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1.
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：7，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
2.
山东的无棣大山和栖霞方山是两个以霞石岩为主的新生代火山,含有大量的地幔橄榄岩捕掳体,橄榄岩捕掳体中的尖晶石常见黑色反应边。在BSE图像上,这些反应边根据结构的不同又可以进一步分为两种:筛状边和均一边。有时两种反应边在同一颗尖晶石中共存并相互过渡。尖晶石捕掳晶和捕掳体中与寄主岩直接接触的尖晶石常发育均一边;发育筛状边的尖晶石则一般不直接与寄主岩接触,但位于捕掳体的边缘。尖晶石的筛状边呈多孔状,为富Cr尖晶石或铬铁矿。筛状边成分上与核部(Cr_2O_3=7.52%~36.75%,Cr#=7.80~44.20,Mg#=44.70~74.48)区别明显,具有高的Cr_2O_3含量(23.42%~65.96%)、Cr#值(78.97~92.49)以及低的Mg#值(17.22~43.02)。另外,筛状边相对其核部(TiO 2=0.00%~0.53%,MnO=0.04%~0.35%)还显示偏高的TiO 2(0.20%~3.60%)和MnO(0.29%~1.93%)。在筛状边附近存在富Al_2O_3(8.00%~17.57%)和MgO(17.89%~26.02%)的玻璃。尖晶石的均一边无孔洞但多发育裂理,成分上与核部突变,并以富TiO 2(20.90%~6.64%)和FeO T(70.79%~53.92%)为特征,最外部为钛磁铁矿。均一边具有明显的成分分带,表现为由内至外TiO 2、FeO T含量逐渐增高,Al_2O_3(0.04%~16.34%)、Cr_2O_3(0.77%~25.69%)和MgO(0.50%~7.16%)含量逐渐降低。尖晶石的两种反应边与寄主岩密切的空间关系说明其成因与寄主岩浆有关。虽然尖晶石筛状边的Cr#值(79.0~92.5)明显高于核部(7.8~44.2),但是其相对核部偏高的TiO 2和MnO含量,以及显著降低的Mg#值均与单纯的部分熔融趋势不吻合。根据尖晶石两种反应边的结构特征、成分特征和相互的空间关系,我们认为筛状边与均一边是岩浆与尖晶石反应不同阶段的产物。当橄榄岩捕掳体被岩浆捕获后,由于成分上的不均衡两者之间将发生溶解反应。反应过程中,尖晶石中不同元素向熔体迁移的速率区别明显,其中Cr是最难熔的元素也是迁移最慢的元素。在反应的初始阶段,由于易溶组份Al、Mg等元素随熔体迁出,尖晶石发育筛状边,并同时伴随Cr#值的显著升高和Mg#值的显著降低。此时,寄主岩浆中的Ti、Mn等元素也部分扩散进入筛状边中的残留尖晶石。如果熔体足够多,反应得以持续进行,筛状边中的Cr最终也将被熔体带走。在反应产生的混合熔体中金属氧化物最早达到饱和并结晶。随着反应的持续进行,结晶出的矿物将继续生长、变粗,并相互连接,直至孔洞消失形成均一边。同时伴随着矿物的不断结晶,溶解界面上的熔体成分也不断变化,从而使均一边具有明显的成分分带。在橄榄岩捕掳体内部,由于渗进捕掳体中的岩浆有限,渗透岩浆与尖晶石之间的反应多限于早期阶段,反应产物为筛状边。在捕掳体边缘,与寄主岩浆直接接触的尖晶石由于参与反应的岩浆量足够多,因此一般产生反应的终端产物———均一边。 相似文献
3.
湖南尖峰岭矿床是一个典型的花岗岩型Li、Nb和Ta稀有金属矿床,为研究花岗岩成矿作用以及指导湘南地区稀有金属找矿工作,采用XRF、ICP-MS和ISE法分析了与成矿有关的黑云母花岗岩、钠长石花岗岩及云英岩的中主量、微量元素和挥发分。结果表明:钠长石花岗岩和云英岩中的SiO_2(70.6%~84.85%)和挥发分F(2.43%~3.74%)质量分数高,富Al_2O_3(9.36%~22.99%),且A/CNK1.0,为过铝质岩石,全碱(w(Na_2O+K_2O)=1.51%~7.52%)和w(CaO)(0.1%~3.44%)变化大,w(Fe_2O_3)、w(MgO)、w(TiO_2)、w(MnO)、w(P_2O_5)较低;稀土元素组成具显著的Eu负异常和"M"型四分组效应,强烈富集Rb、Th、U、Nb、Ta元素,亏损Ba、Sr、Ti元素。花岗岩地球化学特征显示在演化过程中经历了高程度分异演化作用和岩浆不混溶作用,其挥发分F对稀有元素有明显的富集作用,并制约着熔体/流体体系的地球化学行为及其成矿效应。钠长石花岗岩和云英岩的稀有金属富集成矿受到岩浆不混溶作用、水岩反应、风化淋滤作用的共同控制。 相似文献
4.
基性—超基性岩熔体结构对铜(镍)、金成矿作用的制约 总被引：1，自引：0，他引：1
岩浆熔体结构与Cu、Au成矿作用有着密切联系,熔体结构特征可作为Cu、Au成矿的指示标志。本文基于72个不同类型基性—超基性杂岩样品的系统分析,探讨岩浆熔体结构与Cu-Au成矿作用之间的关系,认为基性—超基性杂岩熔体的NBO/T,NBO,M~(2+),FeO和MgO值愈高以及T,M~(3+),Fe_2O_3和CaO值愈低,则愈有利于Cu(Ni)矿化,反之则有利于Au矿化。基性—超基性熔体中的Cu离子主要占据八面体位置,而NBO/T,NBO和M~(2+)值愈高则八面体位置愈多,故有利于Cu的滞留富集,以致最终成矿。元素Au在基性—超基性熔体中主要以Au~+的形式存在,而Au~+主要与Fe~(3+)结合形成四面体结 相似文献
5.
亚拉寨镍矿属岩浆熔离型与晚期岩浆结晶分异型复合的硫化物矿床。矿体赋存于基性～超基性杂岩体底部,有用元素镍平均0.44ω%,伴生铜、钴等。对矿石组份及其赋存状态研究后,提出综合利用建议。 相似文献
6.
笔者在冲绳海槽海底玄武岩基质中发现的中酸性玻璃质熔体 ,与以往在基性火山岩中发现的玻璃质熔体存在明显的差异 :( 1)在存在状态上 ,前者呈充填状态存在于细小的基质矿物之间 ,其体积明显受到岩浆冷却速率的制约 ;后者常出现富铁相和富硅相两种熔体共存现象 ,且一种熔体常呈球状分布于另一种熔体中。 ( 2 )在成分演化上 ,前者随着冷却速率的降低 ,成分向酸性方向演化 ;后者的成分与冷却速率间的关系不明显 ,一直表现为富铁相和富硅相两端员成分 ,缺失中间过渡成分。这两种类型的熔体 ,分别反映了幔源岩浆不同的演化过程 :冲绳海槽海底玄武岩中的中酸性玻璃质熔体 ,反映了幔源岩浆结晶分异演化过程 ,并记录了演化过程中各阶段产物的特征 ;而以往在基性火山岩中发现的富铁相和富硅相两种熔体的共存现象 ,反映了幔源岩浆的熔离过程 ,并记录了熔离产物的特征。 相似文献
7.
该实验用江西相山英安流纹岩加一定量的氟化物作为初始材料。在温度达875～900℃、压力0.5×10~8～1.0×10~8Pa时,含F和H_2O的英安流纹质岩浆的淬火产物中,有两种玻璃生成。其中一种玻璃呈小球出现,其成分相对富FeO、MgO、TiO_2。另一种玻璃,分布于小球之间,相对富SiO_2和Al_2O_3。实验表明,富含挥发分的酸性火山岩浆是比较容易熔离的。在流纹质火山岩中常见的长英质条带大多数不是浆屑,而是流纹质岩浆熔离的产物。 相似文献
8.
西藏南冈底斯广泛分布着一条巨型岩浆岩带,本文报道的墨竹工卡县北部花岗闪长岩LA-ICP-MS锆石U-Pb年龄为(48.84 Ma±0.32 Ma),其形成于始新世。岩体中w(SiO_2)(68.72%~70.69%),w(Al_2O_3)(14.90%~15.68%)和w(Fe_2O_3~T)(2.74%~3.44%)相对富集,贫w(MnO)(0.08%~0.11%),w(TiO_2)(0.31%~0.39%)和w(P_2O_5)(0.11%~0.15%),为一套高钾钙性系列弱过铝质系列(A/CNK为1.05~1.07),具有I型花岗岩的特征。岩石总体表现出轻稀土富集而重稀土亏损的右倾曲线,轻重稀土之比为:ΣLREE/ΣHREE=12.58~14.44。Eu轻微负异常(0.79~0.86)。岩体的大离子亲石元素、高场强元素含量均出现分化,表现出富集不相容元素(Rb,Ba,Pb,Th,U,K和Pb),而明显亏损高场强元素(如Nb,Ta,P,Ti)的特征,其中P的亏损可能指示磷灰石强烈分离结晶。整体显示出岛弧性质花岗岩的特征,暗示源区可能存在含钛矿物相或角闪石残留相。在始新世早期,随着印度-欧亚大陆碰撞的开始,俯冲下插的大洋板片由于重力拖拽作用会与大陆板块脱离,造成软流圈上涌,由此诱发地幔楔熔融产生镁铁质岩浆,并底侵至初生地壳底部,进而导致初生地壳部分熔融形成壳源岩浆。 相似文献
9.
《矿物岩石》2016,(3)
班公湖地区富镍硫化物超基性岩位于藏北班公湖-怒江缝合带西段,呈透镜状产出于侏罗系地层中,岩石已完全蚀变为蛇纹岩,恢复其原岩为方辉橄榄岩。地球化学研究表明:相对于原始地幔,该类超基性岩富w(MgO)(40.96%~42.82%),贫w(Al_2O_3)(0.19%~1.76%)、w(CaO)(0.11%~0.38%)和TiO_2(0.02%~0.06%);稀土元素总量低(0.238×10-6~2.044×10-6),远低于原始地幔值,稀土元素配分型式呈U型;强烈亏损高场强元素Y;岩石的锆石年龄为太古代(2 479 Ma±31 Ma)。以上特征表明其为残余地幔橄榄岩成因。富镍硫化物超基性岩中的镍硫化物呈似球状分布于蛇纹石中,主要为镍黄铁矿,偶见与镍黄铁矿共生的赫硫镍矿。电子探针分析结果表明,镍黄铁矿中w(Ni)为36.77%~42.62%,w(Fe)为18.83%~28.84%,w(S)为31.34%~38.3%。赫硫镍矿中w(Fe)为0.91%~13.36%,w(Ni)为60.5%~70.08%,w(S)为25.25%~27.23%。赫硫铁矿Fe含量高(除两件样品外均2%mol),且与镍黄铁矿的接触边界平直。结合前人的实验资料,认为Fe-Ni硫化物形成于高温阶段(300℃),为贫S的地幔Fe-Ni-S熔体捕虏体成因。 相似文献
10.
产于层状镁铁质-超镁铁质岩体中的太和岩浆型Fe-Ti氧化物矿床是峨眉山大火成岩省内带几个超大型Fe-Ti氧化物矿床之一。太和岩体长超过3km,宽2km,厚约1.2km。根据矿物含量和结构等特征,整个岩体从下向上可划分为下部岩相带、中部岩相带、上部岩相带。下部岩相带主要以(橄榄)辉长岩和厚层不含磷灰石的块状Fe-Ti氧化物矿层组成。中部岩相带韵律旋回发育,(磷灰石)磁铁辉石岩主要位于旋回的底部,旋回上部为(磷灰石)辉长岩。上部岩相带主要是贫Fe-Ti氧化物的磷灰石辉长岩。太和中部岩相带磷灰石磁铁辉石岩含有5%~12%磷灰石、20%~35%Fe-Ti氧化物、50%~60%硅酸盐矿物,且硅酸盐矿物与磷灰石呈堆积结构。磷灰石磁铁辉石岩中磁铁矿显示高TiO2、FeO、MnO、MgO,且变化范围与趋势接近于攀枝花岩体。钛铁矿FeO分别与TiO2、MgO显示负相关,而FeO分别与Fe2O3、MnO显示正的相关,且TiO2、FeO、MnO、MgO含量变化较大,这些特征都暗示磁铁矿和钛铁矿是从富Fe-Ti-P岩浆中分离结晶。因此,可以推断太和磷灰石磁铁矿辉石岩形成于矿物重力分选和堆积。太和下部岩相带包裹在橄榄石中磁铁矿含有相对较高Cr2O3(0.07%~0.21%),而中部岩相带包裹在橄榄石中磁铁矿Cr2O3(0.00%~0.03%)显著降低,且这些磁铁矿Cr2O3含量变化与单斜辉石Cr含量和斜长石An牌号呈正相关。这些特征印证了形成中部岩相带的相对演化的富Fe-Ti-P母岩浆可能是源自中部岩浆房的混合岩浆。上部岩相带磁铁矿和中部岩相带顶部少量磁铁矿显示较低Ti+V可能是由于岩浆房中累积的岩浆热液对磁铁矿成分进行了改造。 相似文献
11.
南苏鲁超高压变质带东海地区富钛榴辉岩及金红石矿的成因 总被引：3，自引：1，他引：3
苏鲁超高压变质带南部的东海地区有富Fe—Ti的钛铁矿榴辉岩和富Ti的金红石榴辉岩。富Fe—Ti榴辉岩的次要矿物主要由钛铁矿和钛磁铁矿组成，可舍少量金红石，具有很低的Si02（38．0％-42．3％）、Na20＋K20（0．48％～2．13％）和Zr、Nb、Ta、Ba、1Kb、REE含量，很高的FeO（18．24％-25．33％）、V和Co含量，并具有不同程度的LREE亏损、明显的正Eu异常；富Ti金红石榴辉岩舍有丰富的金红石和磷灰石，SiO2含量范围（38．0％-54．8％）较宽，FeO含量较低，P2O5含量较高（可达4．1％），而X-TiO2与P205含量具正相关性。相对于原始地慢岩．富Ti金红石榴辉岩具有Rb、Th、K、Nb、Pr、Nd、Eu、Ti、Lu的负异常和Ba、Sr、Zr的正异常．并具相对较高的IKEE含量，LREE富集和HREE亏损的1KEE分配型式。岩石学和地球化学特征揭示，Fe—Ti榴辉岩的原岩是变质的Fe—Ti辉长岩，是基性岩浆强烈分离结晶作用形成的超基性-基性-中酸性层状侵入体的特征组成部分。 相似文献
12.
位于攀西地区的新街层状岩体赋含大量钒钛磁铁矿,是峨眉山大火成岩省的一部分。岩体下部带和中部带以单斜辉石岩为主,并伴生浸染状钒钛磁铁矿矿化;上部带以辉长岩为主,赋存厚层的钒钛磁铁矿矿体。之前研究认为厚层的钒钛磁铁矿矿体的形成与粒间不混熔的富Fe熔体有关,但对富Fe熔体的演化过程缺乏细致研究。本文通过对新街岩体上部带的富矿辉长岩层和上覆浅色辉长岩中斜长石环带结构和成分的研究,揭示了富Fe熔体的演化过程。在浅色辉长岩中保存的岩浆不混熔的直接证据表现为矿物粒间共轭的富Si交生体和富钛铁矿交生体代表的非反应结构。本次研究发现,与粒间富Si交生体接触的斜长石边部的FeO和TiO_2含量随斜长石牌号(An)值的降低而降低,而与粒间富钛铁矿交生体接触的斜长石边部的FeO和TiO_2含量随An值的降低而升高,说明斜长石的边部成分变化记录了粒间共轭的富Si和富Fe熔体的成分特征。在富矿辉长岩中,斜长石可分为初生和新生两种,初生斜长石的An值介于57~62,FeO含量为0.34%~0.50%,TiO_2含量为0.06%~0.13%,新生斜长石具有相对较高的An值(61~81)和FeO、TiO_2含量,二者的内部和边部还发育增生斜长石,其An值(~50)相对较低;在初生斜长石边部可见不连续的新生斜长石环带和增生斜长石边,造成其内部成分显著不均一,并发育复杂的环带结构。本文认为,初生斜长石是岩浆正常分离结晶作用的产物。在粒间熔体发生不混熔后,不混熔的富Fe熔体逐渐向岩浆房下方迁移并结晶出了一些相对高An值的新生斜长石,或沿一些初生斜长石边部生长形成不连续的高An环带。当富Fe熔体演化至晚期,由于矿物生长空间受限,仅在初生和新生斜长石局部形成了相对低An值的增生边、或沿颗粒裂隙进入斜长石内部形成增生斜长石核。 相似文献
13.
攀枝花岩体钛铁矿成分特征及其成因意义 总被引：2，自引：1，他引：1
峨眉大火成岩省是全球最大的钒钛磁铁矿床聚集区,攀枝花岩体是其中的典型代表。根据岩性特点,攀枝花岩体主体可划分为上、中、下三个岩相带,其中中部岩相带和下部岩相带岩性旋回非常发育,每个旋回从下向上铁钛氧化物和暗色硅酸盐矿物逐渐减少,块状铁钛氧化物矿石或磁铁矿辉长岩都出现在每个旋回的底部和下部。然而,尽管钛铁矿固相线以下固溶体出溶远弱于磁铁矿,从而能更好地保留成因信息,但其成分变化的成因意义没有受到足够重视。本次研究发现作为主要金属氧化物之一的钛铁矿的成分不仅在不同岩性中有明显差异,同时,中、下部岩相带的各岩性旋回中钛铁矿成分也具有周期性变化。例如,块状矿石中钛铁矿具有最高的MgO和TiO2及最低的FeO、Fe2O3和MnO,而辉长岩中钛铁矿则具有相反的成分特征。同时,钛铁矿的MgO含量与磁铁矿的MgO含量及橄榄石的Fo牌号具有显著的正相关关系。这种规律性变化说明每个旋回可以代表一次比较明显的岩浆补充,每次新岩浆补充后,钛铁矿和磁铁矿及橄榄石都是结晶较早的矿物。与Skaergaard岩体相比,攀枝花岩体钛铁矿的MgO含量较高,表明攀枝花岩体分离结晶过程中铁钛氧化物结晶较早;与挪威Tellnes斜长岩套铁钛矿床中的钛铁矿相比,攀枝花岩体的钛铁矿不仅具有较高的MgO和FeO,还具有极高的TiO2和MnO,但Fe2O3却很低,说明地幔柱背景下形成的钛铁矿与斜长岩套中钛铁矿的成分有显著的区别。 相似文献
14.
M.L.Tolstykh V.B.Naumov A.D.Babansky 《岩石学报》2007,23(1):93-104
Melt inclusions in minerals from some volcanoes of the Kurile-Kamchatka region were examined.The studied basaltic andesites and andesites were sampled from volcanoes of the Central Kamchatka depression(Shiveluch and Bezymyannyi),Eastern Kamchatka volcanic belt(Avachinskii and Karymskii),and Iturup Island,Southern Kuriles(Kudryavyi).Basalts of the 1996 eruption of the Karymskii volcanic center and dacites of Dikii Greben'volcano,Southern Kamchatka were also studied.More than 260 melt inclusions from 31 rock samples were homogenized,and quenched glasses were analyzed using electron and ion microprobes.The compositions of melt inclusions in andesitic phenoerysts vary in silica contents from 56 to 80wt%.Al_2 O_3 ,FeO,MgO,CaO decrease and Na_2O and K_2O increase with increasing SiO_2.Many inclusions(about 80% )are dacitic or rhyolitic.However,the compositions of silicic glasses(>65wt% SiO_2)in andesites significantly differ in TiO2,FeO,MgO,CaO,and K_2O contents from those in dacites and rhyolites.High-potassium melts(K_2O 3.8～6.8wt% )with various SiO_2 from 51.4 to 77.2wt% were found in minerals of all volcanoes studied.This indicates a contribution of a component selectively enriched in potassium to magmas of the whole region.A great compositional diversity of melt inclusions in plagioelase phenocrysts from the Bezymyannyi andesites suggests a complex history of plagioclase crystallization and magma evolution in the andesite formation.Melts from different volcanoes strongly vary in volatile contents.The highest H_2O contents are found in the melts from Shiveluch(3.0～7.2wt%,4.7wt% on average)and Avachinskii (4.7～4.8wt%);while those are lower in melts of Kudryavyi(0.1～2.6wt% ),Dikii Greben'(0.4～1.8wt%),and Bezymyannyi (<1wt%).Chlorine contents are also variable.The lowest values are found in the Bezymyannyi melts(0.09wt% on average),the highest Cl contents are typical of melt inclusions in minerals from the Karymskii andesites(0.26wt% on average).The melts from Avachinskii,Dikii Greben',Kudryavyi,and Shiveluch show intermediate Cl contents(0.13～0.20wt% ).The pressure of 350～1600 bar determined by CO_2 fluid inclusions in plagioclase from the Shiveluch andesites suggests a magma chamber at a depth of 1.5～6 km. Concentrations of 17 elements were determined in glasses of melt inclusions in plagioclases from five volcanoes(Avachinskii, Bezymyannyi,Dikii Greben',Kudryavyi,and Shiveluch).The studied melts show similar trace-element patterns with Nb and Ti minima and B,K,Be,and Li maxima.The melts are close to typical island arc magmas by Sr/Y,La/Yb,K/Ti,and Ca/St ratios, and have some specific regional geochemical features.REE patterns sensitive to degree of magma differentiation indicate that Kudryavyi magmas are most primitive,while Shiveluch magmas are most evolved. 相似文献
15.
对华北克拉通北缘达里诺尔地区鸽子山附近玄武岩中的含金云母辉石岩捕虏体进行了岩石学、矿物学的研究,并对其中的单斜辉石、斜方辉石、金云母和粒间熔体进行了原位微区主、微量元素分析。结果显示,单斜辉石和斜方辉石具有低的Mg^#、Cr 2O 3和高的Al2O3含量,斜方辉石还具有高的MnO含量,这些特征表明辉石岩代表了交代熔体在地幔中冷却固结堆晶形成的岩脉。辉石岩中金云母、粒间熔体的出现及其不平衡的地球化学特征说明辉石岩形成以后又遭受到了多期次的硅酸盐熔体地幔交代作用。结晶出单斜辉石的母岩浆在蛛网图上具有K、Pb元素的弱负异常但不具有Nb、Ta、Ti元素的负异常,推测形成辉石岩的熔体可能来自软流圈地幔。粒间熔体的低SiO2,高MgO和FeO的特征指示其形成于地幔超基性岩的部分熔融,蛛网图上明显的K、Pb正异常以及Nb、Ta负异常说明其源区也存在俯冲沉积物的贡献。基于此,认为中国东部新生代岩石圈地幔经历了多期次地幔交代作用。 相似文献
16.
IrinaP.Solovova Theodoros Ntaflos Andrei Girnis Natalya N.Kononkova Vyacheslav V.Akinin 《岩石学报》2007,23(1):83-92
Melt and fluid inclusions were studied in the minerals of Cenozoic olivine melanephelinites from the Chukchi Peninsula, Russia.The rock contain several generations of olivine phenocrysts varying in composition at mg=0.88～0.77.The phenocrysts bear fluid and melt inclusions recording various stages of melt crystallization in volcanic conduits and shallow magma chambers.Primary fluid inclusions are CO_2-dominated with a density of up to O.93 g/cm~3.All fluid inclusions are partially leaked,which is indicated by haloes of tiny fluid bubbles around large fluid inclusions in minerals.Melt inclusions contain various daughter crystals,which were completely resorbed in thermometric experiments at about 1230℃.Assuming that this temperature corresponds to the entrapment conditions of the CO_2 fluid inclusions,the minimum pressure of the beginning of magma degassing is estimated as 800MPa.Variations in the compositions of homogenized silicate melt inclusions indicate that olivine was the earliest crystalline phase followed by clinopyroxene,nepheline and orthoclase.This sequence is in agreement with the mineralogy of the rocks.The melts are strongly enriched in incompatible trace elements and volatiles(in addition to CO_2,high C1,F,and S contents were detected).There are some differences between the compositions of melts trapped in minerals from different samples.Variations in SiO_2,FeO,and incompatible element contents are probably related to melt generations at various levels in a homogeneous mantle reservoir. 相似文献
17.
The Neoproterozoic Korab Kansi mafic-ultramafic intrusion is one of the largest (100 km2) intrusions in the Southern Eastern Desert of Egypt. The intrusion consists of Fe-Ti-bearing dunite layers, amphibole peridotites, pyroxenites, troctolites, olivine gabbros, gabbronorites, pyroxene gabbros and pyroxene-hornblende gabbros, and also hosts significant Fe-Ti deposits, mainly as titanomagnetite-ilmenite. These lithologies show rhythmic layers and intrusive contacts against the surrounding granites and ophiolitic-island arc assemblages. The wide ranges of olivine forsterite contents (Fo67.9-85.7), clinopyroxene Mg# (0.57–0.95), amphibole Mg# (0.47–0.88), and plagioclase compositions (An85.8-40.9) indicate the role of fractional crystallization in the evolution from ultramafic to mafic rock types. Clinopyroxene (Cpx) has high REE contents (2–30 times chondrite) with depleted LREE relative to HREE, like those crystallized from ferropicritic melts generated in an island-arc setting. Melts in equilibrium with Cpx also resemble ferropicrites crystallized from olivine-rich mantle melts. Cpx chemistry and its host rock compositions have affinities to tholeiitic and calc-alkaline magma types. Compositions of mafic-ultramafic rocks are depleted in HFSE (e.g. Nb, Ta, Zr, Th and U) relative to LILE (e.g. Li, Rb, Ba, Pb and Sr) due to the addition of subduction-related hydrous fluids (rich in LILE) to the mantle source, suggesting an island-arc setting. Fine-grained olivine gabbros may represent quenched melts approximating the primary magma compositions because they are typically similar in assemblage and chemistry as well as in whole-rock chemistry to ferropicrites. We suggest that the Korab Kansi intrusion crystallized at temperatures ranging from ~700 to 1100 °C from ferropicritic magma derived from melting of metasomatized mantle at <5 Kbar. These hydrous ferropicritic melts were generated in the deep mantle and evolved by fractional crystallization under high ƒO2 at relatively shallow depth. Fractionation formed calc-alkaline magmas during the maturation of an island arc system, reflecting the role of subduction-related fluids. The interaction of metasomatized lithosphere with upwelling asthenospheric melts produced the Fe and Ti-rich ferropicritic parental melts that are responsible for precipitating large quantities of Fe-Ti oxide layers in the Korab Kansi mafic-ultramafic intrusion. The other factors controlling these economic Fe-Ti deposits beside parental melts are high oxygen fugacity, water content and increasing degrees of mantle partial melting. The generation of Ti-rich melts and formation of Fe-Ti deposits in few layered intrusions in Egypt possibly reflect the Neoproterozoic mantle heterogeneity in the Nubian Shield. We suggest that Cryogenian-Tonian mafic intrusions in SE Egypt can be subdivided into Alaskan-type intrusions that are enriched in PGEs whereas Korab Kansi-type layered intrusions are enriched in Fe-Ti-V deposits. 相似文献
18.
The two-liquid field between alkali-carbonate liquids and phonolite or nephelinite magmas from the Oldoinyo Lengai volcano has been determined between 0.7 and 7.6 kb and 900°–1,250° C. The miscibility gap expands with increase in
and decrease in temperature. Concomitantly there is a rotation of tie-lines so that the carbonate liquids become richer in CaO. The element distribution between the melts indicates that a carbonate liquid equivalent in composition to Oldoinyo Lengai natrocarbonatite lava would have separated from a phonolitic rather than a nephelinitic magma. CO2-saturated nephelinites coexist with carbonate liquids much richer in CaO than the Lengai carbonatites, but even so these liquids have high alkali concentrations. If the sövites of hypabyssal and plutonic ijolite-carbonatite complexes originated by liquid immiscibility, then large quantities of alkalis have been lost, as is suggested by fenitization and related phenomena. The miscibility gap closes away from Na2O-rich compositions, so that the tendency to exsolve a carbonatite melt is greater in salic than in mafic silicate magmas. The two-liquid field does not approach kimberlitic compositions over the range of pressures studied, suggesting that the globular textures observed in many kimberlite sills and dykes may be the result of processes other than liquid immiscibility at crustal pressures. 相似文献
19.
This paper reviews the results of investigations of melt inclusions in minerals of carbonatites and spatially associated silicate rocks genetically related to various deep-seated undersaturated silicate magmas of alkaline ultrabasic, alkaline basic, lamproitic, and kimberlitic compositions. The analysis of this direct genetic information showed that all the deep magmas are inherently enriched in volatile components, the most abundant among which are carbon dioxide, alkalis, halides, sulfur, and phosphorus. The volatiles probably initially served as agents of mantle metasomatism and promoted melting in deep magma sources. The derived magmas became enriched in carbon dioxide, alkalis, and other volatile components owing to the crystallization and fractionation of early high-magnesium minerals and gradually acquired the characteristics of carbonated silicate liquids. When critical compositional parameters were reached, the accumulated volatiles catalyzed immiscibility, the magmas became heterogeneous, and two-phase carbonate-silicate liquid immiscibility occurred at temperatures of ≥1280–1250°C. The immiscibility was accompanied by the partitioning of elements: the major portion of fluid components partitioned together with Ca into the carbonate-salt fraction (parental carbonatite melt), and the silicate melt was correspondingly depleted in these components and became more silicic. After spatial separation, the silicate and carbonate-silicate melts evolved independently during slow cooling. Differentiation and fractionation were characteristic of silicate melts. The carbonatite melts became again heterogeneous within the temperature range from 1200 to 800–600°C and separated into immiscible carbonate-salt fractions of various compositions: alkali-sulfate, alkali-phosphate, alkali-fluoride, alkali-chloride, and Fe-Mg-Ca carbonate. In large scale systems, polyphase silicate-carbonate-salt liquid immiscibility is usually manifested during the slow cooling and prolonged evolution of deeply derived melts in the Earth’s crust. It may lead to the formation of various types of intrusive carbonatites: widespread calcite-dolomite and rare alkali-sulfate, alkali-phosphate, and alkali-halide rocks. The initial alkaline carbonatite melts can retain their compositions enriched in P, S, Cl, and F only at rapid eruption followed by instantaneous quenching. 相似文献