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1.
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2.
http://www.sciencedirect.com/science/article/pii/S1674987113000078   总被引：1，自引：0，他引：1  
A sequence of gabbros showing isotropic,layered and fine-grained textures is exposed in the Nalaqing mine at the southern tip of the～260 Ma Panzhihua intrusion,SW China.The field relations,structure,texture and mineralogy of the rocks indicate that the sequence represents the transition between the Lower zone and Middle zone of the intrusion.Isotropic gabbros characteristic of the Lower zone pass upward to layered gabbros of the Middle zone through a～5 m-thick microgabbro sheet,within and close to which small-scaled, concordant Fe-Ti oxide ore horizons are identified.Strong fractionation between HFSE and REE in a subset of samples is ascribed to cumulus titanomagnetite into which HFSE are preferentially incorporated over REE,as reflected in the parallel relations between Nb/La,Hf/Sm and Ti/Ti*.Both the isotropic and layered gabbros display cumulate textures and have similar mineral compositions(Mg# of clinopyroxene =～76-79 and An59-61),isotopic compositions[(87Sr/86Sr)i = 0.7044-0.7045 andεNd（t） = +2.4 to +3.9]and trapped liquid contents inferred from Zr abundance（～17-34 ppm）.However,there are substantial variations in elemental abundances（V,Cr and PGE） and ratios（Ti/V,La/Yb,Ba/Y and Cu/Pd） between the two types of gabbros,features that cannot be explained by cumulate formation from a common magma in a closed system.The microgabbros generally resemble high-Ti Emeishan basalts in major element compositions,but their low trace element abundances indicate some lost of residual liquid is inevitable despite rapid nucleation and cooling.Combined with available data and observations,we propose a model involving in-situ crystallization,followed by magma recharge and closed-system fractionation to explain the formation of texturally distinctive gabbros at Nalaqing and the evolution of the lower part of the Panzhihua intrusion.  相似文献   

3.
哈拉乔拉镁铁质岩体位于新疆阿尔泰造山带东南缘, 主要岩石类型有辉长岩、辉长苏长岩、含长辉石岩、橄榄辉长岩和橄长岩.哈拉乔拉岩体具有低TiO2(0.09%~1.28%)、低碱(Na2O+K2O=0.37%~0.78%)的特点, 属于拉斑玄武岩系列; 富集大离子亲石元素和轻稀土元素, 亏损高场强元素(Nb、Ta等), εNd(t)为-2.62~-0.78, εSr(t)为37.49~45.28.元素地球化学和Nd-Sr同位素组成表明, 岩浆源区为被消减板片交代改造过的富集型岩石圈地幔.原生岩浆为高镁拉斑玄武岩浆, 岩浆演化过程中主要发生了橄榄石、单斜辉石以及斜长石的分离结晶/堆晶, 后期有钛铁矿的析出.   相似文献   

4.
The Neoproterozoic Korab Kansi mafic-ultramafic intrusion is one of the largest (100 km2) intrusions in the Southern Eastern Desert of Egypt. The intrusion consists of Fe-Ti-bearing dunite layers, amphibole peridotites, pyroxenites, troctolites, olivine gabbros, gabbronorites, pyroxene gabbros and pyroxene-hornblende gabbros, and also hosts significant Fe-Ti deposits, mainly as titanomagnetite-ilmenite. These lithologies show rhythmic layers and intrusive contacts against the surrounding granites and ophiolitic-island arc assemblages. The wide ranges of olivine forsterite contents (Fo67.9-85.7), clinopyroxene Mg# (0.57–0.95), amphibole Mg# (0.47–0.88), and plagioclase compositions (An85.8-40.9) indicate the role of fractional crystallization in the evolution from ultramafic to mafic rock types. Clinopyroxene (Cpx) has high REE contents (2–30 times chondrite) with depleted LREE relative to HREE, like those crystallized from ferropicritic melts generated in an island-arc setting. Melts in equilibrium with Cpx also resemble ferropicrites crystallized from olivine-rich mantle melts. Cpx chemistry and its host rock compositions have affinities to tholeiitic and calc-alkaline magma types. Compositions of mafic-ultramafic rocks are depleted in HFSE (e.g. Nb, Ta, Zr, Th and U) relative to LILE (e.g. Li, Rb, Ba, Pb and Sr) due to the addition of subduction-related hydrous fluids (rich in LILE) to the mantle source, suggesting an island-arc setting. Fine-grained olivine gabbros may represent quenched melts approximating the primary magma compositions because they are typically similar in assemblage and chemistry as well as in whole-rock chemistry to ferropicrites. We suggest that the Korab Kansi intrusion crystallized at temperatures ranging from ~700 to 1100 °C from ferropicritic magma derived from melting of metasomatized mantle at <5 Kbar. These hydrous ferropicritic melts were generated in the deep mantle and evolved by fractional crystallization under high ƒO2 at relatively shallow depth. Fractionation formed calc-alkaline magmas during the maturation of an island arc system, reflecting the role of subduction-related fluids. The interaction of metasomatized lithosphere with upwelling asthenospheric melts produced the Fe and Ti-rich ferropicritic parental melts that are responsible for precipitating large quantities of Fe-Ti oxide layers in the Korab Kansi mafic-ultramafic intrusion. The other factors controlling these economic Fe-Ti deposits beside parental melts are high oxygen fugacity, water content and increasing degrees of mantle partial melting. The generation of Ti-rich melts and formation of Fe-Ti deposits in few layered intrusions in Egypt possibly reflect the Neoproterozoic mantle heterogeneity in the Nubian Shield. We suggest that Cryogenian-Tonian mafic intrusions in SE Egypt can be subdivided into Alaskan-type intrusions that are enriched in PGEs whereas Korab Kansi-type layered intrusions are enriched in Fe-Ti-V deposits.  相似文献   

5.
The Cordillera del Paine pluton in the southernmost Andes of Chile represents a deeply dissected magma chamber where mafic magma intruded into crystallizing granitic magma. Throughout much of the 10x15 km pluton, there is a sharp and continuous boundary at a remarkably constant elevation of 1,100 m that separates granitic rocks (Cordillera del Paine or CP granite: 69–77% SiO2) which make up the upper levels of the pluton from mafic and comingled rocks (Paine Mafic Complex or PMC: 45–60% SiO2) which dominate the lower exposures of the pluton. Chilled, crenulate, disrupted contacts of mafic rock against granite demonstrate that partly crystallized granite was intruded by mafic magma which solidified prior to complete crystallization of the granitic magma. The boundary at 1,100 m was a large and stable density contrast between the denser, hotter mafic magma and cooler granitic magma. The granitic magma was more solidified near the margins of the chamber when mafic intrusion occurred, and the PMC is less disrupted by granites there. Near the pluton margins, the PMC grades upward irregularly from cumulate gabbros to monzodiorites. Mafic magma differentiated largely by fractional crystallization as indicated by the presence of cumulate rocks and by the low levels of compatible elements in most PMC rocks. The compositional gap between the PMC and CP granite indicates that mixing (blending) of granitic magma into the mafic magma was less important, although it is apparent from mineral assemblages in mafic rocks. Granitic magma may have incorporated small amounts of mafic liquid that had evolved to >60% SiO2 by crystallization. Mixing was inhibited by the extent of crystallization of the granite, and by the thermal contrast and the stable density contrast between the magmas. PMC gabbros display disequilibrium mineral assemblages including early formed zoned olivine (with orthopyroxene coronas), clinopyroxene, calcic plagioclase and paragasite and later-formed amphibole, sodic plagioclase, mica and quartz. The early formed gabbroic minerals (and their coronas) are very similar to phenocrysts in late basaltic dikes that cut the upper levels of the CP granite. The inferred parental magmas of both dikes and gabbros were very similar to subalkaline basalts of the Patagonian Plateau that erupted at about the same time, 35 km to the east. Mafic and silicic magmas at Cordillera del Paine are consanguineous, as demonstrated by alkalinity and trace-element ratios. However, the contemporaneity of mafic and silicic magmas precludes a parent-daughter relationship. The granitic magma most likely was derived by differentiation of mafic magmas that were similar to those that later intruded it. Or, the granitic magma may have been contaminated by mafic magmas similar to the PMC magmas before its shallow emplacement. Mixing would be favored at deeper levels when the cooling rate was lower and the granitic magma was less solidified.  相似文献   

6.
M. Lachize  J. P. Lorand  T. Juteau 《Lithos》1996,38(3-4):207-232
The Wadi Haymiliyah section, in the Haylayn block (Semail ophiolite, Oman) displays an unusual plutonic sequence closely similar to those of supra-subduction zone harzburgitic ophiolites (“Troodos sub-type”). It comprizes a bottom, 1000 m-thick, coarse-grained layered gabbro unit (MLGU) overlain by a 1000 m-thick, fine-grained, laminated noritic gabbro unit (MLNGU). Taken as a whole, the mineralogical and bulk-rock trends of the Haymiliah plutonic sequence are those of arc-related calc-alkaline plutons. The MLGU layered gabbros are olivine gabbros and gabbros which differ from low-P cumulates of MORB (oceanic gabbros) by Fe3+-rich cumulus chrome spinel [Fe3+/(Fe3+ + Al + Cr) = 0.2-0.3], diopside (Mg# = 85–91) co-crystallized with highly calcic plagioclase (An96-80) and intercumulus magnesian orthopyroxene (Mg# = 87-80). Plagioclase remains highly calcic at decreasing Fo content, indicating crystallization under high water pressure (> 500 bar). Despite an abrupt decrease in grain size, there exists modal and chemical gradations between MLGU and MLNGU. In the uppermost part of the MLGU, coarse-grained, gabbroic cyclic units culminate with two-pyroxene gabbros containing up to 20 wt.% cumulus Opx. These latter are interbedded over a thickness of ca. 300 m with fine-grained two-pyroxene gabbros and noritic gabbros layers which differ only by slightly higher modal opx and plagioclase contents. The bottom of the MLNGU is marked by norite layers containg up to 80 wt.% plagioclase, cumulus Ti-magnetite and abundant intercumulus Ti-pargasite. Unlike low-pressure differentiates of MORBs, the MLNGU lacks pigeonite and Fe-Ti oxide layers. Cumulus titanomagnetite appears immediately after the orthopyroxene (Mg# = 72–76) in the crystallization order of the norites. The abundance of interstitial Ti-poor pargasite increases at the top of the MLNGU which is brecciated by dioritic differentiates. Both features indicate increasing water pressure and oxygen fugacity (NNO + 2 log units) symptomatic of closed-system magmatic differentiation. Mg#'s of both pyroxenes (70–80) decrease moderately relative to the MLGU coarse-grained gabbros. This and the increase of plagioclase and orthopyroxene modal proportions produce increasing SiO2-Al2O3-Na2O and Sr contents at nearly constant FeO/MgO in bulk-rock chemistry. This feature similar to the calc-alkaline differentiation trend, is due primarily to a parental tholeiitic magma more hydrated and oxidized than MORBs (ƒO2 = NNO instead of NNO-2 to NNO-3 log unit); this trend is fully developed in the Wadi Haymiliah section because closure of the magma reservoir in this region allowed larger extent of magmatic differentiation than in other blocks of the Semail ophiolite. The water-rich and oxidized nature of the parental magmas argues for the evolution of the Semail ophiolite in a marginal basin above a subduction zone rather than at a mature oceanic spreading center.  相似文献   

7.
The Sept Iles layered intrusion (Quebec, Canada) is dominated by a basal Layered Series made up of troctolites and gabbros, and by anorthosites occurring (1) at the roof of the magma chamber (100-500 m-thick) and (2) as cm- to m-size blocks in gabbros of the Layered Series. Anorthosite rocks are made up of plagioclase, with minor clinopyroxene, olivine and Fe-Ti oxide minerals. Plagioclase displays a very restricted range of compositions for major elements (An68-An60), trace elements (Sr: 1023-1071 ppm; Ba: 132-172 ppm) and Sr isotopic ratios (87Sr/86Sri: 0.70356-0.70379). This compositional range is identical to that observed in troctolites, the most primitive cumulates of the Layered Series, whereas plagioclase in layered gabbros is more evolved (An60-An38). The origin of Sept Iles anorthosites has been investigated by calculating the density of plagioclase and that of the evolving melts. The density of the FeO-rich tholeiitic basalt parent magma first increased from 2.70 to 2.75 g/cm3 during early fractionation of troctolites and then decreased continuously to 2.16 g/cm3 with fractionation of Fe-Ti oxide-bearing gabbros. Plagioclase (An69-An60) was initially positively buoyant and partly accumulated at the top of the magma chamber to form the roof anorthosite. With further differentiation, plagioclase (<An60) became negatively buoyant and anorthosite stopped forming. Blocks of anorthosite (autoliths) even fell downward to the basal cumulate pile. The presence of positively buoyant plagioclase in basal troctolites is explained by the low efficiency of plagioclase flotation due to crystallization at the floor and/or minor plagioclase nucleation within the main magma body. Dense mafic minerals of the roof anorthosite are shown to have crystallized from the interstitial liquid.The processes related to floating and sinking of plagioclase in a large and shallow layered intrusion serve as a proxy to refine the crystallization model of the lunar magma ocean and explain the vertically stratified structure of the lunar crust, with (gabbro-)noritic rocks at the base and anorthositic rocks at the top. We propose that the lunar crust mainly crystallized bottom-up. This basal crystallization formed a mafic lower crust that might have a geochemical signature similar to the magnesian-suite without KREEP contamination, while flotation of some plagioclase grains produced ferroan anorthosites in the upper crust.  相似文献   

8.
In situ LAM-ICPMS U-Pb, Hf-isotope and trace-element analyses of zircon have been used to evaluate the relative contributions of juvenile mantle and crustal sources to the intrusive rocks of the mafic to intermediate, gold-poor Tuckers Igneous Complex (TIC), and the spatially and temporally related, felsic Mount Leyshon Igneous Complex (MLIC), which hosts a gold-rich porphyry system.

The TIC intrusions range in age from 304.2 ± 9.1 Ma to 288.5 ± 6.4 Ma, and the MLIC intrusions from 291.0 ± 4.8 Ma to 288 ± 6 Ma. Cross-cutting relationships define the intrusion sequence from oldest to youngest; Diorite, Monzodiorite, Mafic Granodiorite and Biotite Microgranite within the TIC; Early Dyke, Southern Porphyry and Late Dyke within the MLIC.

Zircons from the earliest rock type within each complex have a wide range in Hf (5.2 to 14.8 for the TIC Diorite, 2.0 to 12.4 for the MLIC Early Dykes) suggesting the mixing of juvenile and crustal magmas. This interpretation is supported by trace-element data that show the presence of two distinct zircon populations in the MLIC Early Dyke. The later intrusive rocks have narrower ranges in Hf (typically < 4 Hf units) and trace-element patterns of zircon. This homogeneity suggests derivation from magmas produced by further mixing and fractional crystallisation of the TIC Diorite and the MLIC Early Dyke magmas respectively. A greater crustal contribution to the gold-rich MLIC is inferred from the range of median Hf (3.2 to 4.5 for the MLIC, 5.4 to 8.7 for the TIC). We suggest that the MLIC was derived by melting of more felsic crustal rocks, and with less input from juvenile mantle, then the TIC; it was not derived by fractional crystallisation of an intermediate to mafic TIC-like magma. Modelling of Hf isotope data yields a mean model age of 1040 ± 10 Ma (at 176Lu/177Hf = 0.015) for the crustal component in both complexes.

Gold was precipitated in the MLIC Breccia during the emplacement of the Late Dykes. The isotopically homogenous nature of the Late Dykes suggests that no additional juvenile-mantle input was involved at the mineralisation stage. This supports a model in which gold and other metals were indigenous to the Late Dykes magma and were concentrated by magma differentiation and fluid-evolution processes.  相似文献   


9.
为确定云南省个旧地区晚中生代大规模岩浆活动过程中基性端元的时限、地幔源区特点及大地构造环境,选取贾沙辉长．二长岩体为对象进行年代学和地球化学研究。贾沙辉长．二长岩体位于个旧西区,岩性主要为辉长岩和二长岩。锆石U．Pb同位素测年结果表明,岩石侵位时代为（84．0＋0．6）Ma,属于晚白垩世,与个旧地区花岗岩、碱性岩和煌斑岩形成年代范围一致（76～85Ma）。贾沙岩体的辉长岩和二长岩Si02为47．3％～60．O％,K20＋Na20为7．31％～10．1％。稀土含量较高,轻稀土富集重稀土亏损,Eu异常不明显。相对于原始地幔,贾沙岩体富集轻稀土和大离子亲石元素Rb、K、Pb,亏损高场强元素Nb、Ta、Ti和P。地球化学研究显示贾沙岩体母岩浆起源于与俯冲有关的交代地幔,由石榴子石二辉橄榄岩经历了较低程度的（〈5％）部分熔融形成。原始岩浆在就位过程中经历了广泛的地壳混染和橄榄石、辉石的分离结晶作用。二长岩由辉长岩浆结晶分异作用形成。研究显示,贾沙辉长．二长岩体是晚白垩世滇东南．桂西地区大规模岩浆活动的产物,表明这些岩浆岩形成于统一的岩石圈伸展的动力学背景下。  相似文献   

10.
香山西岩体是东天山地区发现的唯一的一个铜镍-钛铁复合型含矿岩体,前人对香山西铜镍-钛铁矿床成因认识一直存在争议。本次通过矿相学研究结合电子探针分析,在香山西铜镍矿石中发现了铜镍硫化物与钛铁氧化物共生的现象,并首次测定了香山西钛铁辉长岩的SIMS锆石U-Pb年龄为278.6±1.8Ma(MSWD=1.2),与前人测得香山中岩体角闪辉长岩的锆石U-Pb年龄基本一致,证实了香山西铜镍矿与钛铁矿为共生关系,两者空间上渐变过渡。岩石地球化学研究表明,香山岩体(包括钛铁辉长岩)为同源岩浆经结晶分异作用形成的一套镁铁-超镁铁质岩体,具有拉斑玄武质岩浆分异演化趋势,并且经历了与地壳物质的混染。与中段和东段岩石相比,香山西辉长岩类具有相对高的REE、SiO2(平均48.99%)、K2O+Na2O(平均3.43%)、TiO2(平均1.26%)和明显低的Mg#值(平均62.4),表现出分异演化程度高于中段和东段。经反演得出香山岩体原始岩浆含MgO约10%,FeO约9%,TiO2约1.14%,与同一成矿带内其它含铜镍矿岩体原始岩浆成份相近,应为 普通的拉斑玄武质岩浆。因此,香山西钛铁矿床的形成机制可能是由普通的拉斑玄武质岩浆,经历了较高程度的分异演化导致钛铁氧化物在残余岩浆中逐步富集,岩浆在上升侵位过程中与地壳物质的混染,不仅促使了岩浆中硫化物的饱和,同时提高了岩浆体系的氧逸度,进而促使了钛铁氧化物结晶沉淀。对香山西钛铁矿床成因研究的启示意义在于,除我国攀西地区高钛的玄武质岩浆外,普通的拉斑玄武质岩浆,在有利的分异演化条件下(如初始低氧逸度、相对高度的分异演化、后期与地壳物质混染)也有可能形成大型钛铁矿床。  相似文献   

11.
The Nantianwan mafic intrusion in the Panxi region, SW China, part of the ~260?Ma Emeishan large igneous province, consists of the olivine gabbro and gabbronorite units, separated by a transitional zone. Olivine gabbros contain olivine with Fo values ranging from 83 to 87, indicating crystallization from a moderately evolved magma. They have 0.2 to 0.9?wt?% sulfide with highly variable PGE (17?C151?ppb) and variable Cu/Pd ratios (1,500?C32,500). Modeling results indicate that they were derived from picritic magmas with high initial PGE concentrations. Olivine gabbros have negative ??Nd(t) values (?1.3 to ?0.1) and positive ??Os(t) values (5?C15), consistent with low degrees of crustal contamination. Gabbronorites include sulfide-bearing and sulfide-poor varieties, and both have olivine with Fo values ranging from 74 to 79, indicating crystallization from a more evolved magma than that for olivine gabbros. Sulfide-bearing gabbronorites contain 1.9?C4.1?wt?% sulfide and 37?C160?ppb PGE and high Cu/Pd ratios (54,000?C624,000). Sulfide-poor gabbronorites have 0.1?C0.6?wt?% sulfide and 0.2?C15?ppb PGE and very high Cu/Pd ratios (16,900?C2,370,000). Both sulfide-bearing and sulfide-poor gabbronorites have ??Nd(t) values (?0.9 to ?2.1) similar to those for olivine gabbros, but their ??Os(t) values (17?C262) are much higher and more variable than those of the olivine gabbros. Selective assimilation of crustal sulfides from the country rocks is thus considered to have resulted in more radiogenic 187Os of the gabbronorites. Processes such as magma differentiation, crustal contamination and sulfide saturation at different stages in magma chambers may have intervened during formation of the intrusion. Parental magmas were derived from picritic magmas that had fractionated olivine under S-undersaturated conditions before entering a deep-seated staging magma chamber, where the parental magmas crystallized olivine, assimilated minor crustal rocks and reached sulfide saturation, forming an olivine- and sulfide-laden crystal mush in the lower part and evolved magmas in the upper part of the chamber. The evolved magmas were forced out of the staging chamber and became S-undersaturated due to a pressure drop during ascent to a shallow magma chamber. The magmas re-attained sulfide saturation by assimilating external S from S-rich country rocks. They may have entered the shallow magma chamber as several pulses so that several gabbronorite layers each with sulfide segregated to the base and a sulfide-poor upper part. The olivine gabbro unit formed from a new and more primitive magma that entrained olivine crystals and sulfide droplets from the lower part of the staging chamber. A transitional zone formed along the boundary with the gabbronorite unit due to chemical interaction between the two rock units.  相似文献   

12.
The wide compositional spectrum of the Variscan batholiths of the Urals, a continuum from gabbros (or diorites) to leucogranites, was produced by crystal fractionation, but the physical mechanisms involved in formation of the bodies remains obscure. To test whether syn-magmatic deformation was essential to enhance the efficiency of the process, we studied the Main Series of Stepninsk, a pluton emplaced into an active crustal-scale strike-slip shear zone. The Main Series (>95 vol.% of total granitoids) is high-K calc-alkaline, comprises rocks with SiO2 from 51 to 77 wt.%, and stands out because most major and many trace elements yield excellent linear or curvilinear correlations with silica. It includes deformed gabbrodiorites to monzogranites, and undeformed syenogranites to alaskites. Deformed and undeformed rocks are coeval (283±2 Ma). All rocks, irrespective of their silica content, have the same initial Sr and Nd isotope ratios (87Sr/86Sr283 Ma=0.70488±0.000131; ε(Nd)283 Ma=−0.79±0.49), and contain amphibole and biotite with the same compositions. Based on thermodynamic and trace-element fractionation simulations, we propose a model of deformation-driven filter-pressing differentiation consistent with these features. The Main Series is derived from a hydrous high-K granodioritic magma which intruded containing 0.3 of early-formed solids. These accumulated locally by flow differentiation to produce the gabbrodiorites. The crystallization continued until the fraction of solids was higher than 0.55, after which different magma batches were efficiently squeezed by differential stress coupled with the opening of tensile fractures in the shear zone. This process produced a range of residua and segregates, the composition of which depended on the fraction of early-formed solids, the fraction of solids present when squeezing occurred and, especially, the efficiency of melt segregation. The monzodiorites and quartz–monzodiorites represent efficiently squeezed residua, the granodiorites to monzogranites represent unfractionated or little fractionated magma batches, and the leucogranites represent melt segregates with a few entrained crystals of amphibole and biotite. We proposed that wide-spectrum fractionation of granite magmas mainly occurs when they crystallize under compressive regimes, and is caused by deformation-driven filter-pressing differentiation.  相似文献   

13.
The Khopoli intrusion, exposed at the base of the Thakurvadi Formation of the Deccan Traps in the Western Ghats, India, is composed of olivine gabbro with 50–55 % modal olivine, 20–25 % plagioclase, 10–15 % clinopyroxene, 5–10 % low-Ca pyroxene, and <5 % Fe-Ti oxides. It represents a cumulate rock from which trapped interstitial liquid was almost completely expelled. The Khopoli olivine gabbros have high MgO (23.5–26.9 wt.%), Ni (733–883 ppm) and Cr (1,432–1,048 ppm), and low concentrations of incompatible elements including the rare earth elements (REE). The compositions of the most primitive cumulus olivine and clinopyroxene indicate that the parental magma of the Khopoli intrusion was an evolved basaltic melt (Mg# 49–58). Calculated parental melt compositions in equilibrium with clinopyroxene are moderately enriched in the light REE and show many similarities with Deccan tholeiitic basalts of the Bushe, Khandala and Thakurvadi Formations. Nd-Sr isotopic compositions of Khopoli olivine gabbros (εNdt?=??9.0 to ?12.7; 87Sr/86Sr?=?0.7088–0.7285) indicate crustal contamination. AFC modelling suggests that the Khopoli olivine gabbros were derived from a Thakurvadi or Khandala-like basaltic melt with variable degrees of crustal contamination. Unlike the commonly alkalic, pre- and post-volcanic intrusions known in the Deccan Traps, the Khopoli intrusion provides a window to the shallow subvolcanic architecture and magmatic processes associated with the main tholeiitic flood basalt sequence. Measured true density values of the Khopoli olivine gabbros are as high as 3.06 g/cm3, and such high-level olivine-rich intrusions in flood basalt provinces can also explain geophysical observations such as high gravity anomalies and high seismic velocity crustal horizons.  相似文献   

14.
The origin and evolution of the magma(s) involved in the formationof the olivine tholeiite cone-sheets which invade the 60-MaCuillin Igneous Complex, Isle of Skye, have been investigatedusing mineral chemistry data together with whole-rock major-and trace-element and isotope (Sr and Nd) geochemistry data.The most primitive compositions identified are almost identicalto those of the basalts being erupted at the present day alongthe spreading centre in Iceland. Rare examples of lavas fromthe slightly older lava pile of west-central and north Skye,together with a large number of dykes from the axial zone ofthe Skye Main Swarm, are of similar composition and are referredto as being of the Preshal More Basalt type (spelling is accordingto current Ordnance Survey of Great Britain maps). The intra-suitecompositional variation exhibited by the cone-sheets can beexplained in terms of relatively low-pressure fractionationof the three-phase assemblage olivine+clinopyroxene+plagioclasein their cotectic proportions of 10: 35: 55. Modelling of major-and compatible trace-element data indicates that the most evolvedcomposition may be derived by 60% crystallization of the leastevolved composition. Incompatible trace-element modelling impliesgreater degrees of crystal-liquid fractionation: Y and Zr indicate64 and 68% crystallization, respectively, whereas the rare earthelements (Eu, Yb, Gd, and Ce) indicate between 71 and 75% crystallization.This decoupled behaviour of compatible and incompatible elementsis attributed to the cone-sheet magma(s) evolving in a subjacentmagma chamber, before final emplacement in the overlying crust.Sr- and Nd-isotope data indicate that the cone-sheet magma(s)assimilated upper-crustal lithologies during fractional crystallization,most likely involving amphibolite facies gneiss of the LewisianGneiss Complex. This style of simultaneous assimilation andfractional crystallization (AFC) process in the upper crustfor the Skye cone-sheet magma(s) is in direct contrast to theprocesses identified for the magmas which produced the bulkof the lava field of west-central and north Skye, where assimilationoccurred after fractionation. The cone-sheet magmas were generatedby relatively large degrees of partial melting of a depletedmantle source associated with significant lithospheric stretching.The cause of this depletion, together with the temporal relationshipsbetween the cone-sheet magmas and the dominant transitionalmagmas of the Skye lava field and sill complex, are also discussed. * Reprint request to B. R. Bell  相似文献   

15.
The Newark Island layered intrusion is a composite layered intrusion within the Nain anorthosite complex, Labrador. The intrusion comprises a lower layered series (LS) dominated by troctolites, olivine gabbros and oxide-rich cumulates and an upper hybrid series (HS) characterized by a wide range of mafic, granitic and hybrid cumulates and discontinuous layers of chilled mafic rocks (Wiebe 1988). The HS crystallized from a series of replenishments of both silicic and basic magmas. The LS crystallized from periodically replenished basic magmas. The LS has a lower zone that consists mainly of olivine-plagioclase cumulates and contains minor cryptic reversals in mineral compositions that resulted from replenishments of relatively primitive magma. An upper zone is dominated by olivine-plagioclaseaugite-ilmenite cumulates. Cumulus titanomagnetite and pyrrhotite occur within some oxide-rich cumulates, and the stratigraphically highest layers contain cumulus apatite. At intermediate levels in the sequence, cumulus inverted pigeonite occurs in place of olivine. Several prominent regressions in the stratigraphy of the upper zone are marked by fine-grained troctolitic layers with much higher Mg no. [100 MgO/(MgO+FeO)] and anorthite than underlying cumulates. These layers coarsen upward and grade back to oxide-bearing olivine gabbros within thicknesses ranging from 10 cm to 15 m. Dikes that cut the LS have major- and trace-element compositions that strongly suggest that they are feeders for the replenishments. In the lower zone when olivine and plagioclase were the only cumulus phases, replenishments were less dense than the resident magma and rose as plumes and mixed with it. Precipitation of cumulus oxides in the upper zone lowered the density of resident magma so that subsequent replenishments were more dense than resident magma. Replenishments that occurred after oxides began to precipitate had small injection velocities. These post-oxide injections flowed along the interface between resident magma and the cumulate pile and precipitated flow-banded, fine-grained troctolites.  相似文献   

16.
西天山哈拉达拉辉长岩的Fe-Ti富集机制及其构造意义   总被引：4，自引：4，他引：0  
贺鹏丽  黄小龙  李洪颜  李洁  于洋  李武显 《岩石学报》2013,29(10):3457-3472
特克斯哈拉达拉辉长岩体是西南天山出露规模最大的层状基性-超基性侵入杂岩体,其富含Fe-Ti氧化物(含量高达15%)。哈拉达拉辉长岩中的橄榄石具有较低的Fo值(64~75),斜长石主要为中-拉长石,单斜辉石相对低Mg#(0.66~0.87),属于次透辉石或普通辉石,总体上显示出较高的岩浆演化程度。Fe-Ti氧化物以钒钛磁铁矿为主(TiO2=0.8%~20.6%;V2O3=0.10%~0.83%),常与钛铁矿呈矿物对共生或出溶钛铁矿。晚期的云母矿物均围绕他形的Fe-Ti氧化物生长,主要为富MgO的金云母,少量属于黑云母;大部分云母成分富含F、Cl(F+Cl高达3.14%),指示岩浆形成于贫水环境。哈拉达拉辉长岩体的主量元素成分变化很大(Mg#=0.48~0.73),橄榄辉长岩主要受橄榄石和斜长石的结晶分异/堆晶作用影响,而辉长岩的成分变化主要受控于斜长石和Fe-Ti氧化物的堆晶作用。哈拉达拉岩体的Fe-Ti氧化物主要为岩浆正常结晶分异作用的结果,该体系具有较低氧逸度、贫水的特点,其地幔源区的熔融程度较高,可能是塔里木地幔柱在天山造山带这一构造薄弱带的早期岩浆活动。  相似文献   

17.
笔架山东基性—超基性岩体位于塔里木板块东北部的新疆北山地区,是笔架山岩带中最东边的一个岩体,岩体形态为椭圆状,出露面积约5 km2.由含长单辉橄榄岩、橄榄辉长岩、含橄辉长岩、辉长岩以及辉绿岩组成.含橄榄石较多的岩石属拉斑玄武岩系列,而辉长岩属钙碱性系列.岩相学、岩石化学和微量元素地球化学特征表明岩浆演化过程中经历了橄榄石、辉石、斜长石的分离结晶作用.Nd、Sr、Pb同位素组成和岩石地球化学特征反映出岩浆与围岩之间存在物质交换.笔架山东岩体的岩浆源区为OIB型地幔源区,原生岩浆为高镁拉斑玄武岩浆[w(MgO)=11.2％],这些性质与塔里木板块东北部其他基性-超基性岩体的特征相似,表明塔里木板块东北部二叠纪基性—超基性岩体的源区主要为OIB型地幔,可能与地幔柱有关.  相似文献   

18.
The Cretaceous gabbros in the Fujian coastal region, southeastern China, experienced different magmatic and tectonic processes associated with deformation of the Changle-Nanao shear zone. Group 1 gabbros (115 Ma) show marked LILE (e.g., Sr, Ba and K) and LREE enrichment, and HFSE (e.g., Ta, Nb, Zr and Hf) depletion, strongly suggesting an island-arc affinity. The parental magma of group 1 gabbros, arguably derived from an arc-related source mantle modified by previous subduction, rose into and interacted with the coexisting syntectonic granitic magma generated during the main stage of shear zone deformation, and produced the gabbro-diorite-granite complexes. Group 2 and 3 gabbros (106-95 Ma) possibly formed by coupling of the subduction-modified source mantle with part of undepleted mantle (e.g., Nb enrichment) in an extensional environment at the end of deformation. Their parental magmas did not undergo significant magma mixing but produced a cumulate nature. All the three groups of gabbros were contaminated by crustal material during the processes of intrusion and emplacement.  相似文献   

19.
在安徽沿江地区,既分布有大量接触交代成因和叠加复合成因的矽卡岩矿床,也分布有岩浆成因的矽卡岩矿床。本文给出了不同类型岩浆矽卡岩及其矿床的定义,论述了安徽沿江地区中生代岩浆矽卡岩及其矿床的特征,并在此基础上分析了区域中生代矽卡岩岩浆－热液成矿作用。根据矽卡岩岩浆就位位置的不同可将岩浆矽卡岩分成原地矽卡岩和异地矽卡岩两类,相应地将岩浆矽卡岩矿床分成原地矽卡岩矿床和异地矽卡岩矿床两大类。两类矽卡岩及其矿床具有明显不同的特征。在地质产状上,原地矽卡岩岩体常与壳幔同熔岩浆侵入体紧密伴生而分布在壳幔同熔岩浆侵入体与碳酸盐围岩的接触带上,在矽卡岩岩体边缘一般没有冷凝边和烘烤边,但常能见到因同化混染作用不彻底而留下的围岩残留体（多已变质成角岩或大理岩）。与此明显不同的是,异地矽卡岩岩体常分布在断裂带或地层虚脱带中,附近一般没有壳幔同熔岩浆侵入体与其紧密伴生,在矽卡岩岩体边缘一般有冷凝边和烘烤边,有时能见到气孔构造以及石榴石或透辉石堆积岩,但见不到围岩残留体。同时,原地矽卡岩和异地矽卡岩均具有明显的水平分带,但两者明显不同。原地矽卡岩的水平分带常表现为从侵入岩体经矽卡岩往碳酸盐围岩方向依次出现侵入岩→同化混染侵入岩→富铁矽卡岩→富钙矽卡岩→同化混染碳酸盐岩→碳酸盐岩,反映同化混染作用逐渐减弱,而异地矽卡岩的水平分带常表现为从矽卡岩体中央往两边依次出现中粗粒矽卡岩－中细粒矽卡岩,反映随降温速度逐渐增加结晶速度逐渐降低。在矿物组成上,原地矽卡岩中的石榴石包含钙铁榴石、钙铁铝榴石和钙铝榴石,辉石主要为透辉石和钙铁辉石,而异地矽卡岩中的石榴石几乎全是钙铁榴石,辉石全是钙铁辉石。在地球化学方面,相对于原地矽卡岩,异地矽卡岩明显富集W、F、Rb、Be、Fe,而亏损Al、Sr、Ba、Cu、Pb、Zn、Cr、Co、Ni等元素。在岩相学上,原地矽卡岩和异地矽卡岩大多具有自形等粒结构,其中大多能见到熔融包裹体,但原地矽卡岩中的石榴石和辉石更为自形且常发育良好环带,熔融包裹体的均一温度明显高于异地矽卡岩中熔融包裹体的均一温度。在矿床类型上,原地矽卡岩一般为铜矿床,矿石矿物主要是铜铁硫化物,而异地矽卡岩一般为铁矿床,矿石矿物主要是铁氧化物。通过综合分析,认为原地矽卡岩和异地矽卡岩是由矽卡岩岩浆在原地或异地发生冷却结晶作用形成的,而原地矽卡岩矿床和异地矽卡岩矿床是由原地矽卡岩岩浆和异地矽卡岩岩浆发生熔离作用和结晶分异作用,熔离出的矿浆和分异出的热液发生冷却结晶和交代蚀变作用形成的。  相似文献   

20.
A number of trace elements have been determined spectrographically in the rocks and minerals of the Skaergaard intrusion, East Greenland. The original basic magma from which the varied rocks of the complex were developed is shown to have had a normal trace element composition. The sorting out of the trace elements into the various mineral series produced by strong fractional crystallization of the original basic magma is traced in detail by means of analyses of the separated minerals. Certain of the trace elements (Cr, Ni) are shown to be strongly concentrated in the early rocks so that later fractions have little or none of them; other elements (P, V, Cu, Sc, Mn, S) reach maximum values in the middle, or late middle stages represented by certain olivine-free gabbros and ferrogabbros; other elements (Li, Zr, Y, La, Ba, Rb) tend to remain in the residual liquid during fractionation and are thus abundant in the latest granite fraction. Still other trace elements (Co, Sr, Ga, Mo) show only small changes in amount throughout the series. Of these Co is a little more abundant in the early and middle stages, Sr in the middle stages, Ga in the later stages and Mo in the early and later but not in the middle stages. The distribution of the trace elements in the rocks is considered in relation to the varying composition of the minerals produced by the fractional crystallization processes and an attempt is made to discuss the mineral compositions in terms of crystal chemical concepts.The Skaergaard sequence of differentiation from gabbros, through ferrogabbros, to granite is considered to be a common trend of fractionation of basic magma at high levels in the crust, and the observed changes in trace element composition are therefore regarded as having wide geochemical significance. The trace element composition of the intermediate Skaergaard differentiates is significantly different from that of diorites reported by other workers and suggests that diorites have had some other origin than by fractionation of basic magma. On the other hand the trace element composition of many granites resembles that of the granite fraction produced in the Skaergaard intrusion.  相似文献   

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