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1.
中天山白石泉镁铁-超镁铁质岩体岩石学与矿物学研究   总被引:16,自引:0,他引:16  
白石泉地区镁铁一超镁铁质岩体处于塔里木板块前缘活动带与中天山地块接合部位,是中天山地块华力西中期岩浆活动的产物。主要岩石类型有辉石橄榄岩(斜方辉石橄榄岩、斜长二辉橄榄岩)、橄榄辉石岩、橄长岩、辉长岩及角闪辉长岩等,主要造岩矿物为橄榄石、斜方辉石、单斜辉石、角闪石、斜长石及黑云母。橄榄石均为贵橄榄石,其Fo值(78-85)位于含铜镍硫化物矿橄榄石的Fo值范围之内;辉石主要有顽火辉石、古铜辉石、紫苏辉石、透辉石等;斜长石的环带构造较为发育;角闪石的FeO含量随着岩浆的演化逐渐增加。它们与造山带环境中的东疆型镁铁一超镁铁杂岩中的造岩矿物具有相同的特征。这些特征表明了白石泉地区的镁铁一超镁铁质岩体的原始岩浆为高镁的拉斑玄武质岩浆。  相似文献   

2.
金川是世界第三大在采岩浆铜镍硫化物矿床,其成因备受中外地质学家的关注。金川岩体被一系列北东-东向左行平移断层自西向东依次划分为Ⅲ、Ⅰ、Ⅱ、Ⅳ等4个岩体。金川岩体主要由硫化物纯橄岩、二辉橄榄岩、橄榄辉石岩组成,边缘断续分布少量斜长石二辉橄榄岩和辉石岩。金川最大的1号矿体产于Ⅱ号岩体的中心,呈现出由中间硫化物纯橄岩向两侧浸染状的二辉橄榄岩和橄榄辉石岩过渡的对称式岩相分布。电子探针分析结果显示,金川Ⅱ号岩体橄榄石Fo值在79.7%~83.9%之间变化,w(Ni)为959×10-6~2060×10-6,大多低于从硫不饱和玄武岩浆中结晶出的橄榄石Ni含量。模拟计算表明金川岩体母岩浆为高MgO玄武岩浆(w(MgO)=10%~13%,w(FeO)=11.5%~12.5%)。橄榄石Ni含量偏低的原因是橄榄石结晶的同时发生了硫化物熔离,橄榄石与硫化物的质量比值约为40﹕1。硫化物纯橄岩和二辉橄榄岩中橄榄石的Ni含量及其与Fo值的相关性都存在显著的区别,暗示它们可能是从Ni含量不同的母岩浆中结晶出来的。同时,硫化物纯橄岩中橄榄岩经历了与硫化物熔体的Fe-Ni交换...  相似文献   

3.
对新疆西天山备战铁矿区附近的基性-超基性岩体———金云母辉石橄榄岩与侵入其中的闪长岩脉进行了年代学和岩石地球化学研究。金云母辉石橄榄岩中金云母~(40)Ar/~(39)Ar坪年龄为298.1±1.9 Ma,该岩石的锆石U-Pb年龄为302.5±1.3 Ma,与备战铁矿的成矿年龄相近。备战金云母辉石橄榄岩具有低Si O_2(42.51%~50.82%)、Al_2O_3(4.87%~7.38%)、Ti O_2(0.25%~0.77%)和全碱(Na_2O+K_2O=0.87%~1.87%)含量,而高Mg O(26.36%~30.17%)、TFe O(12.33%~15.99%)含量的特征,过渡元素丰度(Cr=523×10~(-6)~7 026×10~(-6),Ni=906×10~(-6)~1 088×10~(-6),Co=109×10~(-6)~132×10~(-6))和Mg~#值(0.76~0.79)均较高,表明岩浆经历了橄榄石堆晶作用。由橄榄石最高Fo值(0.79)和岩石的TFe O含量计算得其母岩浆为玄武质岩浆。所有的岩石具有相似的稀土、微量元素配分模式,均呈轻稀土元素富集的右倾型,且重稀土元素较平坦[(Gd/Lu)_N=0.70~2.00],明显富集大离子亲石元素Rb、Ba、U、K,亏损高场强元素Nb、Ta、Zr、Hf和Ti。总体上Sr、Nd同位素较均一,金云母辉石橄榄岩的(~(87)Sr/~(86)Sr)_i=0.704 4~0.704 7,εNd(t)=2.23~3.90,闪长岩(~(87)Sr/~(86)Sr)_i=0.704 4,εNd(t)=3.79~4.07,表明金云母辉石橄榄岩和闪长岩为同源演化的岩石。微量元素特征表明金云母辉石橄榄岩起源于尖晶石相,源区为受俯冲流体或熔体交代的软流圈地幔。结合区域构造背景,推测金云母辉石橄榄岩的形成与西天山造山带在晚古生代的山根拆沉引起的软流圈上涌有关,而备战铁矿晚期成矿事件很可能形成于相同的深部动力学背景下。  相似文献   

4.
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   

5.
白马寨I号岩体是哀牢山—金沙江构造带白马寨Cu-Ni矿区内最大的一个含矿基性—超基性岩体,从中心向边缘依次由含矿橄榄岩、矿化辉石岩和辉长岩3个相带组成环状体。从中心相到边缘相,岩石中SiO2、TiO2、Al2O3、CaO、Na2O和K2O含量逐渐增加,TFe、MgO含量降低;稀土元素中w(∑REE)、w(LREE)/w(HREE)逐渐增加,δEu由负异常到正异常演变;微量元素具有大离子亲石元素和高场强元素逐渐增加、强亲岩浆元素逐渐降低的演变特征。铂族元素配分模式为Pt-Pd型,w(Pt)/w(Pd)比值为0.32~0.68,介于富硫化物拉斑玄武岩(0.38)和原始上地幔(1.36)之间,以及稀土元素配分模式、微量元素蛛网图和铂族元素配分模式中不同岩石配分曲线的相似性揭示3个相带不同岩石之间的高度一致性,展示基性—超基性岩形成于玄武质岩浆演化、熔离及岩浆一次性侵入、分异成岩成矿的特征。矿区内地层层序稳定,岩体与沉积岩之间的侵入接触关系及w(Zr)-w(Y)-w(Nb)图解说明白马寨岩体形成于陆内环境。岩体的低Ti含量、Th强烈正异常和含矿橄榄岩负Eu异常,以及w(Th)/w(Ta)比值、w(Th)/w(Nb)比值和w(Pd)/w(Pt)比值及Ir族元素配分曲线明显不同于峨眉山玄武岩和典型的地幔柱玄武岩,而与大陆裂谷玄武岩非常相近,说明白马寨I号岩体形成于大陆裂谷环境。  相似文献   

6.
南海盆地及周缘地区新生代玄武岩对揭示南海盆地的演化历史至关重要,然而这些玄武岩的成因还存在争议。本文研究了位于南海北部陆缘的海南岛临高县多文组玄武岩岩石地球化学和矿物地球化学特征,并探讨其成因和构造背景。多文组玄武岩主要由橄榄石、单斜辉石、斜长石、斜方辉石、铬尖晶石和铁钛氧化物等组成。橄榄石Fo值变化于55.5~71.1之间,Ni的含量较低,Fe/Mn比值较高。铬尖晶石Cr#值为74.1~82.7,Mg#值为45.5~63.8, Ti的含量较高。斜方辉石Mg#值为63.9~79.6,单斜辉石为66.0~80.6。单斜辉石稀土配分曲线富集MREE,亏损LREE和HREE,呈拱形分布。斜长石以中-拉长石为主(Ab36.56~52.78),富集LREE、Ba、Sr和Eu。铁钛氧化物的TiO2含量为50.19%~51.46%。多文组玄武岩原始岩浆的主量和微量元素组成与夏威夷、峨眉山、塔里木等玄武岩组成一致,地幔源区包含了辉石岩的成分,而且其地幔潜在温度(>1400℃)和氧逸度(Δ...  相似文献   

7.
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   

8.
谢燮  杨建国  王小红  王磊  江磊  姜安定 《现代地质》2015,29(6):1259-1270
甘肃北山红柳沟基性-超基性岩体位于塔里木板块北缘北山裂谷带, 岩体侵位于敦煌岩群,主要岩石类型有辉长岩、橄榄辉长岩、橄榄苏长辉长岩、橄榄角闪苏长岩、橄榄辉长苏长岩、二辉橄榄岩、橄榄辉石岩和辉石岩等。橄榄石Fo介于66.97%~82.92%之间,属贵橄榄石,斜方辉石En成分范围为68.49~77.65,属古铜辉石;单斜辉石En成分范围为45.85~48.81,主要为斜顽辉石和透辉石;斜长石An为58.70~72.69,以拉长石为主;角闪石以普通角闪石为主。岩体母岩浆Mg#值为0.59~0.62,属于高镁拉斑玄武质岩浆,岩浆演化过程中主要发生了橄榄石、斜方辉石、单斜辉石和斜长石的分离结晶作用,主要分离结晶矿物受单斜辉石和斜方辉石的控制,岩浆上升侵位过程中遭受到下地壳物质混染。从构造环境、母岩浆、岩体类型、岩浆分异程度、同化混染等方面综合分析认为红柳沟岩体具有形成铜镍硫化物矿床的较大潜力。  相似文献   

9.
对桂东北鹰扬关地区新发现的罗家山辉长岩开展年代学、矿物学和矿物化学研究,可进一步约束区域构造背景.罗家山辉长岩的主要矿物为单斜辉石(Cpx)和斜长石(Pl).单斜辉石具有高铁铝、低钙钠钛的特征,其成分为Wo27~31En36~47Fs21~32,属于普通辉石;斜长石具有高硅铝钠、低钙钾的特点,其成分为An0~3Ab96~100Or0~2,属于钠长石.根据单斜辉石的化学成分判定罗家山辉长岩的母岩浆属于Si不饱和的亚碱性拉斑玄武岩系列.单斜辉石温压估算结果表明,罗家山辉长岩的形成温度介于1 282~1 292℃,平均值1 287℃;形成压力介于1.53~2.37 GPa,平均值2.02 GPa;对应深度介于50.49~78.21 km,平均值66.80 km.LA-ICP-MS锆石U-Pb年龄表明罗家山辉长岩形成于(768.9±6.8) Ma.单斜辉石的化学成分特征表明罗家山辉长岩属于典型的板内拉斑玄武岩.结合区域构造演化特征,推断罗家山辉长岩起源于地幔物质上...  相似文献   

10.
二叠纪镁铁-超镁铁质岩体在北山造山带广泛分布,其中多发育铜镍硫化物矿化,并集中在新疆北山坡北和甘肃北山柳园地区。本文对柳园地区二叠纪骆驼山(283Ma)和西南山(277Ma)矿化岩体中早期结晶的造岩矿物开展矿物化学分析,并对甘-新北山地区矿化岩体的主要造岩矿物进行系统对比研究。骆驼山和西南山岩体主要由单辉橄榄岩、二辉橄榄岩、橄榄辉石岩、橄榄辉长岩和辉长岩组成,主要造岩矿物为橄榄石、单斜辉石、斜方辉石、斜长石和角闪石,及少量铬尖晶石和金云母。铬尖晶石Cr#值范围为52.2~70.4,TiO2含量为1.1%~4.0%,Al2O3含量为8.1%~18.9%。橄榄石Fo值范围为78~86,Ni含量为856×10-6~2121×10-6,Ca含量为71.3×10-6~720×10-6。斜方辉石主要为顽火辉石和少量古铜辉石;单斜辉石为透辉石和普通辉石,Mg#范围为86~88,Al...  相似文献   

11.
研究表明,西天山阿吾拉勒铁铜成矿带中智博铁矿区火山碎屑岩中的富铁岩屑主要由自形针状/板条状钠长石和富铁基质组成,呈辉绿/斑状结构。电子探针分析显示,富铁岩屑中钠长石端员组分变化范围为An=0.38~2.89,Ab=95.2~99.32,Or=0.17~2.79,端员组分平均值为An_(0.94)Ab_(98.01)Or_(1.06),类似于火山岩中钠长石端员组分变化范围(An=0.74~6.75,Ab=92.85~98.91,Or=0.32~1.76,端员组分平均值为An_(2.63)Ab_(96.65)Or_(0.72)),两者均为岩浆成因钠长石,而非热液交代成因钠长石。富铁基质成分变化范围较大且连续(w(SiO_2)为0.08%~50.04%,w(FeO)为24.89%~87.13%,w(Al_2O_3)为0.04%~14.83%,w(TiO_2)为0.01%~2.83%,w(Na_2O)为0~9.76%,w(MgO)为0.03%~4.88%,w(MnO)为0~0.61%),富铁基质中高Ti磁铁矿和低Ti磁铁矿同时发育,总体上成分不均一,且钠长石呈细针状,为浅成-超浅成低压下快速结晶的产物或为火山喷发作用下快速冷凝结晶所致。通过对磁铁矿-磷灰石矿物组合与安山岩中副矿物磷灰石、矿区磁铁矿的对比研究,认为智博铁矿发生磁铁矿-磷灰石岩浆不混溶作用的可能性很小。通过安山岩基质成分与安山岩成分的对比研究,得出安山岩基质比原岩w(SiO_2)、w(Al_2O_3)、w(CaO)有所降低,w(FeO)、w(Na_2O)、w(MgO)有一定升高,但是程度有限,表明岩浆结晶分异不足以使残留岩浆形成富铁矿。钠长石-磁铁矿富铁岩屑的发育是一种碱铁效应的表现,而碱铁效应对于海相火山岩型铁矿的形成具有重要意义。  相似文献   

12.
智博铁矿床位于新疆西天山阿吾拉勒成矿带东段,主要赋矿围岩为石炭系大哈拉军山组安山岩、玄武质安山岩和火山碎屑岩.该矿床主要有东、中、西3个矿区,其中以东矿区为主矿区.矿体主要呈层状、似层状、厚板状和透镜状.金属矿物以磁铁矿为主,含有少量黄铁矿、赤铁矿和黄铜矿.矿石构造以块状和浸染状构造为主,此外还有角砾状构造、条带状构造...  相似文献   

13.
岩浆-热液系统中铁的富集机制探讨   总被引:8,自引:17,他引:8  
与岩浆-热液系统有关的铁矿类型有岩浆型钒钛磁铁矿床、玢岩铁矿、矽卡岩型铁矿和海相火山岩型铁矿,与这些铁矿有关的岩浆岩从基性-超基性、中性到中酸性岩均有,其中岩浆型钒钛磁铁矿床与基性-超基性深成侵入岩有关,形成于岩浆阶段,主要与分离结晶作用有关,但是厚大的富铁矿石的形成则可归结于原始的富铁钛苦橄质岩浆、分离结晶作用、多期次的岩浆补充以及流动分异等联合过程。钒钛磁铁矿石产于岩体下部还是上部与母岩浆的氧逸度有关:高的氧逸度导致磁铁矿早期结晶而使得其堆积于岩体的下部,相反,低氧逸度则导致低品位的浸染状矿石产于岩体的上部。虽然野外一些证据表明,元古宙斜长岩中的磷铁矿石可能是不混溶作用形成的,但是目前尚无实验证据。某些玢岩铁矿的一些磷灰石-磁铁矿石可能与闪长质岩浆同化混染了地壳中的磷导致的不混溶作用有关。除此之外,其他各类与岩浆作用有关的铁矿床均与岩浆后期的岩浆-热液作用有关。这些不同类型铁矿床的蚀变和矿化过程具有相似性,反映了它们形成过程具有相似的物理化学条件。成矿实验以及流体包裹体研究表明,岩浆-流体转换过程中出溶流体的数量以及成分受多种因素控制,其中岩浆分离结晶作用以及碳酸盐地层和膏盐层的混染可导致出溶的流体中Cl浓度的升高。早期高氧逸度环境可以使得硫以SO42-形式存在,抑制硫与铁的结合形成黄铁矿,有利于铁在早期以Cl的络合物发生迁移。大型富铁矿的形成需要一个长期稳定的流体对流循环系统,而岩浆的多期侵位或岩浆房以及在相对封闭的环境中(需要一个不透水层)一个有利于流体循环的断裂/裂隙系统是形成一个长期稳定的流体对流循环系统的必要条件。但是由于不同地质环境,流体中铁的卸载方式和位置会有明显差别,由此导致不同的矿石结构构造和不同的矿体产状。  相似文献   

14.
通过龙游晚中生代基性岩岩相学观察、全岩主量、微量元素和Sr-Nd同位素及矿物电子探针分析,对岩石成因、岩浆演化和构造环境进行探讨。龙游基性岩岩性为橄榄辉长岩,Sr-Nd同位素显示为幔源特征;主量、微量元素特征显示其经历了以橄榄石、辉石为主的分离结晶作用,且未发生明显的地壳物质混染。橄榄石颗粒具核-边结构,富Mg贫Fe的核部Fo值为90.1~91.8,指示原始岩浆是软流圈地幔,富Fe贫Mg的边部显示橄榄石Fo值为77.4~85.3,且核-边两部分的Fo值相差较大,显示原始橄榄石形成之后受到地幔熔体/流体的交代作用。辉石斑晶大多属于透辉石,在部分斑晶的边部发育少量霓辉石。透辉石斑晶普遍具有核-幔-边结构,从核部到边部的SiO_2含量降低,TiO_2、Al_2O_3含量升高,结晶温度升高,显示原始辉石形成之后受到温度更高的地幔熔体/流体的交代作用。研究认为,古太平洋板块后撤造成岩石圈地幔拉伸作用并形成赣杭构造带深部断裂后,部分软流圈物质受到地幔流体/熔体的交代作用,并沿这些深部断裂向上侵位,经历了以橄榄石和辉石矿物为主的分离结晶作用和微弱的地壳物质混染,最终形成龙游橄榄辉长岩。  相似文献   

15.
We present petrography and mineral chemistry for both phlogopite,from mantle-derived xenoliths(garnet peridotite,eclogite and clinopyroxene-phlogopite rocks)and for megacryst,macrocryst and groundmass flakes from the Grib kimberlite in the Arkhangelsk diamond province of Russia to provide new insights into multi-stage metasomatism in the subcratonic lithospheric mantle(SCLM)and the origin of phlogopite in kimberlite.Based on the analysed xenoliths,phlogopite is characterized by several generations.The first generation(Phil)occurs as coarse,discrete grains within garnet peridotite and eclogite xenoliths and as a rock-forming mineral within clinopyroxene-phlogopite xenoliths.The second phlogopite generation(Phl2)occurs as rims and outer zones that surround the Phil grains and as fine flakes within kimberlite-related veinlets filled with carbonate,serpentine,chlorite and spinel.In garnet peridotite xenoliths,phlogopite occurs as overgrowths surrounding garnet porphyroblasts,within which phlogopite is associated with Cr-spinel and minor carbonate.In eclogite xenoliths,phlogopite occasionally associates with carbonate bearing veinlet networks.Phlogopite,from the kimberlite,occurs as megacrysts,macrocrysts,microcrysts and fine flakes in the groundmass and matrix of kimberlitic pyroclasts.Most phlogopite grains within the kimberlite are characterised by signs of deformation and form partly fragmented grains,which indicates that they are the disintegrated fragments of previously larger grains.Phil,within the garnet peridotite and clinopyroxene-phlogopite xenoliths,is characterised by low Ti and Cr contents(TiO_21 wt.%,Cr_2 O_31 wt.% and Mg# = 100 × Mg/(Mg+ Fe)92)typical of primary peridotite phlogopite in mantle peridotite xenoliths from global kimberlite occurrences.They formed during SCLM metasomatism that led to a transformation from garnet peridotite to clinopyroxene-phlogopite rocks and the crystallisation of phlogopite and high-Cr clinopyroxene megacrysts before the generation of host-kimberlite magmas.One of the possible processes to generate low-Ti-Cr phlogopite is via the replacement of garnet during its interaction with a metasomatic agent enriched in K and H_2O.Rb-Sr isotopic data indicates that the metasomatic agent had a contribution of more radiogenic source than the host-kimberlite magma.Compared with peridotite xenoliths,eclogite xenoliths feature low-Ti phlogopites that are depleted in Cr_2O_3 despite a wider range of TiO_2 concentrations.The presence of phlogopite in eclogite xenoliths indicates that metasomatic processes affected peridotite as well as eclogite within the SCLM beneath the Grib kimberlite.Phl2 has high Ti and Cr concentrations(TiO_22 wt.%,Cr_2O_31 wt.% and Mg# = 100× Mg/(Mg + Fe)92)and compositionally overlaps with phlogopite from polymict brecc:ia xenoliths that occur in global kimberlite formations.These phlogopites are the product of kimberlitic magma and mantle rock interaction at mantle depths where Phl2 overgrew Phil grains or crystallized directly from stalled batches of kimberlitic magmas.Megacrysts,most macrocrysts and microcrysts are disintegrated phlogopite fragments from metasomatised peridotite and eclogite xenoliths.Fine phlogopite flakes within kimberlite groundmass represent mixing of high-Ti-Cr phlogopite antecrysts and high-Ti and low-Cr kimberlitic phlogopite with high Al and Ba contents that may have formed individual grains or overgrown antecrysts.Based on the results of this study,we propose a schematic model of SCLM metasomatism involving phlogopite crystallization,megacryst formation,and genesis of kimberlite magmas as recorded by the Grib pipe.  相似文献   

16.
A variety of rock types is developed in the Shonkin Sag laccolith, with extreme compositions represented by the porphyritic pseudoleucite-bearing chilled margin, shonkinitic in composition, and by the final differentiate, chemically a nepheline syenite. During differentiation the pyroxenes changed in composition from Ca-rich varieties through aegirine-augite to acmite; there is no evidence of an immiscibility gap between Ca-rich and Na-rich pyroxenes. Olivine compositions changed from approximately Fa20 to Fa40, but in marked contrast the coexisting biotites exhibit a more extensive compositional range, from annite24 to annite100; the crystal margins of annites in the most evolved rocks are manganophyllite-rich. Titanomagnetites are TiO2-poor varieties. Arfvedsonite and melanite occur in the most evolved syenites.From mineralogical and thermodynamic data initial and final temperatures of crystallization of the various rock types have been calculated. At an estimated total vapor pressure of 310 bars, the temperature of intrusion was 985° C. Final crystallization of the laccolith took place below 700° C, and crystallization intervals for most rock types are of the order of 170° C. Over the total magmatic temperature range the activity of silica in the melt decreased from 0.13 to 0.09. Oxygen fugacity falls with temperature approximately parallel to the synthetic fayalite-magnetite-quartz oxygen buffer until olivine disappears. The crystallization of Na-rich pyroxenes does not demand an increase in the fugacity of oxygen, but rather requires that the oxygen fugacity fall less rapidly with temperature than would be the case if olivine and magnetite were present.  相似文献   

17.
甘肃北山黑山岩浆铜镍硫化物矿床橄榄石特征及成因意义   总被引:5,自引:2,他引:5  
黑山铜镍硫化物矿床是近年在甘肃北山发现的大型岩浆铜镍硫化物矿床,含矿岩体主要由含矿橄榄岩相和南部边缘的角闪辉长岩相构成。研究发现含矿岩体中的橄榄石属贵橄榄石(Fo值为81.54~86.87),其w(Ni)介于(801.53~2 703.19)×10-6;利用橄榄辉长岩中最高Fo值和主量元素反演,表明原始岩浆属高镁玄武质岩浆,w(MgO)=11.65%,w(FeO)=10.12%;橄榄石分离结晶模拟计算结果表明,橄榄石结晶过程中伴随有0.12%~0.17%硫化物熔离,深部岩浆房中橄榄石分离结晶程度小于3%,橄榄石与硫化物最小质量比约14∶1;隙间硅酸盐熔浆和硫化物熔浆作用明显,是造成早期结晶橄榄石成分变化的重要原因。  相似文献   

18.
The key mineralogical features of the Newania carbonatites, that illustrate their derivation from primary mantle melts (Gruau et al. Terra Nova, Abstract Suppl 1:336, 1995; Viladkar Petrology 6(3):272–283, 1998; Basu and Murty Abstracts of Goldschmidt Conference A40, 2006), are the presence of magnesite, graphite and Cr-rich magnetite. Magnesite is an early crystallizing phase. Cr-rich magnetite and graphite coexist with carbonatite minerals and precipitated from carbonate magma. Graphite, as well as gaseous CO2 and carbonate minerals such as dolomite and magnesite, can be stable in peridotite mantle. Coexistence of these minerals is controlled by fO 2 and PT-conditions. Mineral geothermometers for the Newania carbonatite give temperatures from 463 to 950°C. The parental source for Newania carbonatites was characterized by a relatively high log (fHF/fH2O) level which increased during the crystallization history of Newania. The estimated oxygen fugacity (for ilmenite–magnetite pairs) varies from ?1.5 to +3.5 (log-bar unit deviation from FMQ buffer), which is supported by the presence of Fe-columbite, and the composition of phlogopite, amphibole and pyroxene that have an elevated concentration of Fe3+. However, the oxygen fugacity range represented by co-existing early-crystallized graphite and magnesite is below that of the FMQ buffer and lies on the CCO buffer.  相似文献   

19.
新疆巴楚小海子是近年来在塔里木大火成岩省探获的一个低品位-大吨位岩浆型钒钛磁铁矿床,其成岩成矿机制以及资源利用前景尚不清楚。文章针对小海子岩体2种含矿岩相橄榄辉长岩和橄榄辉石岩开展了地质地球化学研究。橄榄辉长岩相和橄榄辉石岩相虽然在空间上关系不明,但岩相学观察表明它们矿物组成的差异与矿物堆晶作用有关,且二者具有相似的稀土元素球粒陨石标准化和微量元素原始地幔标准化配分曲线,说明是同源岩浆演化的产物,橄榄石较低的Fo值(67.9~72.5)指示幔源母岩浆在深部岩浆房中发生了分异。小海子岩体和与相距约45 km的瓦吉里塔格相比,岩石组成和地球化学组成相似,表明为同源岩浆成因,但后者矿物组成变化范围更大,指示瓦吉里塔格岩体在形成过程中经历了更高程度的分离结晶作用,这可能是造成瓦吉里塔格岩体比小海子岩体的w(TiO2)更高的原因。小海子岩体虽然w(TiO2)较低(3%~4%),但铁钛氧化物固溶体分离结构不发育,且矿物颗粒粗大,使得铁和钛选矿解离比中国其他地区的钒钛磁铁矿更为容易,因此钛资源利用前景巨大,笔者建议出台地方性的勘查技术规范,为这类铁钛资源的开发利用提供技术标准。  相似文献   

20.
The equilibrium phase relations of a mafic durbachite (53 wt.% SiO2) from the Třebíč pluton, representative of the Variscan ultrapotassic magmatism of the Bohemian Massif (338–335 Ma), have been determined as a function of temperature (900–1,100°C), pressure (100–200 MPa), and H2O activity (1.1–6.1 wt.% H2O in the melt). Two oxygen fugacity ranges were investigated: close to the Ni–NiO (NNO) buffer and 2.6 log unit above NNO buffer (∆NNO + 2.6). At 1,100°C, olivine is the liquidus phase and co-crystallized with phlogopite and augite at 1,000°C for the whole range of investigated pressure and water content in the melt. At 900°C, the mineral assemblage consists of augite and phlogopite, whereas olivine is not stable. The stability field of both alkali feldspar and plagioclase is restricted to low pressure (100 MPa) at nearly water-saturated conditions (<3–4 wt.% H2O) and T < 900°C. A comparison between experimental products and natural minerals indicates that mafic durbachites have a near-liquidus assemblage of olivine, augite, Ti-rich phlogopite, apatite and zircon, followed by alkali feldspar and plagioclase, similar to the mineral assemblage of minette magma. Natural amphibole, diopside and orthopyroxene were not reproduced experimentally and probably result from sub-solidus reactions, whereas biotite re-equilibrated at low temperature. The crystallization sequence olivine followed by phlogopite and augite reproduces the sequence inferred in many mica-lamprophyre rocks. The similar fractionation trends observed for durbachites and minettes indicate that mafic durbachites are probably the plutonic equivalents of minettes and that K- and Mg-rich magmas in the Bohemian Massif may have been generated from partial melting of a phlogopite–clinopyroxene-bearing metasomatized peridotite. Experimental melt compositions also suggest that felsic durbachites can be generated by simple fractionation of a more mafic parent and mixing with mantle-derived components at mid crustal pressures.  相似文献   

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