首页 | 本学科首页   官方微博 | 高级检索  
相似文献
 共查询到18条相似文献,搜索用时 109 毫秒
1.
本文报道MaДЖГaBaH(印度中部)火山岩管含金刚石岩石的综合研究结果,首次分析了这个岩管岩石中的金云母、蛇纹石、硫化物的成分。按成分MaДЖГaBaH岩管的岩石实际上完全缺乏碳酸盐物质,TiO2和P2O5含量较高,含有高钛金云母和指示矿物(镁名榴石、铬铁矿、钛铁矿)含量低而不同于典型的金伯利岩。同时这种岩石与含钾镁煌斑岩也有显著差别:含K2O很低(0.46-1.79%),没有发现单斜辉石、钾碱镁闪石。这种岩石似乎是金伯利岩和钾美煌斑岩之间的过渡类型。  相似文献   

2.
中印度的马奇格万含金刚石的岩筒是古老的前寒武纪含金刚石岩筒之一。据现在已有资料分析,它的开采时期早于南非的金刚石的开采(1870年)。它是印度目前唯一开采的矿床。经对马奇格万岩筒综合调查后,其成分主要是金云母、蛇纹石、硫化物。不同于典型金伯利岩的成分,主要是缺少碳酸盐矿物;含高的 Ti_2O 和 P_2O_5,高钛的金云母及低含量的指示矿物(镁铝榴石、铬铁矿、钛铁矿)。但它不同于钾镁煌斑岩的成分,表现在其含 K_2O(0.46—1.79重量%)少。没有发现单斜辉石,钾质锰闪石。认为它是介于金伯利岩及钾镁煌斑岩之间的岩石类型。本文介绍一种划分钾镁煌斑岩分类的方案—四面体扩展法。  相似文献   

3.
王留海 《矿物岩石》1991,11(4):51-56
本文分析了大洪山区钾镁煌班岩中的矿物特征,利用造岩矿物和副矿物的电子探针分析结果与西溴含金刚石钾镁煌斑岩中相应矿物进行对比。并用特征副矿物镁铝榴石、铬铁矿的化学成分作Cr_2O_3—CaO图,Cr_2O_3-MgO图,利用Cr/(Cr+Al)的比值参数,判别岩体的含矿性。认为该区钾镁煌斑岩目前虽然尚未发现金刚石,但成矿有利因素较多。  相似文献   

4.
钾镁煌斑岩是一类较为特殊的火山成因或浅成的超基性岩,是一种重要的深源岩石,是深源岩浆活动的标志性产物,可作为了解地幔信息的窗口,也作为继金伯利岩之后的另一种金刚石寄主岩被持续关注.全球最优质的金刚石产于钾镁煌斑岩中,主要分布于西澳阿盖尔等地.中国钾镁煌斑岩主要分布于黔湘一带、山西饮牛沟、山东大井头、湖北大洪山和西昆仑克里阳地区,综合分析认为,钾镁煌斑岩主要分布于深大断裂附近,中国钾镁煌斑岩受江南台隆西缘的都匀—贵阳—铜仁—怀化深断裂、常德—安仁深断裂以及郯庐断裂带等深大断裂带控制;贵州镇远马坪、湖南宁乡云影窝、山东平邑大井头等钾镁煌斑岩有原生金刚石产出,钾镁煌斑岩的金刚石成矿潜力仍然有待深入研究,尤以湘黔钾镁煌斑岩带、郯庐断裂带大井头等地可望突破.钾镁煌斑岩的标志性矿物有富钛贫铝金云母、钾碱镁闪石、镁橄榄石、镁铝榴石、铬尖晶石、铬铁矿等.其中S1、S2组贫铝富镁铬铁矿对钾镁煌斑岩中金刚石的形成有指示意义.中国钾镁煌斑岩活动具多期性,其中晚侏罗世—早白垩世(147—100 Ma)时期属于中国含金刚石钾镁煌斑岩和相关的金-稀土等金属矿产的重要成矿时期.  相似文献   

5.
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   

6.
贵州东部镇远地区钾镁煌斑岩的矿物学和岩石学研究   总被引:4,自引:0,他引:4  
江万 《现代地质》1995,9(3):351-358
通过对贵州东部镇远地区的一套偏碱性的基性超基性煌斑岩的矿物学及岩石学研究,发现该套岩石具有多种钾镁煌斑岩的特征矿物和结构:含钛的钾碱镁闪石、钛金云母、低铝透辉石、含铁透长石,以及金云母的嵌晶状结构、橄榄石的"犬牙"结构。在岩石地球化学方面,它们与世界典型地区的钾镁煌斑岩相似。根据对比鉴定,将这套岩石定名为:(1)金云母钾镁煌斑岩;(2)含橄榄石嵌晶状钾镁煌斑岩。  相似文献   

7.
贺安生  孙一虹 《岩石学报》1992,8(2):194-200
我们首次在湖南发现了钾镁煌斑岩。这套岩石由于遭受强烈风化和蚀变,与典型的西澳钾镁煌斑岩相比,其K_2O和MgO含量明显偏低,Al_2O_3含量偏高。REE含量、金云母成分及以金云母作为主要载体的元素(如Rb、Ba、Ti、Sc、Zn、Ga和Nb等)都与西澳的钾镁煌斑岩基本一致,此外高度富集LREE和U,Th、Nb、Ta、Zr等不相容元素,并有高的δ~(18)O‰值,表明形成这套岩石的上地幔源区受到了软流圈的交代作用。  相似文献   

8.
新疆瓦吉尔塔格“金伯利岩”是一种特殊类型的岩石,与国外已知典型的金伯利岩有所不同。岩石的角砾成分以异源角砾为主,有岩屑,亦有晶屑,岩球构造不发育,岩石中橄榄石卵斑不多见,两个世代斑晶区分不明显,矿物组台除以橄榄石、金云母为主外,尚有相当数量单斜辉石和普通角闪石,但可能是捕晶成因;副矿物镁铝榴石,尤其是含铬高的镁铝榴石缺乏;岩石化学成分投点在金伯利岩区间,但 MgO,K_2O 均偏低,部分样品 K_2O相似文献   

9.
黔东南钾镁煌斑岩岩石学特征   总被引:1,自引:0,他引:1  
陈慧 《地质与勘探》2018,54(4):702-710
黔东南地区位于扬子地台东南缘与江南褶皱系西缘的过渡带。本文以黔东南马坪、麻江地区发现的钾镁煌斑岩体为主要研究对象,通过地质特征、岩石学、矿物学、地球化学等研究,认为马坪地区金云钾镁煌斑岩具基性-超基性岩的标型元素Cr、Ni、Co含量较高,不相容元素总体富集,稀土元素配分模式为右倾型且分异程度较高,与典型钾镁煌斑岩(西澳含金刚石矿钾镁煌斑岩)在岩浆来源、地球化学特征上具有较大的相似性;麻江地区钾镁煌斑岩Al_2O_3、K_2O含量低,轻稀土富集、重稀土亏损,轻稀土特高,其岩浆形成温度、地球化学成分上与典型钾镁煌斑岩有较大差异。  相似文献   

10.
中国金伯利岩中的单斜辉石   总被引:3,自引:0,他引:3  
董振信 《地质学报》1992,66(1):35-47
本文对我国金伯利岩中,作为巨晶、粗晶、基质相矿物、与镁铝榴石和钛铁矿的连生体、深源岩石包体矿物及金刚石中包体矿物产出的单斜辉石的粒度、形态、颜色及蚀变壳、矿物种属、化学成分特征、端员组分、红外光谱等进行了研究。并与玄武岩中的巨晶及其深源岩石包体矿物、钾镁煌斑岩和云煌岩中的单斜辉石作了对比。研究了单斜辉石和镁铝榴石共生对。探讨了金伯利岩中单斜辉石的成因,形成的温、压条件及所反映出的金伯利岩体形成的构造环境,指出了该矿物在找寻金刚石矿工作中的指示标志。  相似文献   

11.
塔里木地台南缘发现钾镁煌斑岩   总被引:10,自引:1,他引:9  
赵磊  杨万志 《现代地质》1998,12(4):555-558
首次在塔里木地台南缘皮山县境内找到钾镁煌斑岩,它们呈脉状产出,围岩为白云母石英片岩。该钾镁煌斑岩的岩石化学成分与亚洲钾镁煌斑岩的平均岩石化学成分接近,与澳大利亚西金伯利地区钾镁煌斑岩一致,稀土元素及其配分模式位于世界钾镁煌斑岩的范围之内,其中大多数标本具有已知世界钾镁煌斑岩的共同微量元素特征:具Ba、K、La和Ce的正异常及Ta、Nb、Sr和Ti的负异常。该钾镁煌斑岩的发现对研究区金刚石找矿和深部地质过程研究均具深远意义。  相似文献   

12.
青藏高原拉萨地块新生代超钾质岩与南北向地堑成因关系   总被引:3,自引:0,他引:3  
青藏高原拉萨地块广泛分布有新生代超钾质岩,岩石地球化学和Sr-Nd-Pb同位素特征表明这些超钾质岩来源于与古俯冲环境有着密切联系的含金云母的富集地幔源区,它们主要喷发于25~10 Ma。同时在拉萨地块分布有多条南北向地堑(裂谷),且它们的切割深度可能到达下地壳的深部甚至岩石圈地幔,它们主要形成于23~8 Ma。拉萨地块大多数超钾质岩沿着新生代的南北向地堑(裂谷)分布,并且它们在形成时代和空间分布上存在着明显的耦合性,结合沿着印度-雅鲁藏布江缝合带分布的中新世埃达克质岩,笔者认为这些超钾质岩很可能与中新世早期北向俯冲的印度岩石圈沿着印度-雅鲁藏布江缝合带附近发生断离,以及由此而引起拉萨地块东西向伸展构造活动产生的南北向地堑(裂谷)系统有关。  相似文献   

13.
分布于甘肃省榆中县兴隆山地区的兴隆山岩群为一套浅变质火山岩与浅变质碎屑岩所组成的岩石组合,其火山岩主要出露于兴隆山岩群中岩组和上岩组。兴隆山岩群火山岩岩性主要为变质玄武岩,具有低w(K2O)、w(Na2O+K20)和w(TiO2)的特点,且w(TiO2)和w(P2O5)接近于洋中脊玄武岩的平均质量分数,为亚碱性的拉斑玄武岩系列,火山岩稀土元素总量低,轻、重稀土元素分馏不明显,稀土元素配分曲线为轻稀土元素略亏损、重稀土元素平坦型,与洋中脊玄武岩的配分曲线类似,火山岩大离子亲石元素相对富集,高场强元素和重稀土元素平坦,稀土元素、微量元素特征及构造环境判别显示兴隆山岩群的火山岩形成于中元古代秦祁昆多岛洋中部略富集的E型洋中脊的海底扩张环境。  相似文献   

14.
Primitive olivine-mica-K-feldspar lamprophyre dykes, dated at 1831 ± 6 Ma, intrude lower greenschist facies rocks of the Early Proterozoic Pine Creek Inlier, of northern Australia. They are spatially, temporally and probably genetically associated with a post-tectonic composite granite-syenite pluton (Mt. Bundey pluton). The dykes have unusually high contents of large-ion-lithophile (LILE) and LREE elements (e.g. Ba up to 10,000 ppm, Ce up to 550 ppm, K2O up to 7.5 wt. %) that resemble the concentrations found in the West Kimberley olivine and leucite lamproites. However, mineralogically the Mt. Bundey lamprophyres resemble shoshonitic lamprophyres and lack any minerals diagnostic of lamproites; leucite or leucite-pseudomorphs are absent. Mineral compositions are also unlike those in lamproites: micas contain higher Al2O3 than lamproitic mica; amphiboles are secondary actinolites after diopside; and oxides consist of zincian-chromian magnetite and groundmass magnetite. Heavy mineral concentrates contain mantle-derived xenocrysts of magnesiochromite, pyrope, Cr-diopside and rutile indicating a depth of sampling > 70 km. The Mt. Bundey lamprophyres are non-peralkaline to borderline peralkaline (molar (K + Na)/Al = 0.8 − 1.0) and potassic rather than ultrapotassic (molar K/Na < 2.5). They have distinctive major element compositions (≈46−49 wt. % SiO2, ≈1.5−2 wt. % MgO, ≈7 wt. % CaO), and element ratios (e.g. molar Al/Ti ≈10, K/Na ≈2) that indicate they are best classified amongst transitional lamproites, i.e. potassic rocks such as cocites, jumillites and Navajominettes, that have geochemical characteristics transitional between Groups I and III. (Foley et al., 1987). The Mt. Bundey lamprophyres have LILE enrichment patterns that resemble the W. Kimberley pamproites but have moderate negative Ta---Nb---Ti anomalies and HREE abundances that are closely similar to the jumillites of southeastern Spain and Mediterranean-type lamproites. Single-stage modelling of Rb---Sr data is consistent with enrichment of the source-region of the Mt. Bundey lamprophyres ≈ 120–170 Ma before partial melting; i.e. at 1.95–2.10 Ga. Source enrichment does not appear to be associated with subduction processes, but may instead relate to incipient rifting of the Archaean basement. Negative Ta---Nb---Ti anomalies in the Mt. Bundey dykes may, therefore, relate to stability of residual titanate minerals in an oxidized subcontinental mantle source. This view is supported by high Fe3+/ΣFe ratios of mantle-derived magnesiochromite xenocrysts which indicate oxidized mantle conditions (ƒo2 ≈ FMQ + 1 long units), and by the presence of xenocrystic Cr-bearing rutile. Although the Mt. Bundey dykes have sampled upper mantle material, the oxidized nature of the magma source-region, and of the magma itself, suggests that conditions may not be favourable for diamond survival at depth nor for diamond transport in transitional lamproite magmas of this kind.  相似文献   

15.
徐宿地区新元古代辉绿岩床的地球化学特征   总被引:13,自引:1,他引:12  
同位素测年数据显示,徐宿地区的辉绿岩床是震旦纪早期和震旦纪晚期两次侵入的 产物。岩床多呈板状或楔状,为超浅成—浅成侵入体,其化学成分以高SiO2、CaO和低Al 2O3、MgO及(K2O+Na2O)为特征,属大陆拉斑玄武岩系列。稀土元素配分模式为轻 稀土富集型,但稀土元素分馏并不强烈。Rb、K、La等不相容元素富集,而Nb、Sr亏损明显 。δ18O值在6.63‰~9.93‰之间,多数>8‰。研究表明,该区基性岩浆来源于过 渡型地幔,主要通过部分熔融方式形成,在岩浆上侵过程中遭到陆壳或花岗质岩石的混染。  相似文献   

16.
The mineralogical, petrological and geochemical studies on Keliyang (克里阳) potassic dykes have been carried out to understand their rock types, the petrogenesis and the nature of their mantle sources. They are potassic lamprophyre, not lamproites as the previous researchers believed. In this study, the whole-rock major and trace element compositions of another 6 lamproite dykes recently discovered are reported. Major elements were determined by X-ray fluorescence spectrometry (XRF) techniques, while REE and trace elements were determined by inductively coupled plasma mass spectrometry (ICP-MS). They can be classified into phlogopite-diopside lamprophyre, leucite-diopside lamprophyre and granular carbonatite-bearing diopside lamprophyre on the basis of their mineral components. They are all characterized by relatively low SiO2 (41.31% -44. 84%), TiO2 (0.75% -0.86%) and high MgO (7.30%-11.33%), K2O (4.01%-6.01%) concentrations with K2O/Na2O ratios of 2. 77-12.49. In addition, they display enrichment in large-ion iithophile elements (LILEs, e. g., Rb, Sr,Ba) and LREE, but a relative depletion in high-field-strength elements (HFSEs, e.g. , Nb, Ta, Zr, Hf and Ti). They display similar chondrite-normalized REE patterns with slight negative Eu anomalies (δEu=0.64-0. 82), and high initial 87Sr/86Sr ratios, which resemble those of high K/Ti and low-Ti potassic magmas formed in subduction-related settings. Consequently, we suggest that the parental magma was generated by partial melting of the phlogopite-amphibole- bearing garnet lherzolite within the lithospheric mantle that might have been metasomatized by a potassium-bearing fluid released from a subduction oceanic crust.  相似文献   

17.
Chemical, mineralogical and isotopic studies have been made on nodules of the MARID (Mica-Amphibole-Rutile-Ilmenite-Diopside) xenolith suite in southern African kimberlites. All are ultramafic and ultrapotassic (MgO= 20–25%, K2O=4–9%), with bulk compositions reflecting the wide variation in relative proportions of the five minerals amongst the nodules. They are comparable in major element compositions to magnesian lamproites, in particular the ultrabasic olivine-lamproites of Western Australia. In a number of high pressure experimental studies on ultra-potassic rocks, the phases produced between 25–30 kbar from compositions comparable to those of MARID rocks (in the presence of additional water), were predominantly phlogopite and diopside (±K-richterite, ±ilmenite, ±rutile). Furthermore the compositions of experimental minerals produced in the synthetic-biotite-mafurite-H2O system by Edgar et al. (1976) are similar to those in MARID rocks.It is suggested on the basis of these observations and the textural appearance of MARID rocks that they are magmatic compositional equivalents of MgO-rich lamproites that crystallized at high pressures. While lamproites have higher average concentrations of incompatible elements, (including REE), some MARID rocks have comparable abundances. It is suggested that late stage vapour-rich melts carrying substantial REE and other incompatible elements escaped from crystallizing MARID magmas into surrounding subcontinental lithosphere, thus resulting in lower levels of these elements in most MARID rocks. In contrast faster crystallization of lamproitic rocks under volcanic/ hypabyssal conditions would prevent similar losses.The MARID proto-magmas are thought to be either partial melts of metasomatised phlogopite peridotite, or small volume asthenospheric melts which are modified and further enriched by incorporation of small partial melts of enriched subcontinental lithosphere during magma ascent.  相似文献   

18.
熊耳山地区太古宙超镁铁质岩在空间分布上具有不均一性、成带性和多方向性特征 ,岩石以橄榄岩、辉石岩、角闪石岩为主 ,蚀变强烈。岩石贫钙、镁 ,低铝、K2 O Na2 O,稀土总量较高 ,轻重稀土分馏显著。地球化学特征表明大部分超镁铁质岩体为岩浆侵入成因  相似文献   

设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号