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1.
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   

2.
孙洋  马昌前  刘彬 《地球科学》2017,42(6):891-908
江苏省宁镇地区位于长江中下游沿江成矿带的最东端,是长江中下游成矿带的重要组成部分,蒋庙岩体是宁镇地区唯一的基性岩体.对此岩体进行了锆石U-Pb年代学、矿物化学、岩石地球化学和Sr-Nd-Hf同位素研究,讨论了其成因及地幔源区性质.岩体主要由橄榄辉长岩、角闪辉长岩和辉石闪长岩组成,其中辉石闪长岩的锆石LA-ICP-MS(laser ablation inductively coupled plasma mass spectrometry) U-Pb年龄为121±1 Ma.锆石εHf(t)值介于-2.9~-6.4.全岩地球化学研究显示岩石样品富钠低钾,富集轻稀土元素,重稀土元素亏损不明显,富集大离子亲石元素(如K、Ba、Sr等),亏损高场强元素(如Nb、Ta、Ti、Zr、Hf等).蒋庙基性侵入岩在长江中下游地区中生代岩浆岩中具有最高的εNd(t)值以及最低的(87Sr/86Sr)i值,其Sr-Nd同位素组成介于软流圈地幔(depleted MORB mantle,DMM)-富集岩石圈地幔(enriched mantle Ⅱ,EMⅡ)之间.研究认为,蒋庙岩体应来源于软流圈地幔和富集岩石圈地幔的混合组分,可能有少量的俯冲板片物质加入源区,并在成岩过程中经历了一定程度的结晶分异.结合区域地质、年代学、矿物学和地球化学资料,表明蒋庙岩体的形成可能与古太平洋板块俯冲事件密切相关.   相似文献   

3.
高家村岩体辉长岩-橄榄岩中矿物组合、矿物结晶顺序及岩浆成因角闪石的普遍出现,指示矿物结晶于富含水的岩浆体系.主量元素Al2O3、CaO与MgO呈明显的负相关关系,表明斜长石并非早期堆晶相.稀土元素含量为5.97×10-6～221.32×10-6,轻稀土元素相对富集,弱-中等程度轻重稀土元素分异,辉长岩-含辉石闪长岩无明显的Eu异常,而橄榄辉长岩-橄榄岩具有较明显的正Eu异常.微量元素中,辉长岩-含辉石闪长岩类具有明显的Nb、Ta、Zr、Hf和Ti负异常,Ba、Sr正异常,同时εNd(t)为0.59～1.86,低于同期的亏损地幔值,与岛弧基性岩浆特征类似.含辉石闪长岩SHRIMP锆石U-Pb年龄结果822±8Ma,为新元古代.综合分析认为,高家村岩体应形成于受俯冲带流体改造的亏损上地幔部分熔融.  相似文献   

4.
赵磊  吴泰然  罗红玲 《岩石学报》2011,27(10):3071-3082
内蒙古乌拉特中旗温更地区北七哥陶辉长岩岩体由橄榄辉长岩和角闪辉长岩组成,主要造岩矿物为橄榄石、辉石、斜长石及角闪石等.锆石SHRIMP U-Pb同位素定年结果表明,橄榄辉长岩形成于269±8Ma,为晚古生代华北板块北缘岩浆活动的产物.橄榄辉长岩和角闪辉长岩具有相似的稀土元素、微量元素以及同位素特征,即:轻稀土元素( LREE)富集的右倾平滑配分模式;大离子亲石元素(LILE)K、Sr、Ba明显富集,高场强元素(HFSE) Nb、Ta、U、Th相对亏损,但Zr-Hf不亏损;87Sr/86Sr(t)平均值分别为0.706776和0.706960,εNd(t)平均值分别为-8.8和-8.9,206pb/204Pb、207pb/204Pb、208Pb/204Pb比值的平均值分别为17.2019和17.2277、15.4252和15.4524、37.3082和37.4724,在s7 Sr/86Sr(t)-143Nd/144 Nd (t)图解上,北七哥陶辉长岩都落在了EMI型富集地幔附近.根据以上事实,结合区域资料表明,橄榄辉长岩和角闪辉长岩产于后碰撞的构造环境,并且来自相同的岩浆源区,主要继承了华北陆块内部EMI型富集地幔,可能受到了古亚洲洋俯冲消减过程中再循环下地壳组分对岩石圈地幔的改造.  相似文献   

5.
太行山南段平顺杂岩体主要由橄榄角闪辉长岩,角闪辉长-闪长岩和闪长岩组成,锆石SHRIMP U-Pb测年显示,橄榄角闪辉长岩体和闪长岩体年龄分别为123.4±1.7 Ma和125.3±2.3 Ma,说明岩体形成于早白垩世。平顺杂岩体SiO2含量介于42.82%~63.54%之间,以高Mg#,富Na,高Sr、Cr、Ni,以及富集LILE、LREE,亏损HFSE、HREE为特点,并具有相对低的87Sr/86Sr初始比值和明显偏低的εNd(125 Ma)值,表明岩浆具有壳幔双重属性。结合辉长岩中地幔包体已有的研究成果,认为辉长岩是由富硅流体交代的亏损地幔橄榄岩经低程度部分熔融形成;高Mg闪长岩起源于下地壳部分熔融,并与一定规模的幔源岩浆发生混合;角闪辉长-闪长岩形成于辉长质岩浆与高Mg闪长质岩浆的混合作用。  相似文献   

6.
牛鼻子梁岩体位于柴达木地块的北缘,出露面积约8 km2,平面形态呈长条状,主要由斜长二辉橄榄岩、斜长单辉橄榄岩、角闪二辉橄榄岩、角闪橄榄岩、角闪橄榄二辉岩、黑云母化二辉岩、角闪辉石岩、橄榄辉石角闪石岩、角闪橄榄辉长岩、细粒辉长岩、似斑状辉长岩、暗色辉长岩、辉长岩、淡色辉长岩、石英闪长岩和英云闪长岩组成。文章通过岩石学、矿物学、地球化学研究,得到锆石U-Pb年龄为(361.5±1.2)Ma,Sm-Nd等时线年龄为(347±26)Ma。研究认为,牛鼻子梁基性-超基性岩体含矿岩石产于大陆边缘环境。岩体形成于泥盆纪晚期。岩浆分异充分,岩石类型丰富,岩浆演化过程中主要发生了橄榄石和斜长石的分离结晶/堆晶作用。岩体的母岩浆应属于拉斑玄武岩质岩浆。从目前发现的矿化情况来看,牛鼻子梁基性-超基性杂岩体为含矿岩体,有很好的找矿前景。  相似文献   

7.
周口店岩体由三次侵入的中酸性岩石组成, 本次测得石英闪长岩锆石U-Pb年龄为131.6±2.1 Ma, 闪长玢岩锆石U-Pb年龄为128.1±1.4 Ma.周口店岩体各种类型岩石属高钾钙碱性系列、偏铝质, Mg#较高, 重稀土元素和Ta、Nb、P以及Ti明显亏损, 轻稀土元素和Ba、K以及Sr相对富集, Eu没有异常, Yb元素含量小于2×10-6, (La/Yb)N和Sr/Y比值较高.斜长石复杂环带能谱线扫描表明, 花岗闪长岩中的斜长石核部牌号高, 完整的幔部由内向外由反环带和正环带组成, 微粒包体中的斜长石核部牌号低, 幔部以尘状环带开始, 然后演变为正环带, 这揭示存在多期基性岩浆的注入作用, 结合暗色微粒包体的形态、大小、数量、反向脉、矿物含量统计、矿物成分、地球化学和各类环带包体、岩墙状包体群等特征, 说明暗色微粒包体是在花岗闪长岩浆冷凝过程的不同阶段, 多期幔源基性岩浆注入并与酸性岩浆在围绕包体周缘的局部范围内发生不均一机械混合作用的结果.周口店中酸性岩石体现埃达克质岩的地球化学特征, 岩浆成分主要受源区控制, 形成于加厚下地壳环境.由石英闪长岩-花岗闪长岩至中酸性岩脉, 岩石(Er/Lu)N和Nb/Ta比值升高, 说明源区残留相矿物组合由角闪石+石榴石向石榴石+金红石变化, 岩浆源区不断变深.   相似文献   

8.
牛鼻子梁镁铁质-超镁铁质杂岩体岩石特征   总被引：1，自引：1，他引：0  
牛鼻子梁岩体位于柴达木地块的北缘,出露面积约8 km2,平面形态呈长条状,主要由斜长二辉橄榄岩、斜长单辉橄榄岩、角闪二辉橄榄岩、角闪橄榄岩、角闪橄榄二辉岩、黑云母化二辉岩、角闪辉石岩、橄榄辉石角闪石岩、角闪橄榄辉长岩、细粒辉长岩、似斑状辉长岩、暗色辉长岩、辉长岩、淡色辉长岩、石英闪长岩和英云闪长岩组成。文章通过岩石学、矿物学、地球化学研究,得到锆石U-Pb年龄为（361.5±1.2） Ma,Sm-Nd等时线年龄为（347±26） Ma。研究认为,牛鼻子梁基性-超基性岩体含矿岩石产于大陆边缘环境。岩体形成于泥盆纪晚期。岩浆分异充分,岩石类型丰富,岩浆演化过程中主要发生了橄榄石和斜长石的分离结晶/堆晶作用。岩体的母岩浆应属于拉斑玄武岩质岩浆。从目前发现的矿化情况来看,牛鼻子梁基性-超基性杂岩体为含矿岩体,有很好的找矿前景。  相似文献   

9.
位于东天山黄山岩带最东端的四顶黑山镁铁质-超镁铁质层状杂岩体规模较大,呈北东向展布,可分为南、北2个岩体。主要岩石类型有单辉橄榄岩、橄榄辉石岩、橄榄苏长辉长岩、橄榄辉长岩、辉石角闪岩、辉长岩和角闪辉长岩,超镁铁岩相常与辉长岩相呈韵律互层。主量元素化学组成主要属拉斑玄武岩系列。岩石稀土元素配分曲线呈平坦型以及Eu的正异常,普遍富集大离子亲石元素(Rb、Ba、U),显示明显的Sr正异常以及Nb、Ta的亏损。通过橄榄石最高的Fo值(79.6)估算出母岩浆中MgO和FeO含量分别为6.23%和6.60%。岩浆在演化过程中发生了橄榄石、斜方辉石、单斜辉石、斜长石的分离结晶/堆晶作用以及较弱的上地壳同化混染作用。岩石高的(La/Yb)N值1.550和1.744值表明岩浆源区的深度可能大于90km;Th/U值特征以及Th/Yb-Nb/Yb和La/Ba-La/Nb图解表明,四顶黑山岩体的岩浆源区可能为受俯冲作用改造的岩石圈地幔。  相似文献   

10.
天宇和白石泉铜镍矿区含矿镁铁-超镁铁质杂岩体是东疆铜镍成矿带的重要组成部分。天宇矿区杂岩体以角闪辉长岩、角闪单辉橄榄岩、橄榄辉石岩、二辉辉石岩为主;白石泉矿区杂岩体则以辉石闪长岩、角闪辉长岩、橄榄辉石岩、辉石辉长岩、辉石橄榄岩、橄长岩为主;天宇矿区含矿超基性岩中SiO2,Al2O3,CaO,K2O,Na2O的质量分数比白石泉岩体低,Fe2O3,MgO相对较高;两个杂岩体的主要造岩矿物均以橄榄石、辉石、斜长石为主;铜镍矿石的矿物组成都较简单,金属矿物种类基本一致;两个杂岩体基性-超基性岩的成分接近原始岩浆,均来自于地幔,均属含铜镍中等的镁铁质岩石。  相似文献   

11.
Wadi El-Markh gabbro–diorite complex is composed of pyroxene hornblende gabbros, hornblende gabbros, diorites and quartz diorites. According to their bulk rock geochemistry and mineral chemistry, the gabbroic and dioritic rocks represent fractionates along a single line of descent and crystallized from a calc-alkaline mafic magma. When compared to the primitive mantle, all members of the gabbroic–dioritic rock suite are enriched in the large ion lithophile elements relative to the high field strength elements and display distinctive negative Nb and P2O5 anomalies. This signals an arc setting. Fractionation modeling involving the major elements reveals that the hornblende gabbros were generated from the parent pyroxene hornblende gabbros by 61.86% fractional crystallization. The diorites were produced from the hornblende gabbros by fractional crystallization with a 58.97% residual liquid, whereas the quartz diorites were formed from the diorites by 26.58% fractional crystallization. According to geothermobarometry based on amphibole mineral chemistry, the most primitive pyroxene hornblende gabbros crystallized at ～830 °C/～5 kbar. The crystallization conditions of the quartz diorites were estimated at ～570 °C/～2 kbar. In consequence the Wadi El-Markh gabbro–diorite complex represents a single magmatic suite of which fractionates crystallized in progressively shallower levels of an arc crust.  相似文献   

12.
Important mafic–ultramafic masses have been located for the first time in the intersection area between the Keraf Shear Zone and the Nakasib Suture Zone of the Nubian Shield. The masses, comprising most of the members of the ophiolite suite, are Sotrebab and Qurun complexes east of the Nile, and Fadllab complex west of the Nile. The new mafic–ultramafic masses are located on the same trend of the ophiolitic masses decorating the Nakasib Suture. A typical complete ophiolite sequence has not been observed in these complexes, nevertheless, the mafic–ultramafic rocks comprise basal unit of serpentinite and talc chlorite schists overlain by a thick cumulate facies of peridotites, pyroxenites and layered gabbros overlain by basaltic pillow lavas with dolerite dykes and screens of massive gabbros. Associated with pillow lavas are thin layers of carbonates and chert. The best section of cumulate mafic–ultramafic units has been observed in Jebel Qurun and El Fadlab complexes, comprising peridotites, pyroxenites and layered gabbros. Dolerite dykes and screens of massive gabbros have been observed with basaltic pillow lava sections in Wadi Dar Tawaiy. The basal ultramafic units of the complexes have been fully or partly retrograded to chlorite magnetite schist and talc to talc-carbonate rocks (listowenites), especially in the Jebel Qurun and Sotrebab complexes. Petrographically, the gabbros (layered and massive) and the basaltic pillow lavas show mineral assemblages of epidote amphibolite facies. The mafic members from the three complexes show a clear tholeiitic trend and oceanic floor affinity. The pillow lavas plot in the field of oceanic floor basalt, namely in the back arc field. Primitive mantle normalized spider diagram of the pillow lavas reveals a closer correspondence to Enrich-Mid-Oceanic Ridge Basalt (E-MORB) type, which is confirmed by the flat chondrite normalized Rare Earth Elements (REE) pattern. Field, petrographical and geochemical evidence supports ophiolitic origin of the three complexes. The newly discovered ophiolitic complexes mark the western continuation of the Nakasib Suture Zone.  相似文献   

13.
Rocks of the Moruya Batholith range from gabbros and gabbroic diorites through quartz diorites and tonalites to granodiorites and rare adamellites. The gabbros and gabbroic diorites appear as small, early bodies intruded and enclosed by quartz diorites and tonalites. These early gabbroids are petrographically and chemically distinct from the granitoids. The latter occur as a meridionally‐oriented sequence of nine separate plutons. Mafic xenoliths are most abundant in the quartz diorites and tonalites; they are petrographically similar to their host granitoids and are chemically a more mafic extension of the variation in granitoid compositions. The various granitoid bodies are considered to be derived from similar source rocks, with the xenoliths representing modified material relict from partial melting of that source.

Comparison of chemical data from the Moruya granitoids with those of the I‐types of the Jindabyne Suite in the Kosciusko Batholith, shows that the potassium content is indistinguishable in the two suites from each side of the Moruya‐Kosciusko Province, although elsewhere it has been shown to vary systematically across an orogenic belt. The most outstanding difference is the higher Na and Ti and lower Ca in the Moruya Batholith compared with those in Kosciusko Batholith I‐type granitoids.  相似文献   

14.
The lower crust of the Mesozoic Sierra Nevada batholith was made up of high MgO, garnet-poor and low MgO, garnet-rich pyroxenites. Both groups are genetically linked and are collectively complementary to the mafic to intermediate Sierran plutons. High MgO pyroxenites represent high pressure cumulates from a mantle-derived hydrous basalt or basaltic andesite, resulting in derivative magmas having unusually low MgO for a given SiO2 as represented by the numerous mafic enclaves found in many Sierran plutons. The low MgO pyroxenites are either (1) shallow pressure cumulates from these derivative magmas or (2) partial melting residues (restites) of these derivative magmas after they were emplaced and solidified at lower crustal levels. In both cases, the complementary melt to the low MgO pyroxenites is driven to higher SiO2 contents, generating diorites and granodiorites. However, this simple two-stage scenario for the origin of Sierran granitoids cannot explain the observation that the Mg# of Sierran intermediate magmas remains roughly constant at ∼0.45–0.50 with increasing SiO2. Basaltic recharge/mixing with the lower crust is suggested as one means of buffering Mg#s and re-melting the lower crust to generate granitic melts, the latter of which mix with more juvenile magmas to complete the Sierran differentiation series.  相似文献   

15.
The Monteregian Hills consist of a series of alkaline intrusionsand associated dikes and sills emplaced along a linear west-easttrend extending from 35 km west of Montreal, Quebec, to 190km east of Montreal. The igneous activity occurred between 117Ma and 141 Ma and the age data show a distinct bimodality, withstrongly undersaturated magmas emplaced at c. 118 Ma and slightlyundersaturated magmas emplaced at c. 136 Ma. The eastern intrusionslargely consist of gabbros, diorites, and a variety of felsicrocks as compared to the more mafic character of the westernintrusions which largely consist of pyroxenites, gabbros, anddiorites. The eastern intrusions were emplaced through a thicksequence of folded and faulted geosynclinal sediments whichseems to have played a role in determining their felsic character. Mounts Brome and Shefford are located approximately 80 km eastof Montreal. The dominant rock type at Mount Shefford is a dioritewhich has been intruded by arcuate bodies of pulaskite and nordmarkite.Mount Brome consists of an outer crescent-shaped gabbro body,composed of several cyclical units, and a large syenite bodydivided into a slightly quartz-undersaturated unit (pulaskite)and a slightly oversaturated unit (nordmarkite). The two unitsare chemically similar, but the nordmarkite has elevated initialSr ratios suggesting that crustal contamination is responsiblefor its oversaturation. Both complexes have been intruded bynepheline-bearing diorites, and at Mount Brome, foyaites, tinguaites,and laurdalites. Mount Megantic is located approximately 190km east of Montreal and consists of an outer normarkite annulus,separated by a gabbro-dioritic body from an inner granite plug. Five different magma types have been identified in the easternMonteregian Hills. Type 1, precursor to the gabbros and syenitesat Mounts Shefford and Brome, is an alkali picrite generatedby limited partial melting of a garnet lherzolite, with subsequentevolution controlled by the removal of olivine, pyroxene, andplagioclase. Type 2, precursor to the gabbros and nordmarkitesat Mount Megantic, is apparently produced by moderate partialmelting of a spinel lherzolite, and this magma subsequentlyevolved to a quartz-saturated residuum. Type 3, which producedthe rocks of the strongly undersaturated series, is equivalentto the basanite magmas generated by small degrees of meltingof a spinel lherzolite, which formed similar rocks in the westernMonteregian Hills. The high concentration of incompatible elementsand high-charge-density cations in these magmas indicates thatthe mantle source regions were enriched in these elements. Type4, Mount Shefford nordmarkite, and Type 5, Mount Megantic granite,magmas apparently originated in the crust by partial meltingof, respectively, amphibolite or granulite facies metadioriteand metagraywacke sources.  相似文献   

16.
The ranges of the Sierras Valle Fértil-La Huerta expose natural cross sections through a paleo-arc crust that formed in the Late Cambrian - Early Ordovician Famatinian magmatic arc, northwestern Argentina. Thick mafic sequences of amphibole gabbronorites to orthopyroxene-amphibole-biotite diorites form the lower levels of the exposed paleo-arc section. This mafic unit includes lens-shaped bodies of olivine-bearing cumulate rocks and tabular-shaped sill/dike intrusions of fine-grained chilled amphibole gabbro. The mafic magmas were emplaced into regional metasedimentary sequences at lower crustal levels, corresponding to pressure from 5 to 7 kbar. Gabbronorites likely representing the parental magmas that fluxed into the exposed paleo-arc crust differ from primitive magmatic arc rocks in having somewhat lower Mg-number (ca. 0.60) and compatible (Cr and Ni) trace element contents, and slightly higher Al2O3 contents. This difference is taken to indicate that a pyroxene-rich olivine-bearing assemblage with a bulk high Mg/Fe ratio and low Al2O3 content crystallized from mantle-derived melts before mafic magmas reached the crustal levels currently exhumed. However, some gabbronorites have incompatible trace element signatures typical of primitive mafic arc magmatism. Igneous rocks to some extent more evolved than those of the mafic unit make up a tonalite-dominated intermediate unit. The intermediate unit consists of a heterogeneous suite that ranges from orthopyroxene-bearing amphibole-rich diorites to biotite-rich amphibole-poor tonalites. Within the intermediate unit, chilled mafic rocks are found as a network of dikes, whereas metasedimentary migmatites appear interlayered as m-wide septa and km-long strips. The tonalite-dominated intermediate unit passes into a granodiorite batholith through a transitional zone that is up to 2-km wide. The boundary zone separating the tonalite-dominated and granodiorite-dominated units is characterized by mingling of tonalitic and leucogranitic magmas, which together appear multiply-intruded by mafic sill/dike bodies. Within the tonalite- and granodiorite-dominated units, the less evolved mafic rocks occur as: (1) bodies tens of meters long, (2) chilled dikes and sills, and (3) microgranular inclusions (enclaves), supporting the inference that mafic magmatism was the main source for generating a vast volume of intermediate and silicic igneous rocks. Mass balance calculations and trace element systematics are combined to demonstrate that tonalites and granodiorites formed by concurrent closed-system fractional crystallization and open-system incorporation of paragneissic migmatites and/or anatectic leucogranites into the evolving igneous sequence. This study argues that the sequence of igneous rocks from Valle Fértil-La Huerta was formed as the result of complementary petrogenetic processes that operated concurrently at different levels of the Famatinian arc crust.  相似文献   

17.
Located in the northwestern part of the Charlotte terrane of the Carolina zone in central North Carolina, the Mocksville complex is a tabular body which trends NE-SW and covers an area of approximately 500?km2. It consists of late Proterozoic to early Paleozoic, moderately metamorphosed and variably deformed, mainly plutonic ultramafic, mafic and felsic rocks. The ultramafic rocks are pyroxenites, wehrlites, and hornblendites; the mafic rocks are metagabbros and amphibolites; and, the felsic rocks are granites and diorites. Field, geochemical, and geothermobarometry studies suggest that the igneous and metaigneous rocks of the Mocksville complex are likely to be genetically related, formed by calc-alkaline differentiation of mafic magma, and originated in a moderate pressure environment (~8?kbar). Based mainly on the study of volcanic rocks, the terranes of the Carolina zone have been interpreted as magmatic arc terranes in most tectonic models concerning the evolution of the southern Appalachian orogen. The geochemical features of the mafic and ultramafic plutonic rocks of the Mocksville complex corroborate the arc origin of the Charlotte terrane.  相似文献   

18.
Lower crustal xenoliths entrained in a Paleozoic ultramafic lamprophyre breccia pipe on Elovy island, Kola peninsula, Russia, represent some of the oldest lower crustal material yet investigated from Europe. The xenoliths vary from feldspar-poor, garnetrich rocks which resemble eclogites, to feldspar-rich garnet granulites. Quartz-rich felsic granulites, as well as pyroxenites and amphibole-rich rocks are also present.

The mafic granulites/eclogites represent a suite of gabbros and norites that is related by olivine fractionation. The igneous protoliths may have formed in a manner analogous to lower crustal rocks from most other European xenolith localities, i.e. by basaltic underplating, but magmatic cumulates are not in evidence.

The Kola lower crust was subjected to one or more metasomatic events which introduced up to 45% phlogopite and/or amphibole into both eclogites/granulites and pyroxenites. The resulting rocks have strong enrichments in Rb, Ba, and K, indicating that the lower crust is not uniformly depleted in LIL and heat-producing elements. Siliceous (65% SiO2) and mafic (< 50% SiO2) lithologies coexist in migmatitic xenoliths, which provide evidence for partial melting processes and restite formation in mafic metaigneous lower crust. The relationship, if any, between partial melting and metasomatism is unclear.  相似文献   


19.
Summary Suites of coarse-grained clasts (plutonic nodules) within the scoria of two separate mafic post-caldera parasitic vents, on Sete Cidades volcano, are described. These involve dunites, wehrlites, olivine clinopyroxenites, clinopyroxenites and olivine gabbros in the Eguas ankaramitic cone and pyroxene hornblendites, kaersutite gabbros and diorites in the Pico das Camarinhas basaltic-hawaiitic cone. The plutonic nodules are inferred to be cumulates, crystallised within the crust from magmas co-genetic with the post-caldera mafic lavas erupted on the flanks of Sete Cidades.The dunites, wehrlites, pyroxenites and olivine gabbros have assemblages and mineral composition consistent with growth as early, high-temperature cumulates, whereas the pyroxene hornblendites, kaersutite gabbros and diorites represent lower temperature products. However, whereas the kaersutite gabbros were not wholly crystallised at the time of their disruption and contain up to 4% intercumulus trachytic and/or tephriphonolitic glass, the pyroxene hornblendites and the diorites were fully crystallised. Compositions of the intercumulus glasses are similar to those of postcaldera trachytic pumices erupted on Sete Cidades.Although the two suites of plutonic clasts can be considered as complementary, they probably derive from different intrusions. We envisage a lensoid (laccolithic) intrusion at very shallow depth as the source for the pyroxene hornblendite - kaersutite gabbro -diorite suite whereas the dunite - wehrlite - olivine clinopyroxenite - clinopyroxenite -olivine gabbro nodules probably originate from intrusive bodies at greater depth.
Sub-vulkanische Kristallisation am Sete Cidades Vulkan, São Miguel, Azoren: Die Bedeutung mafischer und ultramafischer plutonischer Einschlüsse
Zusammenfassung Wir beschreiben Gruppen von grobkörnigen Klasten (Plutonic nodules) in der Scoria von zwei separaten mafischen post-caldera parasitischen Kratern am Sete Cidades Vulkan: Diese umfassen Dunite, Wehrlite, Olivin-Klinopyroxenite und Olivin-Gabbros in dem ankaramitischen Kegel von Eguas. In den basaltisch-hawaiitischen Kegeln von Pico das Camarinhas, kommen Pyroxen-Hornblendite, Kaersutit-Gabbros und Diorite vor. Wir nehmen an, daß die plutonischen nodules Kumulate repräsentieren, die in der Kruste aus Magmen kristallisierten, die mit den post-caldera mafischen Laven, die an den Flanken von Sete Cidades ausgetreten sind kogenetisch sind.Die Dunite, Wehrlite, Pyroxenite und Olivin-Gabbros führen Paragenesen und Mineral-Zusammensetzungen, die im Einklang mit einer Entwicklung als frühe Hoch Temperatur-Kumulate sind. Hingegen stellen die Pyroxen-Hornblendite, Kaersutit-Gabbros und Diorite niedriger temperierte Produkte dar. Die Kaersutit-Gabbros waren zur Zeit /:ihrer Umlagerung noch nicht ganz auskristallisiert und führen bis zu 4% intercumulus trachytisches oder tephriphonolitisches Glas, die Pyroxenhornblendite und die Diorite sind jedoch ganz kristallisiert. Die Zusammensetzungen der Interkumulusgläser sind denen von post-caldera trachytischen Bimssteinen von Sete Cidades ähnlich.Obwohl die zwei Gruppen plutonischer Klasten als komplementär betrachtet werden können, stammen sie wahrscheinlich von verschiedenen Intrusionen. Es dürfte sich um eine lensoide (lakkolithische) Intrusion in geringer Tiefe als Quelle für die Pyroxenhomblendit-Kärsutitgabbro-Diorit-Abfolge handeln, während die Gruppe der Dunite, Wehrlite, Olivinklinopyroxenite und Olivingabbro-Nodules wahrscheinlich aus größerer Tiefe stammt.

With 9 Figures  相似文献   

20.
The Wengeqi complex in Guyang County, Inner Mongolia, is one of several Pd–Pt-mineralized Paleozoic mafic–ultramafic complexes along the north-central margin of the North China. The complex comprises pyroxenites, biotite pyroxenites, amphibole pyroxenites, gabbros, and amphibolites. Zircons extracted from a pyroxenite yield a U–Pb SHRIMP age of 399?±?4?Ma. Several 2–6-m wide syngenetic websterite dikes contain 1–3?ppm Pd?+?Pd and are dominated by pyrite–chalcopyrite–pyrrhotite–magnetite–(pentlandite) assemblages with minor sperrylite, sudburyite, and kotuskite. Textural relationships indicate that pyrite has replaced magmatic chalcopyrite and that magnetite has replaced magmatic pyrrhotite. The mineralization is enriched in Pd–Pt–Cu > Au >> Rh–Ir–Os–Ni > Ru, similar to other occurrences of hydrothermally modified magmatic mineralization, but very different from the much less fractionated compositions of magmatic PGE mineralization. Textural, mineralogical, and geochemical relationships are consistent with alteration of an original magmatic Fe–Ni–Cu sulfide assemblage by a S-rich oxidizing high-temperature (deuteric) hydrothermal fluid.  相似文献   

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