内蒙古崇根山蛇绿岩中铬铁矿特征及其构造意义     

王成  任利民  张晓军  余国飞  方磊 《吉林大学学报(地球科学版)》2019,49(6):1552-1564

为探讨内蒙古贺根山蛇绿岩形成时的物化条件和大地构造环境,选取崇根山蛇绿岩块中未蚀变副矿物铬铁矿进行矿物学和矿物地球化学分析。结果表明：铬铁矿成分均一,不发育环带结构;铬铁矿中的Cr₂O₃质量分数为38.86%~39.12%,Al₂O₃质量分数为26.56%~26.92%,TFeO质量分数为17.37%~17.50%,Cr^#为49.34~49.58,Mg^#为68.82~69.73,Yfe为6.62~6.97,Fe^2+#为30.27~31.18,为富镁铝铬铁矿,其寄主岩石为蛇绿岩;铬铁矿结晶平均温度为1 396.88℃,平均压力为3.35 GPa,推断其形成深度约为103.72 km;相对于FMQ（fayalite magnetite quartz）缓冲剂的地幔氧逸度为FMQ+1.41~FMQ+1.45 lg单位（平均值为FMQ+1.43 lg单位）;地幔熔融程度为20.93%~20.95%（平均值为20.94%）。推测崇根山铬铁矿原岩橄榄岩单元源区为石榴石二辉橄榄岩,形成于亏损地幔。崇根山蛇绿岩为消减带型蛇绿岩,可能产自俯冲带环境中的洋内弧后盆地环境。  相似文献   

穆斯堡尔光谱仪在揭示地幔氧逸度研究中的应用     

王秋霞  平先权  郑建平  戴宏坤 《地球科学》2023,(3):1217-1231

利用地幔橄榄岩包体中平衡矿物对的氧逸度计可以有效限定岩石圈地幔的氧化-还原状态.本文使用中国地质大学(武汉)新购置的WSS-10型常温穆斯堡尔光谱仪对华北地块西北部狼山地区橄榄岩包体的四相矿物开展了铁价态的直接测定.结果显示,斜方辉石Fe³⁺/∑Fe为0.05～0.11,单斜辉石的为0.16～0.25,尖晶石的为0.16～0.22,橄榄石为0.利用橄榄石-斜方辉石-尖晶石氧逸度计,获得狼山地区岩石圈地幔氧逸度为FMQ-0.82至FMQ-0.39(均值为FMQ-0.65).该值略高于依据电子探针测试数据计算获得的氧逸度值(FMQ-1.49至FMQ-0.8,均值为FMQ-1.25),造成这一差异的原因可能是后者忽略了尖晶石晶格中Fe³⁺过剩和阳离子空位导致的非化学计量比.与全球克拉通岩石圈地幔氧逸度值(均值为FMQ-0.35)相比,华北地块西北缘狼山地区岩石圈地幔整体表现为较还原状态,推测与深部地幔低fO₂熔体上升交代有关.  相似文献   

东太平洋CC区玄武岩岩石成因：³⁹Ar/⁴⁰Ar年代学与地球化学证据     

刘倩  唐立梅  陈灵  胡艳华  吴招才  孟万斌 《地质科学》2023,(2):511-528

玄武岩作为地幔岩浆的产物,其岩石地球化学特征在反映地幔组分和深部动力学作用方面有着极其重要的意义。本文对东太平洋CC区西部和魏源海山两个潜次(Dive64和Dive66)的9个玄武岩样品进行了年代学、全岩地球化学和Sr-Nd-Pb同位素研究。结果显示,Dive64与Dive66玄武岩样品³⁹Ar/⁴⁰Ar年龄分别为83.1±0.3 Ma、74.7±0.3 Ma,属于晚白垩世,主体分别为N-MORB和OIB。Dive64为亚碱性玄武岩,REE总体相对平坦,轻重稀土分馏较弱,无明显Eu负异常;Dive66玄武岩为碱性玄武岩,富集轻稀土元素,亏损重稀土元素,无明显Eu、 Ce异常,MgO含量与CaO/Al₂O₃比值呈反比,与Cr含量、 Sr含量呈略微正相关。Sr-Nd-Pb同位素表明两者的形成可能不止单一源区的贡献,Dive64玄武岩Sr-Nd-Pb同位素比值更靠近DM(亏损地幔)、HIMU(高U/Pb比值地幔)端元,Dive66玄武岩Sr-Nd-Pb同位素比值较接近EMⅠ(Ⅰ型富集地幔)、HIMU端元。...  相似文献   

中国东北鸡西新生代玄武岩源区岩性制约     

郑志翀  曾罡  张慧丽  刘建强  陈立辉  周中彪 《高校地质学报》2023,(2):186-200

新生代火山岩在中国东北地区广泛出露,主要集中于松辽盆地周缘。其中盆地东部多沿抚顺—密山、依兰—伊通断裂带分布,尤其集中于长白山地区,以钠质玄武岩为主。前人研究表明,东北地区的地幔源区存在显著的化学不均一性,暗示这些玄武岩复杂的成因。为进一步查明它们的地幔源区岩性,揭示其岩石成因,文章选择抚顺—密山断裂带北部鸡西地区的玄武岩开展研究工作。研究区玄武岩岩性变化较大,其SiO₂含量为44.2～49.6 wt%,MgO含量为6.7～10.6 wt%,在TAS分类图上可进一步细分为碧玄岩、粗面玄武岩及玄武岩三个类别。微量元素上,研究样品呈现不相容元素相对富集的特征,具Nb、Ta的正异常和Pb、Ti的负异常,与洋岛玄武岩的微量元素组成相类似。通过计算研究样品的原生岩浆组成,发现其具有富MgO、贫SiO₂和CaO的特征,在透辉石向CATS-橄榄石-石英的投影图上落在贫硅辉石岩的区域内;同时结合玄武岩较高的FC3MS(FeO^T/CaO-3×MgO/SiO₂)值,认为其源区确实存在辉石岩组分的贡献。为进一步证实上述岩...  相似文献   

峨眉山二滩玄武岩地球化学特征   总被引：3，自引：0，他引：3  

严再飞  黄智龙  许成  温春齐  张振亮 《矿物岩石》2006,26(3):77-84

峨眉山大火成岩省二滩地区玄武岩w(S iO2)/%=40.5~59.65;普遍高碱,w(K2O N a2O)=2.64%~7.67%。w(T iO2)=2.10%~6.53%,T i/Y>500,该区玄武岩属于高钛(HT)型玄武岩;其M g#=58~84,明显高于高于宾川高钛玄武岩(31~53),说明岩浆演化程度明显低于宾川高钛玄武岩浆。岩石样品中Sr显示明显负异常,暗示了二滩玄武岩经历了广泛的斜长石结晶分离;而Eu不显异常,则反映了玄武岩岩浆中有高Eu3 /Eu2 比值的存在,其环境为氧化环境。在二滩玄武岩和宾川高钛玄武岩中,N i,Z r,T iO2和M g#均显示了明显差异,说明二滩玄武岩具有独立的地球化学特征。二滩玄武岩不相容元素(R b,B a,Th,U,N b,T a,L a,C e等)配分曲线与O IB相似,及其T a/Y b vs Th/Y b双变量图解也显示出了富集地幔特征,这些特征反映了峨眉山二滩玄武岩源区为富集地幔源,玄武岩岩浆可能为地幔柱物质。此外,B a/Th,Z r/N b,L a/N b,B a/N b等比值介于EM I O IB和EM II O IB之间,以及C e/Pb比值也说明:二滩玄武岩缺少H IMU O IB端元组分,是EM I O IB和EM II O IB两端元的混合产物。  相似文献   

西秦岭太阳山斑岩铜-钼矿床岩体氧逸度及成矿意义     

勾宗洋  于皓丞  邱昆峰  吴鸣谦  周春生  朱锐  李俊  温依瞳 《地学前缘》2019,26(5):243-254

甘肃天水三叠纪太阳山斑岩铜钼矿床位于西秦岭造山带东段。矿体主要赋存于石英闪长斑岩、二长斑岩、石英二长斑岩和泥盆系大草滩群。氧逸度是表征岩石物理化学性质的重要参数,对岩浆热液成矿具有明显的控制作用。在综合评述常用氧逸度计算方法及适用性的前提下,文中应用激光剥蚀等离子质谱分析方法对太阳山矿床含矿岩体锆石微量元素进行测定,选用含量较高的Sm、Nd进行Ce异常计算,查明含矿斑岩岩浆氧逸度,探讨其成矿意义。太阳山矿床岩浆氧逸度计算结果表明,太阳山成矿二长斑岩和石英二长斑岩相对氧逸度ΔFMQ分别为+3.04和+3.15,成矿前石英闪长斑岩相对氧逸度ΔFMQ为-1.83,成矿岩体氧逸度明显高于成矿前岩体。成矿岩体岩浆氧逸度高于成矿前岩体的原因可能与富集地幔有关。富集岩石圈地幔的加入,带来了大量的硫和金属铜,并提高了岩浆氧逸度。  相似文献   

地球氧逸度     

《地球化学》2020,(1)

地球是一个"氧化性"的星球。在太阳系所有行星中,只有地球大气中含有高浓度的O_2(约占21%)。研究表明,地球演化的早期,其大气组成与火星等类地行星相似,都是以CO_2为主,O_2含量可以忽略不计。在大约24-21亿年前,地球大气中O_2含量突然大幅度升高,一度超过现今O_2含量的1%,而后又在中元古代回落到现今O_2含量的0.1%以下。沉积物中氧化还原敏感元素的含量变化显示,大约6.3亿年前雪球地球结束之后,地球大气中的O_2含量再次大幅度升高至20%左右,而后在显生宙经历一系列复杂变化并最终演化至现今的水平。Re/Os比值显示,硅酸盐地球的氧逸度远高于月球,也高于火星。考虑到月球与地球分异发生在45亿年前,月球的低氧逸度暗示地球早期的氧逸度可能也较低。可以影响地球氧逸度的元素主要有O、H、Fe、S和C等。控制地球氧逸度变化的主要过程包括:核幔分异、板块俯冲和火山喷发去气等。在核幔分异以前,金属Fe可能是控制硅酸盐地球及其表生环境低氧逸度的关键因素。核幔分异过程中,Fe是控制氧逸度变化的关键元素。核幔分异将金属Fe与铁氧化物分开,造成地幔Fe~(3+)/Fe~(2+)比值升高。尤其是在下地幔,Fe~(2+)在高压下发生歧化反应,形成金属Fe和Fe~(3+)。其中Fe~(3+)赋存在布里奇曼石中,导致下地幔氧逸度低。在板块俯冲过程中,当有板片进入下地幔时,布里奇曼石会因体积补偿,被运移到上地幔,并发生分解,释放出Fe~(3+),导致周围地幔氧逸度的升高。但是,V/Sc和Zn/Fe等元素比值则显示在过去30多亿年以来,地幔的氧逸度变化不大,可能与上、下地幔间氧化还原缓冲层或者是上述元素比值对氧逸度不够敏感有关。在地球演化早期,金刚石是最早形成的矿物。由于金刚石的密度在上地幔高于地幔橄榄岩熔体,而在下地幔小于地幔橄榄岩熔体,因此在岩浆海阶段,金刚石倾向于在上地幔底部富集,成为一个富金刚石的储层。在板块俯冲阶段,这些金刚石会被布里奇曼石分解所释放的Fe~(3+)所氧化,形成富碳酸盐和CO:的层位,同时起到稳定上地幔氧逸度的作用。俯冲带地幔橄榄岩和岛弧火山岩的氧逸度均高于板内环境,因此一般认为板块俯冲会导致氧逸度升高。在板块俯冲过程中,氧逸度主要受到Fe和H_2O(水分解释放出H_2)的控制。蚀变大洋岩石圈中含有大量的H_2O,板块俯冲过程中脱水会导致地幔楔蛇纹石化。蛇纹石化过程会形成磁铁矿,释放出味,使局部在短时间内氧逸度降低。但是,由于H_2很容易逸散到大气中,而磁铁矿则保留在地幔楔中,其结果导致岩石中Fe~(3+)/Fe~(2+)比值升高,从而在发生部分熔融时形成高氧逸度岩浆。板块俯冲对氧逸度的影响是多方面的,还与俯冲板块的年龄、沉积物的性质等有关。对于富含有机物的沉积物俯冲过程,C是主要的氧逸度控制元素。在板块俯冲的浅部,有机物分解,释放出CH_4等还原性气体,造成上覆岩石圈氧逸度下降。富含铁锰结核等氧化性沉积物的俯冲则可以导致地幔楔氧逸度的升高,这一过程中Fe和Mn是控制氧逸度的主要元素。火山喷发可以释放出CH_4、CO_2、H_2S和SO_2等气体,也可以影响大气中O_2的含量。有研究认为,火山气体中的H_2S随岩浆房压力增加而增加,SO_2则随压力的增加而减少,因此岩浆房压力可以影响其排气的氧化-还原性,进而影响大气的O_2含量。一种观点认为,正是由于太古宙末期大量出现陆相火山岩,导致了大氧化事件,在这一模型中,S是控制氧逸度的关键。氧逸度对多种成矿作用均具有重要的控制作用。其中,斑岩铜金矿床的形成往往与高氧逸度的埃达克岩有关。这是由于当岩浆的氧逸度高于AFMQ+1.5时,岩浆中S主要以硫酸盐的形式存在。由于硫酸盐在岩浆中的溶解度远远高于硫化物,因此,在俯冲洋壳部分熔融过程中形成的高氧逸度埃达克质岩浆可以熔出更多的亲硫元素,有利于成矿。锡矿床的形成则往往与还原性岩浆有关。这是因为在高氧逸度岩浆中,Sn主要呈Sn~(4+),易于在岩浆结晶早期进入矿物中;而在还原性岩浆中,Sn主要以Sn~(2+)形式存在,表现为不相容元素,倾向于在岩浆中富集,并在岩浆期后热液阶段富集成矿。其他氧化还原敏感元素,如U、V、Mo、Re、Sb和Fe等,可以在表生过程中富集,有利于进一步富集成矿。  相似文献   

辽宁赛马霓霞正长岩黑云母地球化学特征、40Ar-39Ar年龄及其地质意义          下载免费PDF全文

钟军  范洪海  陈金勇  孟艳宁  赵敬洋  史长昊  王生云 《地球科学》2020,45(1):131-144

黑云母不仅是理想的40Ar-39Ar年代学定年矿物,其化学组成还可用来指示母岩浆物理化学条件、岩浆源区及分异演化程度、成矿潜力和成岩构造环境.本文对辽宁赛马碱性杂岩体中分布最为广泛的霓霞正长岩中的黑云母开展系统电子探针分析和40Ar-39Ar定年,结合pMELTS软件对前人全岩主量元素分析数据开展了平衡结晶计算,探讨了母岩浆物理化学性质、演化过程和成岩构造背景.电子探针分析结果表明赛马霓霞正长岩黑云母具有高铁高钛特征,属铁质黑云母.根据黑云母主量元素含量及比值估算黑云母结晶温度为770~800℃,lgf_O2介于-16~-14,而pMELTS平衡结晶计算结果表明整个霓霞正长岩岩浆体系于1 300℃以上便已开始结晶,且随温度降低氧逸度呈现不断降低的趋势,这种较高温度和持续降低的氧逸度环境不利于岩浆热液的分异,使得碱金属（Na）、挥发分及铀钍稀有元素保留在岩浆房内并在后期钠质岩浆（异霞正长岩）结晶分异过程中富集成矿.部分黑云母发育完好的振荡环带,且核部较幔部具有更高的TiO₂、Na₂O含量和更低的SiO₂含量和Fe3+/（Fe3++Fe2+）比值,也进一步证实黑云母结晶后残余岩浆具有更低氧逸度和更高Na含量.赛马碱性岩是华北克拉通北缘近东西向碱性岩带的一部分,本文获得其黑云母40Ar-39Ar年龄为222 Ma左右,形成于古亚洲洋闭合之后的后碰撞伸展构造背景.   相似文献   

长白山区二道白河流域早更新世玄武质熔岩的成因   总被引：2，自引：1，他引：1  

马晗瑞  杨清福  盘晓东  武成智  陈聪 《岩石学报》2015,31(11):3484-3494

采用岩石化学和同位素分析方法,研究了二道白河流域早更新世玄武质熔岩的成因。玄武质熔岩由钠质拉斑玄武岩和钾质粗面玄武岩、玄武质粗面安山岩组成。它们的REE分配形式比较相近,表明它们来自共同的源区。Sr、Nd、Pb同位素示踪表明,二道白河流域早更新世玄武质熔岩岩浆源区接近于似原始地幔。它们的Mg#=100Mg O/(Mg O+Fe O)低于中国东部新生代玄武岩原始岩浆的Mg#(60~68),Ni(27.76×10-6~200.6×10-6)低于原始地幔,Rb/Sr(0.05~0.09)、Ba/Rb(15.64~264)高于原始地幔,说明这些岩石不是源自原始地幔。玄武质熔岩的DI变化于42~67,具有高Ca、高Sr、Eu正异常,微量元素图解显示玄武岩保留部分熔融趋势,粗面玄武岩、玄武质粗安岩具有结晶分异趋势,岩浆上升过程中发生了不同程度的地壳混染作用。玄武质熔岩的Nb/Ta之比为14.8~15.8,与勘察加半岛深俯冲带火山类似。Nb/Ta-(Na2O-K2O)关系图解显示研究区玄武质岩浆的形成与俯冲板片的部分熔融有关。  相似文献   

幔源岩浆氧化还原状态及对岩浆矿床成矿的制约   总被引：7，自引：5，他引：2  

柏中杰  钟宏  朱维光 《岩石学报》2019,35(1):204-214

岩浆的氧化还原状态是控制许多基本地质过程的关键热动力学参数之一。估算玄武质岩浆和源区岩石氧化还原状态的常用方法主要包括多价元素的价态、多价元素的分配系数、共存矿物对的化学平衡和全岩化学比值。岩石学实验的深入和分析技术手段的快速发展使精确估算岩浆氧逸度成为可能。这有力地促进了对地幔源区成分、岩浆的部分熔融程度和熔融方式与分异演化历史,以及岩浆矿床的成因机制及成矿过程的研究。幔源岩浆的氧化还原状态复杂多变,不仅与构造背景有关,还与地幔深度(压力)、交代作用和部分熔融有着密切联系。而在岩浆到达浅部地壳后,结晶分异、岩浆去气和同化混染等过程也能不同程度地改变岩浆的氧逸度。因此,即使来自同一构造背景的幔源岩浆也呈现出明显的氧逸度不均一性。氧逸度的高低对源区部分熔融过程中金属元素的地球化学行为、岩浆的分异演化趋势、Fe-Ti-V氧化物饱和时间的早晚和S在岩浆中的溶解度具有明显的控制作用。因此,岩浆的氧逸度对钒钛磁铁矿矿床和汇聚板块边缘的岩浆硫化物矿床的成矿过程具有显著的影响。  相似文献   

Petrogenesis of ultramafic rocks and associated chromitites in the Nan Uttaradit ophiolite, Northern Thailand   总被引：1，自引：0，他引：1  

B. Orberger  J. P. Lorand  J. Girardeau  J. C. C. Mercier  S. Pitragool 《Lithos》1995,35(3-4):153-182

The ultramafic sequence and associated chromitites of the Nan-Uttaradit ophiolite in the northeastern part of Thailand have been studied in the field and by applying petrography and geochemistry to whole rock samples and minerals. The ultramafic rocks comprise irregulary shaped bodies of dunite, harzburgite, orthopyroxene-rich lherzolite and orthopyroxene-rich harzburgite, clinopyroxene-rich dunite and intrusive clinopyroxenite-websterite bodies. Three types of chromitite were distinguished. Type I chromitite lenses and type II layers which are hosted in orthopyroxenite in the northern part and in dunite in the central part of the ophiolite. Type III chromitite forms lenses or layers in clinopyroxenites in the central and southern parts of the belt. According to the modal and chemical composition the peridotites and orthopyroxenites are strongly refractory. They originated during different stages of interaction between percolating melts and peridotite. The chromitites of types I and II, which are very rich in Cr (up to 68 wt.% Cr₂0₃), crystallized from a boninitic parental magma under highly reducing conditions in the northern part and moderate oxygen fugacities (FMQ) in the central part of the ophiolite. The chromitite of type III which are characterized by the highest Fe³⁺/(Fe³⁺ + Cr + Al) -ratios, and hosted in intrusive clinopyroxenite-websterite-rocks, cumulated from a CaO-rich transitional boninitic melt under fO₂ conditions around FMQ.  相似文献   

The nature of the sub-continental mantle: constraints from the major-element composition of continental flood basalts   总被引：1，自引：0，他引：1  

Simon Turner  Chris Hawkesworth 《Chemical Geology》1995,120(3-4):295-314

Many continental flood basalts (CFB) have isotope and trace-element signatures that differ from those of oceanic basalts and much interest concerns the extent to which these reflect differences in their upper mantle source regions. A review of selected data sets from the Mesozoic and Tertiary CFB confirms significant differences in their major- and trace-element compositions compared with those of basalts erupted through oceanic lithosphere. In general, those CFB suites characterised by low Nb/La, high (⁸⁷Sr/⁸⁶Sr)_i and low εNd_i tend to exhibit relatively low TiO₂, CaO/Al₂O₃, Na₂O and/or Fe₂O₃, and relatively high SiO₂. In contrast, those which have high Nb/La, low (⁸⁷Sr/⁸⁶Sr)_i and high εNd_i ratios, like the upper units in the Deccan Traps, have major- and trace-element compositions similar to oceanic basalts. It would appear that those CFB that have distinctive isotope and trace-element ratios also exhibit distinctive major-element contents, suggesting that major and trace elements have not been decoupled significantly during magma generation and differentiation.

When compared (at 8% MgO) with oceanic basalt trends, the displacement of many CFB to lower Na₂O, Fe₂O₃^*, TiO₂ and CaO/Al₂O₃, but higher SiO₂, at similar Mg#, is not readily explicable by crustal contamination. Rather, it reflects source composition and/or the effects of the melting processes. The model compositions of melts produced by decompression of mantle plumes beneath continental lithosphere have relatively low SiO₂ and high Fe₂O₃^*. In contrast, the available experimental data indicate that partial melts of peridotite have low TiO₂, Na₂O and Fe₂O₃^*CaO/Al₂O₃, if the peridotite has been previously depleted by melt extraction. Moreover, melting of hydrated, depleted peridotite yields SiO₂-rich, Fe₂O₃- and CaO-poor melts. Since anhydrous, depleted peridotite has a high-temperature solidus, it is argued that the source of these CFB was variably melt depleted and hydrated mantle, inferred to be within the lithosphere. Isotope data suggest these source regions were often old and relatively enriched in incompatible trace elements, and it is envisaged that H₂O±CO₂ were added at the same time as the incompatible elements. An implication is that a significant proportion of the new continental crust generated since the Permian reflected multistage processes involving mobilization of continental mantle lithosphere that was enriched in minor and trace elements during the Proterozoic.  相似文献   

Study of oxygen fugacity during magma evolution and ore genesis in the Hongge mafic–ultramafic intrusion,the Panxi region,SW China     

Mingyang Liao  Yan Tao  Xieyan Song  Yubang Li  Feng Xiong 《中国地球化学学报》2016,35(1):25-42

Economic concentrations of Fe–Ti oxides occurring as massive layers in the middle and upper parts of the Hongge intrusion are different from other layered intrusions (Panzhihua and Baima) in the Emeishan large igneous province, SW China. This paper reports on the new mineral compositions of magnetite and ilmenite for selected cumulate rocks and clinopyroxene and plagioclase for basalts. We use these data to estimate the oxidation state of parental magmas and during ore formation to constrain the factors leading to the abundant accumulation of Fe–Ti oxides involved with the Hongge layered intrusion. The results show that the oxygen fugacities of parental magma are in the range of FMQ?1.56 to FMQ+0.14, and the oxygen fugacities during the ore formation of the Fe–Ti oxides located in the lower olivine clinopyroxenite zone (LOZ) and the middle clinopyroxenite zone (MCZ) of the Hongge intrusion are in the range of FMQ?1.29 to FMQ?0.2 and FMQ?0.49 to FMQ+0.82, respectively. The MELTS model demonstrates that, as the oxygen fugacity increases from the FMQ?1 to FMQ+1, the proportion of crystallization magnetite increases from 11 % to 16 % and the crystallization temperature of the Fe–Ti oxides advances from 1134 to 1164 °C. The moderate oxygen fugacities for the Hongge MCZ indicate that the oxygen fugacity was not the only factor affecting the crystallization of Fe–Ti oxides. We speculated that the initial anhydrous magma that arrived at the Hongge shallow magma chamber became hydrous by attracting the H₂O of the strata. In combination with increasing oxygen fugacities from the LOZ (FMQ?1.29 to FMQ?0.2) to the MCZ (FMQ?0.49 to FMQ+0.82), these two factors probably account for the large-scale Fe–Ti oxide ore layers in the MCZ of the Hongge intrusion.  相似文献   

The redox state of subduction zones: insights from arc-peridotites   总被引：23，自引：0，他引：23  

Ian J. Parkinson  Richard J. Arculus 《Chemical Geology》1999,160(4):347-423

Spinel peridotites from a variety of island arcs have been utilised to calculate the redox state of the mantle wedge above subduction zones. Oxygen fugacities (f_O2 values) calculated from the ferric iron content of spinels, measured by Electron Microprobe (EMP) using secondary standards [Wood, B.J., Virgo, D., 1989. Upper mantle oxidation state: ferric iron contents of lherzolite spinels by ⁵⁷Fe Mössbauer spectroscopy and resultant oxygen fugacities. Geochim. Cosmochim. Acta, 53, 1277–1291.], yield values which range from 0.3 to 2.0 above the fayalite–magnetite–quartz (FMQ) buffer. These data provide further evidence that the mantle wedge is ubiquitously oxidised relative to oceanic and ancient cratonic mantle. There is no correlation between f_O2 values and the presence of hydrous phases and, in fact, the most oxidised samples contain no hydrous phases. Within individual suites there is no correlation between f_O2 and degree of depletion as indicated by spinel Cr#, except for a suite of reacted forearc-peridotites. However, when the data is viewed as a whole there is broad a positive correlation between f_O2 and spinel Cr# suggesting that partial melting processes may influence the redox state of the mantle wedge. We suggest that the ultimate source of the oxygen which oxidises the mantle wedge is from the subducted slab. It is not clear whether this oxidising agent is a solute-rich hydrous fluid or a water-bearing silicate melt. However, our data does indicate that silicate melts are effective oxidisers of the depleted shallow upper mantle. Simple mass balance calculations based on the ferric iron content of primitive subduction zone magmas indicates that the source region must contain 0.6–1.0 wt.% Fe₂O₃. This amount of Fe₂O₃ in a fertile spinel peridotite yields an oxygen fugacity of 0.5–1.7 log units above FMQ in the IAB source. If water is the sole oxidising agent in the mantle wedge then 0.030–0.075 wt.% H₂O is required which is considerably less than the 0.25% H₂O envisaged by Stolper and Newman [Stolper, E.M., Newman, S., 1994. The role of water in the petrogenesis of Mariana trough magmas. Earth Planet. Sci. Lett., 121, 293–325.], suggesting water is not necessarily an efficient oxidising agent. Alternatively, ferric iron may be added to the mantle wedge by addition of a ferric iron-rich sediment melt or more likely as a solute-rich hydrous fluid. This model would produce spinel, orthopyroxene or amphibole in the wedge with only a slight increase in f_O2 of the source region. Although it is unclear which model is correct the maximum f_O2 of the fertile mantle wedge is unlikely to be above FMQ+2 and therefore some decompression melting in the mantle wedge is required to explain the higher f_O2 values of primitive arc lavas than arc-peridotites.  相似文献   

Determination of Fe<Superscript>3+</Superscript>/ΣFe ratios in chrome spinels using a combined Mössbauer and single-crystal X-ray approach: application to chromitites from the mantle section of the Oman ophiolite     

Davide?LenazEmail author  Jacob?Adetunji  Hugh?Rollinson 《Contributions to Mineralogy and Petrology》2014,167(1):958

We present the results of a comparative study in which we have measured Fe³⁺/ΣFe ratios in chromites from mantle chromitites in the Oman ophiolite using Mössbauer spectroscopy and single-crystal X-ray diffraction. We have compared these results with ratios calculated from mineral stoichiometry and find that mineral stoichiometry calculations do not accurately reflect the measured Fe³⁺/ΣFe ratios. We have identified three groups of samples. The majority preserve Fe³⁺/ΣFe ratios which are thought to be magmatic, whereas a few samples are highly oxidized and have high Fe³⁺/ΣFe ratios. There is also a group of partially oxidized samples. The oxidized chromites show anomalously low cell edge (a ₀) values and their oxygen positional parameters among the lowest ever found for chromites. Site occupancy calculations show that some chromites are non-stoichiometric and contain vacancies in their structure randomly distributed between both the T and M sites. The field relationships suggest that the oxidation of the magmatic chromitites took place in association with a ductile shear zone in mantle harzburgites. Primary magmatic Fe³⁺/ΣFe ratios measured for the Oman mantle chromitites are between 0.193–0.285 (X-ray data) and 0.164–0.270 (Mössbauer data) and preserve a range of Fe³⁺/ΣFe ratios which we propose is real and reflects differences in the composition of the magmas parental to the chromitites. The range of values extends from those MORB melts (0.16 ± 0.1) to those for arc basalts (0.22–0.28).  相似文献   

Magmatic and hydrothermal processes in the Bouvet Triple Junction Region (South Atlantic)     

V.A. Simonov  A.A. Peyve  V.Yu. Kolobov  A.A. Milosnov  S.V. Kovyazin 《地学学报》1996,8(5):415-424

Results of electron microprobe and microthermometric studies of samples collected from the Bouvet Triple Junction Region (BTJR) during a joint Russian-Italian geological expedition on the R/V Academician Nikolaj Strakhov (1994) have revealed new data on the composition of basaltic magmas and oceanic hydrothermal fluids connected with magmatic processes. Detailed analysis of basaltic glasses shows that the modem Mid-Atlantic Ridge (MAR) rift valley is composed of normal mid-ocean ridge basalts with low concentrations of K₂ O and TiO_z (N-MORB), while its flanks are more enriched with these components approaching E-MORB. A marked influence of the Bouvet hot spot volcanism on magma generation on the South-West Indian Ridge (SWIR) near Bouvet Island is observed. Basaltic melts in this area belong to alkalic and transitional series and have maximum contents of K₂O, TiO₂, H₂O.
Microthermometric analyses of fluid inclusions in the samples from the BTJR have revealed major differences in the oceanic hydrothermal fluid systems on the MAR and near SWIR, which depends on the peculiarities of magma. In the area of the MAR (with dry melts) only H₂O solution inclusions in quartz were found; thus, seawater is probably the only primary source of hydrothermal fluids (NaCl + MgCl₂+ H₂O; T = 170–200°C). In the SWIR area (with the high content of water in melts) syngenetic liquid CO₂ and H₂O solution inclusions in quartz indicate the influence of the magmatic fluid component on the ore-forming water/carbon dioxide solutions (NaCl + CaC1₂+ H₂O + CO₂; T = 200–310 °C; P = 900–1700 bar).  相似文献   

Phlogopite in the generation of olivine-melilitites from Namaqualand, South Africa and implications for element fractionation processes in the upper mantle     

N. W. Rogers  C. J. Hawkesworth  Z. A. Palacz 《Lithos》1992,28(3-6):347-365

Major and trace element and Sr, Nd and Pb isotope analyses are presented for thirteen olivine-melilitites from Namaqualand, South Africa. Major element variations are consistent with derivation from carbonated garnet-peridotite at depths of at least 100 km and trace element abundances indicate melt fractions of 4%. Ubiquitous negative K anomalies and low, buffered K₂O concentrations are interpreted to reflect the effect of residual phlogopite during melting. It is suggested that phlogopite stability and low melt potassium saturation concentrations are enhanced by high CO₂/(CO₂ + H₂O) conditions. Residual phlogopite can also account for low measured Rb/Sr, Ba/Sr and Th/U ratios in the melilitites. REE abundances are controlled by residual garnet and hence Sm/Nd ratios are low (0.13–0.18). U/Pb ratios vary from 0.05 to 5 and are a function of Pb concentration which is in turn controlled by residual Pb-rich phase (probably sulphide). Nd and Sr isotopes are comparable with OIB from St. Helena, although two samples extend to higher ⁸⁷Sr/⁸⁶Sr ratios. Present day Pb isotopes are much more variable and partly reflect radiogenic growth since emplacement as a result of the highly variable U/Pb ratios.

Many of the trace element characteristics of the melilitites are distinct from those of within-plate potassic magmas despite both being derived from phlogopite-bearing, enriched mantle source regions. This can be attributed to the depth at which source enrichment occurred and the subsequent control exerted by phlogopite and carbonate during melting. In contrast to melilitites, potassic magmas are derived from shallower depths under low CO₂/(CO₂ + H₂O) conditions and at higher temperatures at which phlogopite melts more readily.

The incompatible element ratios of the melilitites are also similar to those both observed in HIMU ocean island basalts (OIB) and inferred for HIMU OIB source regions from isotope variations (viz, low Sm/Nd, Rb/Sr, K/Nb, Th/U and high U/Pb and Ce/Pb). It is suggested that HIMU OIB's may be derived from sources that have been subject to enrichment by a melt generated in the presence of residual phlogopite.  相似文献   

中国东部新生代玄武岩及其他幔包体的氧逸度   总被引：1，自引：0，他引：1  

张毅刚  鄂莫岚 《岩石学报》1994,10(2):161-170

地幔环境的氧逸度与温度和压力一样，是控制许多地幔过程的一个重要参数。本文计算了中国东部几个具有代表性地区的玄武岩和尖晶石二辉橄榄岩的氧逸度，尖晶石二辉橄榄岩的氧逸度变化不大，均位于１ｏｇ（ｆｏ２）＝ｌｏｇ（ｆｏ２ＦＭＱ）＋０．０左右，而各地区玄武岩的氧逸度却变化很大，其平均值从尚志地区的ｌｏｇ（ｆｏ２ＦＭＱ＋０．６到长白山地区的ｌｏｇ（ｆｏ２ＦＭＱ）＋３．３左右（其中东北地区钾质玄武岩的氧逸度比除尚志以外其它地区的低），并且总体具有比地幔橄榄岩高得多的氧逸度。推测钾质玄武岩和尚志地区破性玄武岩的氧逸度比中国东部其它地区玄武岩的氧逸度低的可能原因是，前二个地区的玄武岩来源于更深部的（金云母）石榴石二辉橄榄岩，而其它地区的玄武岩来源于略浅部的尖晶石二辉橄榄岩。  相似文献   

中国东北软流圈地幔中的原始橄榄岩质地幔:来自大兴安岭地区新生代玄武岩的地球化学证据          下载免费PDF全文

薛笑秋  陈立辉  刘建强  何叶  王小均  曾罡  钟源 《地球科学》2019,44(4):1143-1158

为了进一步了解中国东北新生代玄武岩地幔源区的物质属性,报道了大兴安岭哈拉哈河-柴河地区新生代玄武岩的全岩主量、微量元素和Sr、Nd、Pb、Hf同位素组成.哈拉哈河-柴河玄武岩属钠质碱性系列,具有与洋岛玄武岩相似的微量元素特征,如富集大离子亲石元素（LILEs）、明显的Nb、Ta正异常等.它们具有中等亏损的Sr-Nd-Hf同位素组成（87Sr/86Sr=0.703 5~0.703 9、ε_Nd=5.21~6.55、ε_Hf=10.00~11.25）,接近中国东部新生代玄武岩的亏损端元.这些玄武岩具有中等的放射成因Pb同位素组成（206Pb/204Pb=18.37~18.57、207Pb/204Pb=15.52~15.54和208Pb/204Pb=38.24~38.43）,在206Pb/204Pb-207Pb/204Pb相关图上位于4.42~4.45 Ga的地球等时线之间.它们在Sr-Nd-Pb同位素相关图中均落入地幔柱来源的、高3He/4He比（>30R_a）的洋岛玄武岩范围内,暗示其源区可能存在来自深部地幔的古老原始地幔物质.此外,这些玄武岩具有高MgO（8.49%~11.58%）、高Ni（174×10-6~362×10-6）和高Mg#（59.1~66.9）的特征,表明它们接近于原始岩浆的成分.反演的哈拉哈河-柴河玄武岩的原始岩浆组成具有中等的SiO₂、低Al₂O₃以及高CaO/Al₂O₃比的特征,与石榴子石橄榄岩高压（>2.5 GPa）实验熔体的成分相当,暗示玄武岩的源区岩性最可能为橄榄岩.对以原始地幔（而不是亏损地幔）的微量元素为初始成分的饱满石榴子石二辉橄榄岩进行低程度（1%~2%）部分熔融的模拟计算,产生的熔体与哈拉哈河-柴河玄武岩具有一致的微量元素特征,这进一步支持了上述推断.综上所述,认为大兴安岭地区哈拉哈河-柴河玄武岩的源区含有来自深部地幔的古老的橄榄岩质原始地幔组分.   相似文献