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1.
冀北赤城红旗营子群黑云斜长片麻岩的岩石学、地球化学及原岩特征 总被引：1，自引：0，他引：1
冀北赤城红旗营子群黑云斜长片麻岩具斑状变晶结构,变基质为中、细粒鳞片粒状变晶结构,片麻状构造,局部保留有变余砂状结构。岩石主要由斜长石(28%~32%)、石英(35%~40%)、黑云母(18%~25%)及少量石榴石(2%~8%)和石墨(1%~4%)等组成,其变质演化可能是一个降温、降压的过程。黑云斜长片麻岩样品具有较宽的常量元素变化范围,稀土元素含量不是很高且变化较大,ΣREE介于49.45×10-6~140.10×10-6之间,具有轻稀土富集、重稀土平坦的球粒陨石标准化稀土配分模式,轻、重稀土元素比值为5.23~9.16,(La/Yb)CN值为5.07~8.70。大多数样品具中等程度的负Eu异常和不太明显的负Ce异常,(Eu/Eu*)CN和(Ce/Ce*)CN值分别为0.63~0.81和0.82~1.01。岩石中Rb、Sr、Cs、Ba、Zr、Hf、Nb、Ta、Th和U等微量元素含量均低于上地壳的平均含量,但Sr/Ba和Th/U值高于上地壳的平均值。红旗营子群黑云斜长片麻岩的地球化学特征表明其原岩应为泥质(或含泥质)砂岩,可能形成于大陆岛弧环境。 相似文献
2.
中国大陆科学钻探工程主孔2000～3000米正、副片麻岩的地球化学性质及其成因机制 总被引：9，自引：7，他引：9
中国大陆科学钻探工程主孔(CCSD-MH)2000.0-3000.0米深度范围内出露的岩心以正、副片麻岩为主,夹有薄层榴辉岩和斜长角闪岩等。地球化学研究结果表明,主孔20000.0-3000.0米之间的正片麻岩SiO2含量普遍偏高,为73.26%～78.17%之间,平均值76.40%;Al2O3含量为11.30%-13.66%。TiO2、Fe2O3、FeO、MnO和MgO含量则明显偏低,其中Fe2O3总量为0.39%-1.71%,FeO=0.20%-1.49%,MgO=0.01%-0.06%。CaO含量为0.19-1.41%,Na2O和K2O含量分别为3.38%-5.35%和1.31%-4.87%。正片麻岩的稀土元素和微量元素配分模式可分为三种类型。第一类表现出较强的轻、重稀土元素分馏,具有中等的负Eu异常,Eu/Eu*=0.39-0.64;洋脊玄武岩(MORB)标准化蛛网图表现出强烈富集大离子亲石元素(K、Rb、Ba、Th)的特点,显示明显的正Ba异常,Ba/Ba*=1.09-2.34,高场强元素Ti、Nb和Ta呈明显的负异常。第二类正片麻岩具有明显的负Eu异常,Eu/Eu*=0.39-0.41,稀土元素配分曲线具有明显右倾斜的特点,轻稀土元素明显富集,而重稀土元素明显亏损;洋脊玄武岩(MORB)标准化蛛网图与第一类正片麻岩比较相似,但却具有中等的负Ba异常,Ba/Ba*=0.57-0.67。第三类正片麻岩主要为含磁铁矿二长花岗质片麻岩,稀土元素球粒陨石标准化曲线呈“V”字型特点,具有异常强烈的负Eu异常,Eu/Eu*普遍低于0.11;洋脊玄武岩(MORB)标准化蛛网图显示出强烈富集大离子亲石元素(K、Rb、Th)的特点,具有异常强烈的负Ba异常,Ba/Ba*=0.03-0.21。2000.0-3000.O米深度范围内的正片麻岩具有多成因的特点,部分正片麻岩具有A型花岗岩的地球化学特征,反映它们有可能形成于板内的构造环境;而另一部分的原岩则可能形成于陆缘火山弧的构造环境。主孔2000.0-31000.0米深度范围内副片麻岩SiO2含量明显低于正片麻岩,Al2O3、Fe2O3 FeO、MgO和CaO含量则明显偏高,而Na2O和K2O含量则与正片麻岩大体相当。其中SiO2含量为64.21%-74.12%;Al2O3含量为13.06%-15.38%,Fe2O3 FeO含量为1.61%-4.92%;CaO含量为1.10%～3.27%,Na2O和K2O含量分别为3.68%-5.39%和2.46%-5.85%。副片麻岩稀土元素配分模式和洋脊玄武岩(MORB)标准化蛛网图与正片麻岩也存在明显差异。其中稀土元素配分模式表现出一定程度的轻、重稀土元素分馏,大多数样品具负Eu异常,Eu/Eu*=0.56-0.93之间,但远不及正片麻岩的明显;洋脊玄武岩(MORB)标准化蛛网图则显示出富集大离子亲石元素(K、Rb、Ba、Th)的特点,具有异常明显的正Ba异常,且变化范围较大,Ba/Ba*=1.02-4.83之间,高场强元素如Ti、Nb和Ta呈现负异常的特点。副片麻岩的原岩可能是形成于被动大陆边缘的一套典型的沉积岩或变沉积岩。SHRIMPU-Pb定年结果表明,主孔副片麻岩锆石微区记录了十分复杂的年代学信息。继承性碎屑锆石核部的年龄(206Pb/238U的年龄)为313-659Ma,表明原岩继承性碎屑锆石来源的复杂性,以及部分碎屑锆石在超高压变质过程中发生不完全重结晶,导致年龄变新;在含柯石英锆石微区记录的超高压变质年龄(206Pb/238U的年龄)为220-236Ma,加权平均值为227±5Ma;而锆石晶体边部所记录的退变质年龄(206Pb/238U的年龄)为209-219Ma,加权平均值为214±6Ma,上述含柯石英锆石微区和锆石边部的SHRIMPU-Pb定年结果分别与主孔CCSD-MH中的正片麻岩锆石微区获得的超高压变质年龄(227±2Ma)和角闪岩相退变质年龄(209±3Ma)十分接近,这进一步证明了中国大陆科学钻探工程主孔中的正、副片麻岩的原岩曾一起发生深俯冲,并经历了新三叠纪的超高压变质作用。 相似文献
3.
蒙古-鄂霍茨克洋俯冲的记录：额尔古纳地区八大关变质杂岩的证据 总被引：4，自引：1，他引：3
本文对额尔古纳地块西缘八大关杂岩进行了锆石LA-ICP-MS U-Pb定年和岩石地球化学分析,以确定该套杂岩的形成时代及其构造属性。原定义为"佳疙瘩组"的八大关杂岩主要由黑云角闪斜长片麻岩和花岗质糜棱岩组成。LA-ICP MS锆石U-Pb研究表明,3个样品的锆石发育典型的岩浆振荡环带,高Th/U(0.13~1.42),轻稀土元素亏损,重稀土元素富集,具有强烈的正Ce异常和强烈的负Eu异常等特征,表明锆石均属于岩浆成因。测年结果表明2个黑云角闪斜长片麻岩形成时代分别为210±2Ma、214±2Ma,花岗质糜棱岩的原岩年龄为203±3Ma;样品中同时存在~501Ma和~795Ma的捕获/继承锆石。上述结果显示八大关杂岩的形成时代应为晚三叠世而不是前人认为的新元古代,而捕获锆石则显示与东北其它地块具有相同的构造演化历史。地球化学研究显示,八大关杂岩具有高钠、铝等特点,A/CNK=0.86~1.05,A/NK=1.53~1.97,为准铝质到弱过铝质钙碱性系列;轻稀土元素富集、重稀土元素亏损(La/Yb)N=6~31,Eu弱亏损(Eu/Eu*=0.50~1.01),具有较高的Sr含量(在378×10-6~598×10-6之间)及低的Yb含量(在0.71×10-6~3.50×10-6之间);微量元素原始地幔标准化蛛网模式图显示,富集Rb、Ba、K及Sr等大离子亲石元素、强烈亏损Nb、Ta、P、Ce及Ti等高场强元素。这些地球化学特征表明八大关杂岩形成于活动大陆边缘的岛弧环境。因此,八大关杂岩应形成于蒙古-鄂霍茨克洋向额尔古纳地块俯冲的大地构造背景,为蒙古-鄂霍茨克洋在三叠纪晚期南向俯冲提供了关键证据。 相似文献
4.
冀东杏山BIF铁矿形成时代及成因探讨 总被引：2，自引：2，他引：0
杏山BIF型铁矿位于冀东曹庄一带,矿体赋存于太古界三屯营组变质岩系中。矿石多为条纹-条带状构造,其围岩和夹层以斜长角闪岩为主,兼具少量黑云石英片岩和黑云钾长片麻岩。对BIF铁矿进行的地球化学分析表明,条带状铁矿石富集重稀土((La/Yb)*PAAS平均0.46),Eu正异常(Eu/Eu*PAAS平均2.19)、La正异常(La/LaPAAS平均2.14)和Y的正异常(Y/Y*PAAS平均1.85)明显,加之高的Y/Ho值(平均46.81),说明成矿物质来源于海底高温热液与周围海水的混合溶液;无Ce的负异常说明BIF形成于低氧逸度环境;BIF显示较低的Al2O3和TiO 2含量,且二者缺乏相关性,说明在BIF沉淀过程中几乎没有陆源碎屑物的加入。对矿体围岩斜长角闪岩、黑云石英片岩及黑云钾长片麻岩的原岩恢复,表明斜长角闪岩的原岩为玄武岩-安山质玄武岩,黑云石英片岩及黑云钾长片麻岩的原岩可能为泥质碎屑岩。元素地球化学分析表明,黑云钾长片麻岩具有较低的总稀土含量(59.46×10-6~66.99×10-6)、不明显的Eu负异常(Eu/Eu*=0.77~0.91)、略微的Th和U富集、无Nb和Ta的亏损;而黑云石英片岩具有较高的稀土总量(168.7×10-6~171.0×10-6)、强烈的轻稀土富集((La/Yb)N=6.81~7.07)和较弱的Eu负异常(Eu/Eu*=0.64~0.68),两者不一致的地球化学特征说明他们具有不同的物质来源。斜长角闪岩与N-MORB具有相似的特征,如富集大离子亲石元素(LILEs),亏损Th和U、Nb、Ta、Ti、Zr和Hf等无明显亏损。综合分析表明斜长角闪岩的母岩浆来源于尖晶石二辉橄榄岩30%的部分熔融,且其母岩浆在分异结晶过程中可能受到陆壳物质的混染。对矿体夹层斜长角闪岩LA-ICP-MS锆石U-Pb定年,结果表明其原岩形成于2859±22Ma至2491±13Ma之间,最有可能形成于新太古代晚期,这间接约束了杏山BIF型铁矿的形成时代,暗示着迁西岩群主体可能仍形成于新太古代晚期。而2859±22Ma的捕掳锆石年龄反映杏山-曹庄地区可能存在有中太古代表壳岩。 相似文献
5.
出露于阿中地块库木塔什萨依一带的亚干布阳片麻岩主要岩性为黑云斜长片麻岩、黑云二长片麻岩。利用LA-ICPMS方法进行锆石微区U-Pb同位素定年,得到206Pb/238U年龄加权平均值为900.2±2.9Ma,表明亚干布阳片麻岩原岩形成于新元古代早期青白口纪;地球化学结果显示,主量元素具有高SiO_2、Al_2O_3、K_2O+Na_2O含量,低Na_2O、MgO、CaO和TiO_2含量的特征,A/CNK值介于0.95～1.22之间,属于高钾钙碱性系列的过铝质花岗岩。岩石富集Rb、Th、K等大离子亲石元素,亏损Nb、Sr、P、Hf、Ti等高场强元素;岩石轻稀土元素分馏较强而重稀土元素分馏较弱,具有明显的负Eu异常,总体呈右倾的"V"字形稀土元素配分模式,显示典型的地壳重熔型花岗岩特征。亚干布阳片麻岩的源岩主要为地壳中沉积岩类的部分熔融,形成于俯冲-同碰撞构造环境。综上说明亚干布阳片麻岩是新元古代早期俯冲碰撞热事件的产物,反映阿中地块和柴达木地块青白口纪处于汇聚碰撞阶段,构造岩浆活动强烈,与Rodinia超大陆汇聚事件具有一致性。 相似文献
6.
马拉苏地区早泥盆世地层为一套滨海—浅海相火山—沉积岩系,对其中的火山岩夹层进行锆石U-Pb同位素定年和岩石地球化学研究,定年结果显示有大量的新太古代和中新元古代锆石,表明该区存在古老的大陆地壳物质。火山岩样品Si O2含量为52.38%~69.6%,Na2O含量为2.80%~4.85%,K2O为0.16%~0.96%,Ti O2为0.5%~1.96%,Al2O3为14.62%~18.18%,Mg O(1.08%~5.75%)变化范围较大,Mg#值在22.92~38之间,具有高钠、低钾的特征,属于钙碱性、低钾拉斑系列。稀土元素总量∑REE=73×10-6~115×10-6,LREE/HREE值为2.66~3.25,具有明显的Eu负异常(0.83~0.92)。玄武安山岩样品相对富集K、Rb、Ba、Sr等大离子亲石元素,亏损Nb、Ta、Zr、Hf等高场强元素,与典型火山弧玄武岩地球化学特征一致。英安斑岩样品也具有富集大离子亲石元素、亏损Nb、Ta、Ti等高场强元素的特征,反映源区可能有较多壳源物质的加入,其稀土元素配分曲线和微量元素蛛网图与玄武安山岩相似,表明其可能为同源岩浆演化的产物。综合研究认为,这套火山岩具有岛弧火山岩特征,形成于板块俯冲拼贴过程中的岛弧环境。 相似文献
7.
华北克拉通阜平杂岩中~2.7GaTTG片麻岩的厘定及其地质意义 总被引：7，自引：7，他引：0
通过详细的地质工作,本文从阜平杂岩中厘定出一套~2.7Ga的条带状TTG片麻岩系,其原岩主要为英云闪长岩,经历了强烈的变形和深熔改造。该片麻岩可分为岩石主体和条带,按条带形态和成分可分为三种:细小的暗色条带、深熔浅色条带和后期注入的长英质脉体。用LA-MC-ICPMS法对英云闪长岩中锆石进行了原位U-Pb年龄测试,其形成年龄为2669.2±9.7Ma。该片麻岩SiO2=64.32%~70.02%,具有高铝(Al2O3=14.00%~15.87%)富钠(Na2O=3.85%~4.22%)贫钾(K2O=1.13%~2.42%)及低K/Na比值的特点,Mg#指数为39.5~49.6。该片麻岩具有中等-强烈程度的稀土元素分异[(La/Yb)N=3.67~51.38],Eu异常不明显。其富集Sr(303×10-6~431×10-6)、Ba(191×10-6~696×10-6)等大离子亲石元素,亏损Nb(4.70×10-6~9.78×10-6)、Ta(0.19×10-6~0.75×10-6)、Ti(1378×10-6~3259×10-6)、P(174.6×10-6~960.6×10-6)等高场强元素,Cr(5.87×10-6~119.4×10-6)、Ni(6.72×10-6~45.75×10-6)等相容元素含量也较低。Yb(0.31×10-6~1.75×10-6)和Y(3.61×10-6~18.88×10-6)含量低,Sr/Y比值高(16.0~119.1),属于高铝的TTG,与高硅埃达克岩特征相似。推断是热的太古宙新生洋壳部分熔融而成。阜平地区~2.7Ga TTG片麻岩的厘定,进一步证实了华北克拉通在新太古代早期经历了强烈的陆壳增生,并为华北克拉通早期岩浆事件与世界范围的岩浆事件的对比提供了新的依据,为华北克拉通早期陆块及绿岩带的划分提供了新的限定。 相似文献
8.
赤峰蒙古营子岩体位于华北板块以北的兴蒙造山带南端,岩性主要为花岗闪长岩。其Si O2含量介于56.88%~68.82%之间,Na2O含量为4.32%~4.54%,K2O含量为2.3%~3.86%,且Na2OK2O。里特曼指数σ=2.4~3.29,Al2O3含量介于15.1%~16.8%之间,A/CNK=0.81~0.92,属于高钾钙碱性I型花岗岩。富集轻稀土元素(LREE)、亏损重稀土元素(HREE)和高场强元素(HFSE)。Sr含量为782×10-6~1230×10-6,Y和Yb平均值分别为20.1×10-6和1.77×10-6,(La/Yb)N值为19.84~22.03,δEu=0.81~1.04,Eu异常不明显。岩体总体显示出C型埃达克岩的地球化学属性,暗示岩浆可能源于加厚的下地壳部分熔融。采用LA-ICP-MS技术测得的锆石206Pb/238U年龄为252.8±2.4Ma,表明该岩体形成于古生代末期—早中生代。结合兴蒙造山带的构造演化历史,认为蒙古营子花岗闪长岩应为西伯利亚板块和华北板块后碰撞阶段的产物,具有幔源岩浆底侵诱发地壳生长的指示意义。 相似文献
9.
滇西双江勐库地区新发现的退变质榴辉岩呈构造透镜体产于奥陶纪湾河蛇绿混杂岩的白云母构造片岩内,勐库地区是目前云南省境内唯一退变质榴辉岩产地。岩石地球化学分析结果显示,退变质榴辉岩的SiO2含量为4722%~5040%,全碱(Na2O+K2O)含量为228%~415%,Al2O3含量为1370%~1558%,TiO2含量为139%~395%,可分为中Ti(139%~183%)和高Ti(330%~395%)两种类型。退变质榴辉岩的主要原岩是拉班玄武岩,少部分具碱性玄武岩特征。多数原岩为拉斑玄武岩的样品具TiO2含量高、Eu异常不明显及缓右倾稀土元素配分模式特征,其稀土元素配分模式和微量元素蛛网图特征均与E MORB相似而与N MORB不同,投在MORB和E MORB范围,推测其原岩很可能形成于E MORB环境;少部分原岩为碱性玄武岩的样品,其TiO2含量中等,较原岩为拉斑玄武岩样品具更高的ΣREE和ΣLREE含量,投在OIB范围,推测其原岩可能形成于OIB环境。勐库地区退变质榴辉岩样品的岩石地球化学特征与其赋存的奥陶纪湾河蛇绿岩颇为相似,暗示可能是其俯冲消减作用的产物。此外,研究样品同时具有E MORB和OIB的特征,且与青藏高原羌塘中部榴辉岩相似,表明在特提斯洋演化过程中地幔柱岩浆和正常洋中脊亏损地幔岩浆的相互作用可能是广泛存在的。 相似文献
10.
中亚造山带东段南缘早志留世岩体锆石U-Pb定年、地球化学特征及其地质意义 总被引：6，自引：4，他引：2
本文报道了分布于中亚造山带南缘苏尼特右旗太古生庙地区太古生庙岩体和库伦哈达岩体的岩相学、地球化学和年代学特征,以讨论该岩体的形成时代、岩石成因及其构造环境。锆石U-Pb定年结果显示,太古生庙英云闪长岩结晶年龄为442.6±2.4Ma,库伦哈达石英闪长岩结晶年龄为434.2±2.2Ma,说明太古生庙地区早古生代存在岩浆活动。其中太古生庙岩体地球化学特征类似于典型的埃达克岩,其Si O2含量56%(70.02%~70.51%),Al2O3含量≥15%(15.99%~16.37%),Mg O3%(0.56%~0.83%),Na2O3%(4.33%~4.66%),K2O/Na2O比值0.5(0.3~0.4);在微量元素特征方面,Sr400×10-6(681×10-6~783×10-6),Yb1.9×10-6(0.6×10-6~0.9×10-6),Y18×10-6(5.4×10-6~9.3×10-6),无明显的Eu异常。库伦哈达岩体与太古生庙岩体相比,Si O2含量较低(57.92%~66.78%),Al2O3为相当(14.91%~18.26%),MgO含量为1.17%~2.31%,Na2O含量为3.29%~4.36%,K2O含量为1.43%~3.09%;在微量元素判别图解中,库伦哈达岩体的岩石样品投图位于埃达克岩和典型的岛弧型火山岩的叠加区域,而太古生庙岩体样品全部落入埃达克岩区域内,太古生庙岩体可能是洋壳部分熔融的产物,而库伦哈达岩体可能是早期俯冲的洋壳部分熔融的产物混染了部分熔融的地幔楔之后形成了这种具有正常岛弧岩浆特征的岩石,其形成的环境为岛弧环境。 相似文献
11.
Through detailed studies we have delineated a suite of banded TTG gneisses from the Zanhuang Complex. The protolith of the gneisses, predominantly tonalite, has undergone intensive metamorphism, deformation and anatexis and in a banded structure is intimately associated with melanocratic dioritic gneiss and leucocratic trondhjemitic veins. SHRIMP Zircon U–Pb data show that the tonalite was formed ca. 2692 ± 12 Ma ago. The tonalitic gneiss has the features of high SiO2 (67.76–73.31%), high Al2O3 (14.38–15.83%), rich in Na2O (4.48–5.07%) and poor in K2O (0.77–1.93%). The gneiss is strongly fractioned in REE ((La/Yb)N = 12.02–24.65) and shows a weak positive Eu anomaly (Eu/Eu* = 1.05–1.64). It has high contents of Ba (199–588 ppm) and Sr (200–408 ppm), low contents of Yb (0.32–1.00 ppm) and Y (3.41–10.3 ppm) with high Sr/Y ratios (21.77–96.77) and depletion in HFSE Nb, Ta and Ti. These characteristics are similar to those of the high-Si adakitic rocks. The melanocratic dioritic gneiss has low SiO2 (59.81%), high MgO (6.34%), high Al2O3 (14.02%) contents, rich in Na2O (3.7%) and poor in K2O (1.79%), with high Mg index (Mg# = 67). REE and trace elements are on the whole similar to that of the tonalitic gneiss, but compatible element abundances V (116 ppm), Cr (249 ppm), Co (37 ppm) and Ni (179 ppm) are higher. The leucocratic felsic bands (approximating trondhjemite in composition) have major oxides similar to that of the TTG gneisses but the REE and compatible elements are extremely low, which are indicative of the products of anatexis. The tonalitic gneiss has positive εNd(t) (2.37–3.29) and low initial Sr (0.69719–0.70068) values with depleted mantle Nd model age of ca. 2.8 Ga, suggesting its generation from partial melting of mantle-derived juvenile crust. The dioritic gneiss was also derived from subduction environment, but has undergone significant metasomatism of mantle wedge. The delineation of the ca. 2.7 Ga TTG gneisses in the Zanhuang Complex further proves that the North China Craton experienced large-scale continental crustal accretion in early Neoarchean, and gives new constraints on the subdivision of the early blocks and greenstone belts of the craton. 相似文献
12.
The bimodal suite (BMS) comprises leucotonalitic and trondhjemitic gneisses interlayered with amphibolites. Based on geochemical parameters three main groups of siliceous gneiss are recognized: (i) SiO2 < 73%, Al2O3 > 14%, and fractionated light rare-earth element (REE) and flat heavy REE patterns; (ii) SiO2 and Al2O3 contents similar to (i) but with strongly fractionated REE patterns with steep heavy REE slopes; (iii) SiO2 > 73%, Al2O3 < 14%, Zr ～ 500 ppm and high contents of total REE having fractionated light REE and flat heavy REE patterns with large negative Eu anomalies. The interlayered amphibolites have major element abundances similar to those of basaltic komatiites, Mg-tholeiites and Fe-rich tholeiites. The former have gently sloping REE patterns, whereas the Mg-tholeiites have non-uniform REE patterns ranging from flat (～ 10 times chondrite) to strongly light REE-enriched. The Fe-rich amphibolites have flat REE patterns at 20–30 times chondrite.The Dwalile metamorphic suite, which is preserved in the keels of synforms within the BMS, includes peridotitic komatiites that have depleted light REE patterns similar to those of compositionally similar volcanics in the Onverwacht Group, Barberton, basaltic komatiites and tholeiites. The basaltic komatiites have REE patterns parallel to those of the BMS basaltic komatiites but with lower total REE contents. The Dwalile tholeiites have flat REE patterns.The basic and ultrabasic liquids were derived by partial melting of a mantle source which may have been heterogeneous or the heterogeneity may have resulted from sequential melting of the mantle source. The Fe-rich amphibolites were derived either from liquids generated at shallow levels or from liquids generated at depth which subsequently underwent extensive fractionation. 相似文献
13.
S.A. Drury 《Precambrian Research》1978,7(3):237-257
Seventeen rocks from the Lewisian Gneiss of the Inner Hebrides of Scotland, which represent three distinct lithological types at granulite to greenschist facies of metamorphism show rare-earth element patterns which seem not to have been disturbed by their complex metamorphic history. Some indication of their origin can be obtained by simple geochemical models.Three tonalitic pyroxene gneisses are characterized by: (1) light REE enrichment and heavy REE depletion; (2) low total REE contents; (3) moderate Eu enrichment. Their REE chemistry can be approximated by a model involving 10% partial melting of various garnet-bearing basaltic source materials. Alternatively, they may be some form of crystal cumulate, preserving their original anhydrous mineralogy, representing 30% crystallization of a parent tonalitic magma.Three tonalitic to granodioritic hornblende-biotite gneisses are characterized by: (1) light REE enrichment and heavy REE depletion; (2) significantly higher total REE contents than the pyroxene gneisses; (3) moderate Eu depletion. Their REE patterns can be approximated by a residual silicic melt in a model involving 30% fractional crystallization of solids with the modal mineralogy of the pyroxene gneisses or 40% removal of pure anorthosite from a parent dacitic magma.Two strongly metasomatised diopside-actinolite gneisses and one highly sheared epidote-chlorite gneiss have REE patterns which are not significantly different from the hornblende-biotite gneisses which were their precursors before metasomatism and late greenschist-facies shearing. This suggests that strong alteration has not enciphered the REE systematics of the gneisses.Basic gneisses of quartz tholeiite composition occurring as early dykes, which shared the same metamorphic history as the tonalitic to granodioritic gneisses, are characterised by: (1) slight enrichment in light REE relative to heavy REE; (2) variable total REE contents; (3) little difference between granulite and amphibolite facies types. Their REE patterns can be matched by models involving 5–15% partial melting of ultrabasic mantle with 3 times chondritic REE abundances, leaving a residue of olivine and orthopyroxene. 相似文献
14.
垭口片麻岩的主要岩石化学特征 总被引：2，自引：0，他引：2
出露于川西滇中地区的垭口片麻岩及相应岩石是一套英云闪长质-奥长花岗质(为主)-花岗闪长质片麻岩(灰色片麻岩即TTG岩套)和花岗质片麻岩组合,后者可能是前者活化时遭受钾长石化的结果。其常量元素、过渡金属元素和稀土元素特征与早前寒武纪低铝型灰色片麻岩一致,是本区晚太古代结晶基底(花岗地体)。 相似文献
15.
16.
The Chakradharpur Granite—Gneiss complex (CKPG) is exposed as an elliptical body within the arcuate metamorphic belt sandwiched between the Singhbhum Granite in the south and the Chotonagpur Granite—Gneiss to the north. It consists of an older bimodal suite of grey gneiss and amphibolites, intruded by a younger unit of pegmatitic granite. The bimodal suite represents the basement to the enveloping metasediments.The average major-element chemistry of the grey gneiss conforms to the definition of trondhjemite and includes both low-Al2O3 and high-Al2O3 types. The amphibolites can be grouped into a low-MgO and a high-MgO type. Rocks of the younger unit range in composition from granodiorite to quartz monzonite. The two granitic units also differ significantly in their Rb, Sr and Ba contents, and in the REE distribution pattern. The grey gneiss shows a highly fractionated REE pattern and a distinct positive Eu anomaly, with Eu/Eu* values increasing with increase in SiO2 %. In samples of the younger granite, the REE pattern is less fractionated, with higher HREE abundance relative to the grey gneiss and usually shows a negative Eu anomaly. The two types of REE patterns in amphibolites are interpreted to represent the two broad groups identified on the basis of major element chemistry.On the basis of chemical data, a two-stage partial melting model for the genesis of grey gneiss is suggested, involving separation of hornblende and varying amounts of plagioclase in the residual phase. Varying amounts of plagioclase in the residuum result in the wide range of Al2O3 content of the partial melt from which the trondhjemites crystallised. Residual hornblende produces the highly fractionated REE pattern, but a relatively higher HREE content of the trondhjemites compared to those produced by separation of garnet in the residual phase. The high level of Ba together with moderate levels of Sr in the trondhjemites can also be explained by plagioclase in the residue, whose effectiveness in partitioning Ba compared to Sr is lower. Of the two groups of amphibolites, the low-MgO type shows relative depletion of LREE compared to the high-MgO type. It contains varying amounts of plagioclase and is tentatively suggested to represent the residue. The other group, with a slightly fractionated REE pattern (CeN/ YbN = 2.01), is generally considered to represent the source material for the trondhjemites. This may have been generated by 5–15% partial melting of mantle peridotites, containing higher concentrations of LIL elements than those which produced average Precambrian tholeiites. This first phase of partial melting resulted in the slightly fractionated REE pattern of these amphibolites. Derivation of the younger granitic unit from the trondhjemites can be ruled out on the basis of REE data alone. REE data suggest partial melting of metasediments to be the origin of these rocks. It is also possible that deeply buried volcanic rocks, similar to calc-alkaline components of greenstone belts, are the parent for this component. 相似文献
17.
Robert Cullers Sambhudas Chaudhuri Neil Kilbane Richard Koch 《Geochimica et cosmochimica acta》1979,43(8):1285-1301
The REE (rare-earth) contents of sixty-three <2 μ fractions of Pennsylvanian and Permian platform sediment from the mid-continent of the U.S.A. vary considerably (ΣREE = 46–439 ppm;La/ Lu = 5.2–15.7; correlation coefficient of REE with La/Lu = 0.89), but the Eu/Sm ratios are nearly constant even in reducing environments that concentrate U (0.16–0.22). There is no correlation of REE content to clay mineralogy.Lower Permian <2 μ fractions from continental to nearshore marine sediment in Oklahoma have higher REE content (244–261 ppm) than marine facies in Kansas (46–140ppm), but <2μ Upper Permian fractions in an evaporite basin have constant but high REE content (288–281 ppm; one = 153—ppm). All Pennsylvanian <2 μ fractions from Oklahoma have high REE content (209–439 ppm), and fractions from Kansas cyclothems have variable REE content (86–438 ppm). REE content in the <2 μ fractions is inherited from the provenance, but is modified by ion exchange during weathering, transportation, or deposition. Exchangable REE tend to be concentrated in clay minerals in basic environments, but removed in acid environments.Sand and gravel-size fractions consist mostly of quartz or chert so their REE content is low (7.9–40.6 ppm) although heavy minerals may contribute a large fraction of the REE content. Unexpectedly, silt-size fractions have REE contents (74–355 ppm) that are usually lower but similar to their <2 μ fractions, and the REE contents do not correlate to clay mineral/quartz ratios. The interpretation of REE content in sedimentary rocks needs to be done cautiously due to the above factors. 相似文献
18.
Kiyoto Futa 《Geochimica et cosmochimica acta》1981,45(7):1245-1249
The Sm-Nd isotopic system of a tonalitic augen gneiss and its constituent minerals from northern Michigan was disturbed during metamorphism. Sm-Nd zircon ages are lower than the wholerock Sm-Nd model age. However, closely associated pairs of minerals (for example, sphene and biotite or apatite and plagioclase) retain their apparent metamorphic ages. The Sm-Nd model age for the tonalitic augen gneiss of 3919 ± 30myr, appears to reflect open system behavior during metamorphism. A mineralogically different gneiss from the same location has a Sm-Nd model age of 3520 ± 70 myr. The two whole rocks differ in their Sm-Nd and Rb-Sr systematics and in their chondrite-normalized rare earth element (REE) patterns. The whole-rock-normalized mineral REE patterns show the contribution of the major and trace minerals to the REE content of the whole rock. The trace minerals contain a significant amount of the total REE. 相似文献
19.
The Askot crystallines form a doubly plunging synformal belt and occurs as a detached crystalline belt or klippen in the vast
sedimentary terrain lying between Central crystallines towards north and the Almora crystallines to the south. It is dominated
by granite gneiss and augen gneiss, and also comprise of metapelites, migmatites and basic intrusives. In this paper, the
geochemical studies of the granite gneiss and augen gneiss from the Askot crystallines, Kumaun Himalaya were carried out in
order to understand their origin and evolution.
The granite gneiss is generally foliated, with less foliated and porphyritic variety seen in the core part. The K-feldspar
shows Carlsbad twinning, while plagioclases show complex twinning. They show euhedral zircon and apatite along with titanite
as accessory minerals. The granite gneiss is moderately evolved (Mg# ∼50) and has granodiorite composition with metaluminous,
calc-alkaline trends. They show higher concentration of Ti, Ca, Mg and low abundance of ∑REE (∼165 ppm) in comparison to augen
gneiss. They show volcanic arc signatures and compare well with Lateorogenic granites of Proterozoic times distributed world
wide. These calc-alkaline granites appear derived from a Paleoproterozoic mafic/intermediate lower-crust reservoir probably
involving arc magma underplating. Granite gneiss is also peraluminous with molar A/CNK>1.1, and the heterogeneity of granite
gneiss can be explained with the precursor melts, experiencing assimilation during up-rise through crust or contamination
of source itself involving sediments from the subduction zone. 相似文献