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141.
Robin W. Renaut R. Bernhart Owen Tim K. Lowenstein Gijs De Cort Emma Mcnulty Jennifer J. Scott Anthony Mbuthia 《Sedimentology》2021,68(1):108-134
Saline alkaline lakes that precipitate sodium carbonate evaporites are most common in volcanic terrains in semi‐arid environments. Processes that lead to trona precipitation are poorly understood compared to those in sulphate‐dominated and chloride‐dominated lake brines. Nasikie Engida (Little Magadi) in the southern Kenya Rift shows the initial stages of soda evaporite formation. This small shallow (<2 m deep; 7 km long) lake is recharged by alkaline hot springs and seasonal runoff but unlike neighbouring Lake Magadi is perennial. This study aims to understand modern sedimentary and geochemical processes in Nasikie Engida and to assess the importance of geothermal fluids in evaporite formation. Perennial hot‐spring inflow waters along the northern shoreline evaporate and become saturated with respect to nahcolite and trona, which precipitate in the southern part of the lake, up to 6 km from the hot springs. Nahcolite (NaHCO3) forms bladed crystals that nucleate on the lake floor. Trona (Na2CO3·NaHCO3·2H2O) precipitates from more concentrated brines as rafts and as bottom‐nucleated shrubs of acicular crystals that coalesce laterally to form bedded trona. Many processes modify the fluid composition as it evolves. Silica is removed as gels and by early diagenetic reactions and diatoms. Sulphate is depleted by bacterial reduction. Potassium and chloride, of moderate concentration, remain conservative in the brine. Clastic sedimentation is relatively minor because of the predominant hydrothermal inflow. Nahcolite precipitates when and where pCO2 is high, notably near sublacustrine spring discharge. Results from Nasikie Engida show that hot spring discharge has maintained the lake for at least 2 kyr, and that the evaporite formation is strongly influenced by local discharge of carbon dioxide. Brine evolution and evaporite deposition at Nasikie Engida help to explain conditions under which ancient sodium carbonate evaporites formed, including those in other East African rift basins, the Eocene Green River Formation (western USA), and elsewhere. 相似文献
142.
新疆喀拉通克铜镍硫化物矿床成矿岩浆作用过程 总被引:3,自引:2,他引:3
喀拉通克铜镍硫化物矿床3个主要含矿镁铁质岩体的主量元素、微量元素和铂族元素组成分析及母岩浆组成估算结果表明:3个岩体中不同类型岩石的主要氧化物含量的变化具玄武质岩浆结晶分异的特征;在MgO含量为10%~15%区间,SiO2含量迅速增高;微量元素和稀土元素原始地幔标准化配分模式相似,具Nb和Ta亏损,K、Sr富集的特征.与1号和2号岩体相比,3号岩体中大离子亲石元素及轻稀土元素相对富集,(La/Yb)N介于6.8~9.2之间,δEu显示轻微负异常,在460 m深度表现出Cu-Ni等成矿元素与SiO2含量同时剧变的特征,铂族元素配分模式与2号岩体相似.上述结果显示,3个岩体可能是同源岩浆不同期次的产物,原始岩浆为高镁玄武岩浆.成矿岩浆演化过程中经历的岩浆分离结晶作用和富硅地壳组分混染可能是成矿岩浆硫饱和及硫化物熔离的主要诱因. 相似文献
143.
东昆仑祁漫塔格地区构造岩浆作用与成矿关系初步探讨 总被引:4,自引:0,他引:4
以钾、钠含量变化为主要指标获取祁漫塔格地区各个地史时期花岗岩类的成因类型.结果表明,区内构造岩浆作用在时间上具有明显的阶段性,加里东中晚期是本区第一次侵入岩浆作用的高峰期,印支中晚期为本区花岗岩浆作用的鼎盛时期,加里东中晚期和印支中晚期也是区内两次区域成矿作用的大爆发期.岩体分布具有明显的方向性.主要由北东向和北西向两... 相似文献
144.
Precambrian metaplutonic rocks of the São Gabriel block in southernmost Brazil comprise juvenile Neoproterozoic calc-alkaline gneisses (Cambaí Complex). The connection with associated (ultra-)mafic metavolcanic and metasedimentary rocks (Palma Group) is not well established. The whole complex was deformed during the Brasiliano orogenic cycle. Both metasedimentary and metavolcanic rocks as well as metaplutonic rocks of the Cambaí Complex have been sampled for geochemical analyses in order to get constraints on the tectonic setting of these rocks and to establish a tectonic model for the São Gabriel block and its role during the assembly of West-Gondwana. The major element compositions of the igneous rocks (Palma Group and Cambaí Complex) indicate a subalkaline character; most orthogneisses have a calc-alkaline chemistry; many metavolcanic rocks of the Palma Group show signatures of low-K tholeiitic volcanic arc basalts. Trace element data, especially Ti, Zr, Y, Nb, of most igneous samples from both the lower Palma Group and the Cambaí Complex indicate origin at plate margins, i.e., in a subduction zone environment. This is corroborated by relative enrichment in LREE, low contents of Nb and other high field strength elements and enrichment in LILE like Rb, Ba, and Th. The data indicate the possible existence of two suites, an oceanic island arc and a continental arc or active continental margin. However, some ultramafic samples of the lower Palma Group in the western São Gabriel block indicate the existence of another volcanic suite with intra-plate character which possibly represents relics of oceanic island basalts (OIB). Trace element data indicate contributions from andesitic to mixed felsic and basic arc sources for the metasedimentary rocks. The patterns of chondrite- and N-MORB-normalized spider diagrams resemble the patterns of the igneous rocks, i.e., LILE and LREE enrichment and HFS depletion. The geochemical signatures of most igneous and metasedimentary samples and their low (87Sr/86Sr)t ratios suggest only minor contribution of old continental crust.A geotectonic model for the São Gabriel block comprises east-ward subduction and following accretion of an intra-oceanic island arc to the eastern border of the Rio de la Plata Craton at ca. 880 Ma, and westward subduction beneath the newly formed active continental margin between ca. 750 and 700 Ma. The São Gabriel block represents relics of an early Brasiliano oceanic basin between the Rio de la Plata and Kalahari Cratons. This ocean to the east of the Rio de la Plata Craton might be traced to the north and could possibly be linked with Neoproterozoic juvenile oceanic crust in the western Brasília belt (Goiás magmatic arc). 相似文献
145.
太行山南段中生代杂岩体的岩石成因:元素和Nd-Sr-Pb同位素地球化学证据 总被引:13,自引:0,他引:13
通过太行山南段三个中生代杂岩体(西戌、武安和洪山)的元素和同位素地球化学特征的研究。讨论其成因和地球动力学环境。结果表明,西戌和武安杂岩体主要由从二长辉长岩到二长岩的一系列岩石组成,其地球化学性质相似(高Mg^s,具微弱至正Eu异常的REE模式等)。西戊杂岩体的εNd(135Ma)=-12.3~-16.9,Isε=0.7056~0.7071,与武安杂岩体稍有不同。西戌杂岩体的(^206Pb/^204Pb)i=16.92~17.3,(^207Pb/^204Pb)i=15.32~15.42,(^208Pb/^201Pb)i=37.16~37.63,较武安杂岩体的略高。西戊-武安杂岩体都起源于EM1型富集地幔,但被下地壳物质不同程度混染。洪山杂岩体(正长岩-花岗岩)也来自EM1型富集地幔的部分熔融,但属于不同的岩浆事件,并仅受轻微的下地壳混染。太行山岩浆作用的发生可能与古太平洋板块的水平俯冲消减而形成的弧后伸展环境有关。 相似文献
146.
近年来相继在嫩江多宝山地区发现了一系列晚三叠世岩浆岩。但该期岩浆活动的构造背景、成因机制及成矿作用迄今尚未得到很好的解读,这些问题对深入理解该地区构造演化、寻找多金属矿产具有重要意义。本文以多宝山矿区英云闪长岩、争光矿区闪长岩为研究对象进行系统的岩石学、地球化学及同位素年代学研究。锆石的LA-ICP-MS定年结果表明,多宝山英云闪长岩形成时代为(226.3±2.3) Ma,争光闪长岩形成时代为(229.3±3.1) Ma,两者在误差范围内一致,可能是同一岩浆房演化的产物。地球化学特征显示,多宝山英云闪长岩以高SiO2(64.25%~66.44%)、Al2O3(16.54%~17.21%)、K2O+Na2O(8.16%~8.49%),低CaO(2.27%~2.95%)、MgO(0.99%~1.16%)、TiO2(0.31%~0.36%)、P5O2(0.16%~0.17%)为特征;争光闪长岩以SiO2(57.12%~58.5%)、Al2O3(14.59%~15.26%)、(Na2O+K2O)(5.34%~6.16%)、 TiO2(0.83%~0.97%)、P2O5(0.15%~0.27%)及TFeO/MgO(1.12~1.25)相近为特征;多宝山英云闪长岩亏损Rb、Nb、Sm,富集Ba、U、Zr和Sr,Eu正异常明显(δEu=1.21~1.57),争光闪长岩Rb、Nb、Sm亏损,Ba、Th、Sr、Hf富集,Eu弱正异常(δEu=0.93~1.22)。二者富集轻稀土元素(LREE),亏损重稀土元素(HREE),稀土及微量曲线形态近似,显示同一源区的特征,原始岩浆起源于受俯冲流体交代的地幔楔的部分熔融,形成于与蒙古—鄂霍茨克洋板块俯冲有关的活动大陆边缘环境。多宝山矿集区晚三叠世钙碱性岩浆岩的确定指示蒙古—鄂霍茨克洋俯冲作用可影响到兴安地块东缘。综合区域晚三叠世矿床成矿时代及成矿背景,证实多宝山地区晚三叠世岩浆活动具有较强的银铜钼成矿能力,成矿潜力巨大。 相似文献
147.
Volcanism in the Vitim Volcanic Field, Siberia: Geochemical Evidence for a Mantle Plume Beneath the Baikal Rift Zone 总被引:5,自引:1,他引:5
JOHNSON J. S.; GIBSON S. A.; THOMPSON R. N.; NOWELL G. M. 《Journal of Petrology》2005,46(7):1309-1344
The Baikal Rift is a zone of active lithospheric extension adjacentto the Siberian Craton. The 616 Myr old Vitim VolcanicField (VVF) lies approximately 200 km east of the rift axisand consists of 5000 km3 of melanephelinites, basanites, alkaliand tholeiitic basalts, and minor nephelinites. In the volcanicpile, 142 drill core samples were used to study temporal andspatial variations. Variations in major element abundances (e.g.MgO = 3·314·6 wt %) reflect polybaric fractionalcrystallization of olivine, clinopyroxene and plagioclase. 87Sr/86Sri(0·70390·7049), 143Nd/144Ndi (0·51270·5129)and 176Hf/177Hfi (0·28290·2830) ratiosare similar to those for ocean island basalts and suggest thatthe magmas have not assimilated significant amounts of continentalcrust. Variable degrees of partial melting appear to be responsiblefor differences in Na2O, P2O5, K2O and incompatible trace elementabundances in the most primitive (high-MgO) magmas. Fractionatedheavy rare earth element (HREE) ratios (e.g. [Gd/Lu]n > 2·5)indicate that the parental magmas of the Vitim lavas were predominantlygenerated within the garnet stability field. Forward major elementand REE inversion models suggest that the tholeiitic and alkalibasalts were generated by decompression melting of a fertileperidotite source within the convecting mantle beneath Vitim.Ba/Sr ratios and negative K anomalies in normalized multi-elementplots suggest that phlogopite was a residual mantle phase duringthe genesis of the nephelinites and basanites. Relatively highlight REE (LREE) abundances in the silica-undersaturated meltsrequire a metasomatically enriched lithospheric mantle source.Results of forward major element modelling suggest that meltingof phlogopite-bearing pyroxenite veins could explain the majorelement composition of these melts. In support of this, pyroxenitexenoliths have been found in the VVF. High Cenozoic mantle potentialtemperatures (1450°C) predicted from geochemical modellingsuggest the presence of a mantle plume beneath the Baikal RiftZone. KEY WORDS: Baikal Rift; mafic magmatism; mantle plume; metasomatism; partial melting 相似文献
148.
巴尔哲超大型稀有稀土矿床成矿机制研究 总被引:7,自引:2,他引:7
巴尔哲矿床中的矿化和非矿化碱性花岗岩主要造岩矿物均为微斜长石、石英、钠闪石和钠长石,但其相对含量及颗粒大小明显不同,且两类岩石中包裹体的组成特征及锆石的结晶习性也有显著差异.主量元素分析显示,矿化与非矿化碱性花岗岩均以富硅、富碱、贫镁和钙为特征,为较典型的非造山A型花岗岩.尽管矿化碱性花岗岩中K_2O和Na_2O的含量均没有明显的增加,但其Na+K/Al、Na_2O+K_2O/CaO、FeO~*/MgO及K_2O/MgO等岩石化学参数与非矿化碱性花岗岩明显不同.在矿化碱性花岗岩中除了矿化的稀土元素及Nb、Zr强烈富集外,U、Th及Y也明显富集,而Ba、Sr、P、Eu和Ti表现为强烈的亏损.在非矿化碱性花岗岩中除了大离子亲石元素Rb略有富集外,稀土元素、Nb、Zr、U、Th、Ta及Y并无明显富集,虽然Sr、P、Eu和Ti也表现为亏损,但与矿化碱性花岗岩相比其亏损程度明显降低.岩相学、岩石化学及微量元素地球化学特征显示,矿化碱性花岗岩不可能是非矿化碱性花岗岩硅化和钠长石化作用的产物,二者应是同一岩浆体系不同演化阶段熔体固结的产物.K/Rb、Rb/Sr及δEu等地球化学参数显示,矿化碱性花岗岩是高演化A型花岗质熔体固结的产物;而岩石学、包裹体及地球化学特征则显示,这种高演化的A型花岗质熔体已经进入了岩浆一热液过渡阶段.巴尔哲矿床稀有稀土元素的超常富集和成矿与A型花岗岩的高演化过程密切相关. 相似文献
149.
江西安远路迳金伯利质煌斑岩筒研究——一种新型的幔源碱性超基性岩 总被引:1,自引:0,他引:1
路迳岩筒属火山通道相,由金伯利质煌斑岩、角砾岩、角砾凝灰岩组成,富含幔源橄榄岩包体、普通辉石巨晶和岩球。造岩矿物是橄榄石、斜方辉石、单斜辉石、角闪石和金云母,深源特征指示矿物有镁铝榴石、铬透辉石、铬尖晶石和镁钛铁矿。岩石化学组成超低SiO2,低MgO,高Al2O3,富碱,富挥发组分。轻稀土元素富集,相容元素贫化,不相容元素明显富集。岩浆起源深度约85km。其中:岩体产状,富含包体、巨晶和岩球,岩石结构和构造,矿物组成,岩石化学组成超低SiO2、富碱、富挥发组分等特征与金伯利岩相似;但岩石化学组成高Al2O3,低MgO,K2O低于Na2O,REE和LREE/HREE偏低,部分微量元素的亏损或富集,金云母成分富TiO2,富TFeO,贫MgO,镁铝榴石、铬透辉石、铬尖晶石和镁钛铁矿的Cr2O3含量偏低,岩浆起源深度较浅,均与金伯利岩有重大差异,而更接近煌斑岩类。研究认为,是幔源岩浆岩的一种新类型,岩石名称界定为金伯利质煌斑岩。 相似文献
150.