显的岩浆混合作用特征。岩石具有岛弧或活动陆缘岩系的微量元素分布特征。地球化学特征和微量元素构造判别图解揭示,勐养早白垩世花岗闪长岩形成于碰撞后岩浆弧环境。花岗闪长岩为幔源岩浆与高黎贡山群古老地壳部分熔融的岩浆混合的产物。该区早白垩世花岗闪长岩是腾冲地块早白垩世侵入岩与班公湖-怒江-泸水-瑞丽洋盆的闭合、洋壳向南西俯冲及板块间的碰撞造山作用的产物。 相似文献
19.
本文将晚古生代以来苏门答腊火成岩划分出四个岩浆-构造旋回或岩浆活动期次（海西期、印支期、燕山期和喜山期）,并讨论其板块构造背景。结果表明：分布于西苏门答腊地体海西期酸性侵入岩属于碰撞后地壳的火山弧I-型花岗岩带,其火山岩为大陆拉张带（初始裂谷）中的安山．玄武岩系列,而分布在东苏门答腊地体的大多数酸性侵入岩具有s-型花岗岩的性质。印支期西苏门答腊地体侵入岩为I-型花岗岩,属于火山弧花岗岩。印支期碰撞后板内岩浆活动带（廖内群岛-班加岛-勿里洞岛）的侵入岩以含锡s-型花岗岩为特色。燕山期以后的深成岩-火山岩活动的岩石类型和分布特征,受大陆拉张带（初始裂谷）及其相邻的洋岛的控制。燕山早期细碧岩属于陆缘裂谷火山岩。喜山期火山岩属于陆缘火山弧,其中橄榄玄粗岩落在洋岛玄武岩与洋中脊玄武岩（MORB）交界线附近。 相似文献
20.
Tin polymetallic deposits are the most important type of tin deposit in the Nanling region. Manyresearchers both at home and abroad consider this type of tin deposit to be the product of differentiation andevolution of granite magmas resulting from anatexis of continental crust and to be genetically related to thetransformation-type (S-type) granitoids. In this paper, on the basis of the geological settings, petrology, REEgeochemistry and strontium and oxygen isotopic compositions of 6 granite intrusions associaied with tinpolymetallic deposits in the Nanling region, the authors suggest that the ore-bearing granites of this type areprobably the products of differentiation and evolution of acid magmas resulting from 40-50‰ fractionalcrystallization of magmas formed by partial melting of the pre-existing intermediate-basic volcanic rocks ofmantle origin in the lower crust and a small amount of sialic material and belong to crust-mantle-derivedgranitoids (approaching I-type of B. W. Chappell and A.J.R. White, but being evidently different from theS-type granitoid related to W, Sn, Nb, Ta and REE deposits). 相似文献