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1.
金刚石中的矿物包裹体 总被引：1，自引：0，他引：1
山东、辽宁金伯利岩区金刚石中的矿物包裹体是单晶相及多晶相的。大部分原生矿物包裹体为橄榄石,也有铬尖晶石、镁铝榴石、单斜辉石、斜方辉石、自然铁、针镍矿、柯石英、方解石及石墨。云母为后生包裹体矿物。橄榄石包裹体矿物富含Fo及Cr_2O_3。镁铝榴石矿物包裹体为紫红色,含Cr_2O_3,MgO及镁铬榴石分子高,形成压力为7.5GPa。单斜辉石包裹体矿物为绿色,形成温度和压力分别为:1531℃和4.5GPa。铬尖晶石包裹体矿物含Cr_2O_3及Cr/(Cr+Al)比值高,而含Al_2O_3低。柯石英的SiO_2含量为99.15％。自然铁含有少量的Co,Ni。针镍矿在金刚石中较常见。在橄榄石矿物包裹体内,见有方解石产出,其为同生矿物包裹体。 相似文献
2.
橄榄石流体包裹体中分子水的发现 总被引：11，自引：4，他引：7
利用激光拉曼和红外光谱测定了内蒙古东部喀喇沁地区玻基橄辉岩橄榄石斑晶中的原生流体包裹体的成分,发现了波长分别为３２４５～３５６５ｃｍ＾－１的液态水和波长为３６２７的ｃｍ＾－１气态水的特征峰,而未发现结构水的特征峰,橄榄石的惰性气体同位素测定结果表明包裹休事的水来源于地幔岩浆,而非混染陆壳水。这一发现,揭示了地幔水可以以流体包裹体的形成赋存在火山岩的矿物斑晶中。 相似文献
3.
桂北元宝山宝坛地区约825Ma镁铁-超镁铁岩的地球化学及其地质意义 总被引：13，自引：0，他引：13
镁铁－超镁铁岩的岩石学和地球化学特征表明，元宝山超镁铁岩中橄榄石的Fo为78－83，岩石具有明显的包橄结构，具有LREE亏损，低Th/Nb和La/Nb比值以及高（t)值（约＋5），是来源于亏损地幔低程度部分熔融的岩浆堆晶的产物；宝坛地区镁铁－超镁铁岩富集LREE，具有高的Th/Nb,La/Nb比值和低的（t)值（－0．45－7．01），是镁铁质岩浆上升，结晶过程中与地壳物质混染（AFC）的结果，超镁铁岩与澳大利亚Garidner岩脉群具有相似的不相容元素分布型式和Nd(t) 值，是导致新元古代Rodinia超大陆裂解的地幔柱熔融的产物。 相似文献
4.
橄榄石水溶性与含铁量相关性的实验研究 总被引：3，自引：2，他引：3
本文首次报导了含铁量不同的橄榄石单晶在不同温压条件下水溶性的试验研究结果。橄榄石单晶试件在300MPa静水压和1000℃至1300℃的温度条件下进行热压，每隔50℃进行一组试验，氧逸度被控制在Ni/NiO水平上。对热压后试件的抛光无包裹体区域做了显微红外光谱分析，红外光束平行于试件的[010]方向，最小直径为15－25μm。分析结果表明，在实验温压范围内，橄榄石中的水含量随铁含量的增加而增加。对于同样铁含量的橄榄石，则随湿度的增加，橄榄石的水含量也增加。最后，本文就实验结果对地幔动力学过程的启示进行了简单的讨论。 相似文献
5.
浙江新昌地幔岩捕虏体中的硫化物包裹体初步研究 总被引：8，自引：1，他引：7
浙江新昌一带晚第三纪碱性玄武岩中地幔岩（二辉橄榄岩）捕虏体内存在大量硫化物熔体包裹体。电子探针分析表明,硫化物相成分主要为镍黄铁矿,次为磁共铁矿。硫化物包裹体的Ｎｉ／Ｆｅ值与寄主地幔岩的橄榄石含量呈正相关。同一包裹体的硫化物相成分不均一,自中心至边缘硫化物的Ｎｉ／Ｆｅ、（Ｆｅ＋Ｎｉ）／Ｓ值和Ｎｉ呈均呈增加趋势。通过与中国汉诺坝、德国ＷｅｓｔＥｉｆｅｌ东欧Ｎｏｇｒａｄ－Ｇｏｍｏｒ地区资料的综合分析, 相似文献
6.
刘蒙华 《华东地质学院学报》1988,(1)
本文对富钾火山岩及其地幔包体和橄榄石捕虏晶中的包裹体进行了详细观察研究,并分别测量了熔融包裹体的均一温度(富钾火山岩1150—1200℃,地幔包体1200—1280℃,捕虏晶1200℃),在此基础上探讨了包裹体所反映的成因意义。通过包裹体的研究,进一步验证了如下结论:地幔包体与橄榄石捕虏晶有相同成因;地幔是含水的,地幔岩发生过部分熔融。 相似文献
7.
地幔岩中流体包裹体研究 总被引：5，自引：2，他引：3
地幔岩石中的流体包裹体代表地幔流体的样品。地幔流体包裹体可以存在从地幔来的金刚石,地幔捕虏体和岩浆碳酸岩中。研究这些岩石和矿物中的流体包裹体可以得出其所代表的地幔流体的温度、压力、成分和同位素。我们目前见到的这三类地幔岩石的包裹体主要可在橄榄石、辉石、金刚石、方解石和磷灰石中见到。这些包裹体可以粗略地分为CO2包襄体和硅酸盐熔融体包裹体。又可细分为四类包裹体：（1）富碳酸盐的硅酸盐熔融包裹体。这种包裹体在金刚石、地幔岩捕虏体和岩浆碳酸盐岩中见到,它又可分为结晶质熔融包裹体和玻璃包裹体。（2）CO2包裹体。这种包裹体大多见于地幔捕虏体中,在金刚石和岩浆碳酸岩中也可见到。（3）含硫化物的包裹体。这种包裹体见于地幔捕虏体中,与纯CO2包裹体和含CO2的熔融包裹体共存。（4）高密度的流体包裹体。这种包裹体见于金刚石中,是一种高盐度、高密度的含K、Cl和H2O的流体包裹体,又可分为高卤水包裹体和含卤水的富硅的碳酸盐岩浆包裹体。从对金刚石、地幔捕虏体和岩浆碳酸盐岩中流体包裹体的研究表明,地幔流体存在不均匀性和不混溶性。 相似文献
8.
从金刚石成因研究,流体包裹体、表征流体存在的固态包裹体及晶格原子、流体成分组合的制约因素等方面,论述了深部地幔流体的存在。华北地台原生金刚石中与流体包裹体共存的钛铁矿+铬铁矿、金红石+金云母+橄榄石、锆石+碳酸盐+橄榄石、磷灰石+金云母+橄榄石组合。相平衡原理揭示地幔流体存在着复杂的自催化反应。华北地台由金刚石流体包裹体所反映的深部地幔组成C、H、O、S和N分别为16.87%、47.47%、30.90%、3.02%和5.38%(皆为原子百分比),与现代大气圈、水圈相比明显富H贫O。 相似文献
9.
东天山香山镁铁-超镁铁岩中富CH4流体包裹体的特征及其意义 总被引：1，自引：0，他引：1
香山岩体是东天山镁铁-超镁铁杂岩带的一个典型岩体，相带发育。各相带都含有韭闪石质普通角闪石巨晶，后环绕橄榄石和拉长石生长，构成包橄结构和包含结构，表明母岩浆富水。本研究的样品采自于香山岩体中岩体。拉长石和橄榄石中的流体包裹体孤立分布，或成群分布，大小不等，无明显方向性，或成串分布，平行于寄主矿物的颗粒边界和生长晶面。流体包裹体主要为原生，一部分为次生或假次生，是在以角闪石结晶为标志的岩浆流体大量出溶期间捕获的，因而代表了岩浆源区的流体。运用显微激光拉曼光谱仪，在100～4000cm。全波段范围内对拉长石和橄榄石中的50多个流体包裹体的气泡进行了分析。结果表明，流体包裹体的气体成分分为4类：a)富CH4气体；b)富H2O气体；c)H2O CH4混合气体；d)多组分(C2H6 N2 CH4，C2H6 CH4 N2 C4H6)混合气体。因而，香山岩体所携带的流体是一种富CH4等还原性挥发份和富H2O的流体。由于上地幔处于相对氧化状态，上地幔的挥发份以CO2为主。因而，香山岩体的母岩浆和流体应该来自于地幔过渡带或软流圈，这同时也表明新疆北部晚古生代的地幔过渡带或软流圈可能是未被氧化的、含C—H系列流体的圈层。俯冲板片的再循环，为地幔深处的H2O提供了来源。富CH4还原性C—H流体和富H2O流体，为地幔深处的熔融发挥了重要作用，进而产生了新疆北部造山后广泛分布的镁铁一超镁铁岩浆以及铜镍硫化物矿床。 相似文献
10.
我国东部沿海地区新生代碱性玄武岩中,广泛分布尖晶石二辉橄榄岩等地幔岩包体,地幔岩的退火时间和退火温度是岩石圈演化的重要标志。研究表明,地幔橄榄岩是宿主岩石中的异源包体,为先已存在的固态的地幔物质。镜下观察表明,地幔橄榄岩的主要造岩矿物中常含有圆形矿物包裹体,如橄揽石中含有尖晶石和斜方辉石,斜方辉石中含有橄榄石和尖晶石包裹体等。矿物包裹体从原始的多边形转变为球粒状的形态变化是地幔岩在某种退火温 相似文献
11.
内蒙古贺根山蛇绿岩型铬铁矿中固体包裹体矿物化学成分研究 总被引：4，自引：0，他引：4
内蒙古贺根山蛇绿岩型(豆荚型)铬铁矿矿床分布于内蒙古-大兴安岭海西褶皱带的蛇绿岩套内的贺根山岩块中。该蛇绿岩块主要由地幔橄榄岩、堆积岩和基性熔岩组成。铬铁矿矿体主要赋存于地幔橄榄岩相内的纯橄岩脉内,或被薄层的纯橄岩(数厘米到数米)外壳包围,矿体成群和成带分布。 在铬铁矿矿石中发现多种固体包裹体矿物,如橄榄石、斜方辉石、单斜辉石、角闪石、韭闪石、硬玉、钠长石、钛钠金云母等。这种特殊的固体包裹体矿物组合反映了铬铁矿矿床的成因或形成环境。 相似文献
12.
坡一含铜镍基性-超基性岩体是新疆北山西段早二叠世幔源岩浆活动产物之一。本文主要对该岩体中铬铁矿及内部固体包裹物进行了电子探针分析。坡一岩体铬铁矿主要成分呈线性变化并具低Zn、Ti和Fe3+的特征。铬铁矿内部固体包裹物由橄榄石、辉石等无水单矿物相包裹物,角闪石、金云母等含水多矿物相包裹物以及硫化物三类组成,硅酸盐包裹物化学成分上表现出富镁高铬的特点,其中云母具有富碱高镁的特征。估算得到铬铁矿结晶温度在1340~1411℃之间,结晶压力在2.56~3.33 GPa之间,坡一岩体原始岩浆Al2O3含量约为14.13%,Ti O2含量约为1.57%。结合已有研究成果,认为坡一岩体原始岩浆早期属于低钛苦橄质岩浆,可能是软流圈地幔环境下经历了15.5%~18.9%程度的部分熔融产物。原始岩浆早期存在含水富挥发份流(熔)体相且达到了硫饱和,铬铁矿结晶可能是导致硫饱和的重要原因。 相似文献
13.
Exsolutions of Diopside and Magnetite in Olivine from Mantle Dunite, Luobusa Ophiolite, Tibet, China 总被引：1，自引：0，他引：1
The exsolutious of diopside and magnetite occur as intergrowth and orient within olivine from the mantle dunite, Luobusa ophiolite, Tibet. The dunite is very fresh with a mineral assemblage of olivine （〉95%） ＋ chromite （1%-4%） ＋ diopside （〈1%）. Two types of olivine are found in thin sections： one （Fo = 94） is coarse-grained, elongated with development of kink bands, wavy extinction and irregular margins; and the other （Fo = 96） is fine-grained and poly-angied. Some of the olivine grains contain minor Ca, Cr and Ni. Besides the exsolutions in olivine, three micron-size inclusions are also discovered. Analyzed through energy dispersive system （EDS） with unitary analytical method, the average compositions of the inclusions are： Na20, 3.12%-3.84%; MgO, 19.51%-23.79%; Al2O3, 9.33%-11.31%; SiO2, 44.89%-46.29%; CaO, 11.46%-12.90%; Cr2O3, 0.74%-2.29%; FeO, 4.26%- 5.27%, which is quite similar to those of amphibole. Diopside is anhedral f＇dling between olivines, or as micro-inclusions oriented in olivines. Chromite appears euhedral distributed between olivines, sometimes with apparent compositional zone. From core to rim of the chromite, Fe content increases and Cr decreases; and A! and Mg drop greatly on the rim. There is always incomplete magnetite zone around the chromite. Compared with the nodular chromite in the same section, the euhedral chromite has higher Fe3O4 and lower MgCr2O4 and MgAI2O4 end member contents, which means it formed under higher oxygen fugacity environment. With a geothermometer estimation, the equilibrium crystalline temperature is 820℃-960℃ for olivine and nodular chromite, 630℃-770℃ for olivine and euhedral chromite, and 350℃-550℃ for olivine and exsoluted magnetite, showing that the exsolutions occurred late at low temperature. Thus we propose that previously depleted mantle harzburgite reacted with the melt containing Na, Al and Ca, and produced an olivine solid solution added with Na^＋, Al^3＋, Ca^2＋, Fe^3＋, Cr^3＋. With temperature d 相似文献
14.
Hugh Rollinson 《Geology Today》2016,32(2):58-64
Recent studies of chromite deposits from the mantle section of ophiolites have revealed a most unusual collection of minerals present as inclusions within the chromite. The initial discoveries were of diamonds from the Luobosa ophiolite in Tibet. Further work has shown that mantle chromitites from ophiolites in Tibet, the Russian Urals and Oman contain a range of crustal minerals including zircon, and a suite of highly reducing minerals including carbides, nitrides and metal alloys. Some of the minerals found represent very high pressure phases indicating that their likely minimum depth is close to the top of the mantle transition zone. These new results suggest that crustal materials may be subducted to mantle transition zone depths and subsequently exhumed during the initiation of new subduction zones—the most likely environment for the formation of their host ophiolites. The presence of highly reducing phases indicates that at mantle transition zone depths the Earth's mantle is ‘super’‐reducing. 相似文献
15.
Silicate and oxide mineral inclusions in diamonds from the geologically and historically important De Beers Pool kimberlites in Kimberley, South Africa, are characterised by harzburgitic compositions (>90%), with lesser abundances from eclogitic and websteritic parageneses. The De Beers Pool diamonds contain unusually high numbers of inclusion intergrowths, with garnet+orthopyroxene±chromite±olivine and chromite+olivine assemblages dominant. More unusual intergrowths include garnet+olivine+magnesite and an eclogitic assemblage comprising garnet+clinopyroxene+rutile. The mineral chemistry of the De Beers Pool inclusions overlaps that of most worldwide localities. Peridotitic garnet inclusions exhibit variable CaO (<5.8 wt.%) and Cr2O3 contents (3.0–15.0 wt.%), although the majority are harzburgitic with very low calcium concentrations (<2 wt.% CaO). Eclogitic garnet inclusions are characterised by a wide range in CaO (3.3–21.1 wt.%) with low Cr2O3 (<1 wt.%). Websteritic garnets exhibit intermediate compositions. Most chromite inclusions contain 63–67 wt.% Cr2O3 and <0.5 wt.% TiO2. Olivine and orthopyroxene inclusions are magnesium-rich with Mg-numbers of 93–97. Olivine inclusions in chromite exhibit the highest Mg-numbers and also contain elevated Cr2O3 contents up to 1.0 wt.%. Peridotitic clinopyroxene inclusions are Cr-diopsides with up to 0.8 wt.% K2O. Eclogitic and websteritic clinopyroxene inclusions exhibit overlapping compositions with a wide range in Mg-numbers (66–86).
Calculated temperatures for non-touching inclusion pairs from individual diamonds range from 1082 to 1320 °C (average=1197 °C), whereas pressures vary from 4.6 to 7.7 GPa (average=6.3 GPa). Touching inclusion assemblages are characterised by equilibration temperatures of 995 to 1182 °C (average=1079 °C) and pressures of 4.2–6.8 GPa (average=5.4 GPa). Provided that the non-touching inclusions represent equilibrium assemblages, it is suggested that these inclusions record the conditions at the time of diamond crystallisation (1200 °C; 3.0 Ga). The lower average temperatures for touching inclusions are attributed to re-equilibration in a cooling mantle (1050 °C) prior to kimberlite eruption at 85 Ma. Pressure estimates for touching garnet–orthopyroxene inclusions are also skewed towards lower values than most non-touching inclusions. This apparent difference may be an artefact of the Al-exchange geobarometer and/or the result of sampling bias, due to limited numbers of non-touching garnet–orthopyroxene inclusions. Alternatively pressure differences could be caused by differential uplift in the mantle or possibly variations in thermal compressibility between diamond and silicate inclusions. However, thermodynamic modelling suggests that thermal compressibility differences would cause only minor changes in internal inclusion pressures (<0.2 GPa/100 °C). 相似文献
16.
Origin of phlogopite-orthopyroxene inclusions in chromites from the Merensky Reef of the Bushveld Complex,South Africa 总被引：1，自引：1，他引：0
About 30% of the chromite grains of variable sizes in a chromitite seam at the base of the Merensky Reef of the Bushveld Complex
on the farm Vlakfontein contain abundant composite mineral inclusions. The inclusions are polygonal to circular with radial
cracks that protrude into the enclosing chromite. They vary from a few microns to several millimeters in diameter and are
concentrated in the cores and mantles of chromite crystals. Electron backscattered patterns indicate that the host chromites
are single crystals and not amalgamations of multiple grains. Na-phlogopite and orthopyroxene are most abundant in the inclusions.
Edenitic hornblende, K-phlogopite, oligoclase and quartz are less abundant. Cl-rich apatite, rutile, zircon and chalcopyrite
are present at trace levels. Na-phlogopite is unique to the inclusions; it has not been found elsewhere in the Bushveld Complex.
Other minerals in the inclusions are also present in the matrix of the chromitite seam, but their compositions are different.
The Mg/(Mg+Fe2+) ratios of orthopyroxene in the inclusions are slightly higher than those of orthopyroxene in the matrix. K-phlogopite in
the inclusions contains more Na than in the matrix. The average compositions of the inclusions are characterized by high MgO
(26 wt%), Na2O (2.4 wt%) and H2O (2.6 wt%), and low CaO (1.1 wt%) and FeO (4.4 wt%). The δ18O value of the trapped melt, estimated by analysis of inclusion-rich and inclusion-poor chromites, is ∼7‰. This value is consistent
with the previous estimates for the Bushveld magma and with the δ18O values of silicate minerals throughout the reef. The textural features and peculiar chemical compositions are consistent
with entrapment of orthopyroxene with variable amounts of volatile-rich melts during chromite crystallization. The volatile-rich
melts are thought to have resulted from variable degrees of mixing between the magma on the floor of the chamber and Na-K-rich
fluids expelled from the underlying crystal pile. The addition of fluid to the magma is thought to have caused dissolution
of orthpyroxene, leaving the system saturated only in chromite. Both oxygen and hydrogen isotopic values are consistent with
the involvement of a magmatic fluid in the process of fluid addition and orthopyroxene dissolution. Most of the Cr and Al
in the inclusions was contributed through wall dissolution of the host chromite. Dissolution of minor rutile trapped along
with orthopyroxene provided most of the Ti in the inclusions. The Na- and K-rich hydrous silicate minerals in the inclusions
were formed during cooling by reaction between pyroxene and the trapped volatile-rich melts. 相似文献
17.
The investigated chromitite dike is located at the top of an upwelling mantle structure of the Oman ophiolite (Maqsad diapir), in undeformed dunites displaying evidence for magma impregnation and circulation, just below the paleo-ridge axis. The chromitite dike is undeformed, its shape is that of an upward widening tube. It exhibits an internal layering which is roughly perpendicular to the cavity axis and comprises a vertical succession of four main layers showing a graded-bedding. Chromitite magmatic structures are beautifully preserved and result from a progressive crystallization from small euhedral crystals to wide octahedron-shaped nodules; dissolution textures provide evidence for late magmatic desequilibrium; sedimentation structures include flattening of the largest nodules. The silicate matrix comprises poikilitic forsterite and a locally abundant association of primary pargasite and plagioclase and alteration minerals (vesuvianite-chlorite-dolomite); pargasite inclusions are very abundant in the chromite. Chromite composition changes from one layer to the other and from core to rim in the chromite nodules (chromium decreases and titanium increases); Ti contents are generally high (0.4 to 0.8 wt.% TiO2) with respect to podiform chromites. Platinum-group elements are not abundant but they show a strong fractionation at the scale of the orebody and of the main graded-bedded layers (Pd/Ir ratio varies from 0.5 to 11.5). REE patterns of chromitite parallel to those of gabbros and furthermore display a sea water related hydrothermal alteration (Ce negative anomaly).
The chromitite dike of Maqsad provides evidence for the crystallization of chromitite bodies in subvertical magma conduits below oceanic ridges; it corroborates the model of Cassard et al. (1981) and Lago et al. (1982) concerning the formation of chromitite pods in ophiolites which were later deformed and transposed into the horizontal plane due to the plastic flow prevailing away from the paleo-axial zone. Layering and chromite compositional variations are ascribed to a multicellular convective system segregating various stocks of chromite particles either in the upwelling flow of fresh magma or in the convective cells of fractionated residual magma in the confined part of the cavity. The estimated life-time for the magma influx is very short (<2 months). The parent-magma was probably of MORB-type and already fractionated (Ti-rich and PGE-poor), which is consistent with the strong evidence of magma-peridotite interactions in the core of the Maqsad diapir. Hydrous fluids were present during chromite crystallization (pargasite inclusions) suggesting that fluid-rich melts occur in the upper mantle. 相似文献
18.
Gehad M. Saleh 《中国地球化学学报》2006,25(4):307-317
1 Introduction The association of massive Fe-Ni-Cu sulfides andchromite is a very unusual feature of podiformchromitites occurring in mantle tectonites of ophioliticcomplexes. It has only been described in theSoutheastern Desert, Egypt, where sulfides a… 相似文献
19.
U-type paragenesis inclusions predominate (94.7%) among the crystalline inclusion suite of 115 diamonds (−4+2 mm) obtained from the recently discovered Snap Lake/King Lake (SKL) kimberlite dyke system, Southern Slave, Canada. The most common inclusions are olivine (90) and enstatite (22). Sulfide, Cr-pyrope, chromite and Cr-diopside inclusion are less abundant (15, 10, 5 and 1, respectively). Results of the inclusion composition study demonstrate the following. (a) The relatively enriched character of the mantle parent rocks of the U-type diamonds. The average Mg# of olivine inclusions is 92.1, and of enstatite inclusions average 93.3. CaO content in Cr-pyrope inclusions is relatively high (3.73–5.75 wt.%). (b) Four of ten U-type Cr-rich pyrope inclusions contain a majoritic component up to 16.8 mol.% which requires pressures of 110 kbar. Carbon isotopes compositions for 34 diamonds with U-type inclusions have a δ13C range from −3.2‰ to −9‰ with a strong peak around −3.5‰. This is much heavier than the ratios of U-type diamonds from Siberia and South Africa (4.5‰). Diamonds with olivine inclusions can be divided into two groups based on their δ13C values as well as the Mg# and Ni/Fe ratio in the olivines. Most show a narrow range of δ13C values from −3.2‰ to −4.8‰ (average −3.72‰) and have olivine inclusions with Mg# less than 92.3 and relatively high Fe/Ni ratios. A second group is characterized by a much wider variation of C isotope composition (δ13C varies from −3.8‰ to −9.0‰, average −5.97‰), and the olivine inclusions having a higher Mg# (up to 93.6) and relatively low Fe/Ni ratios. This difference in the C isotope composition may have several explanations: (a) peculiarities of asthenosphere degassing coupled with an abnormal thickness of lithosphere; (b) the abnormal thickness and enriched character of lithospheric mantle; (c) involvement of subducted C of crustal origin in the processes of the diamond formation. The presence of subcalcic Cr-rich majorite (up to 17 mol.%) pyropes of low-Ca harzburgite paragenesis among the crystalline inclusion suite of SKL diamonds is strong evidence for the existence of diamondiferous depleted peridotite in lithospheric mantle at depth near 300 km beneath Southern Slave area and is postulated to be one of the main reasons for the much heavier C isotope composition of SKL U-type diamonds in comparison with those from Siberian and South African kimberlites. 相似文献
20.
扬子地块北缘周庵超镁铁质岩体矿物学特征及其对铜镍矿化的启示 总被引：2，自引：0，他引：2
扬子地块北缘~635 Ma周庵超镁铁质岩体是一个新发现的含铜镍硫化物矿化的隐伏岩体,主要由二辉橄榄岩组成。文章通过研究周庵岩体中橄榄石、铬铁矿和辉石的矿物成分变化探讨了岩浆演化过程和含矿岩体成因。根据岩石的矿物组合和蚀变程度,岩体从上到下分为3个部分:上部绿泥石-蛇纹石化二辉橄榄岩相带、中部二辉橄榄岩相带和下部绿泥石-角闪石化二辉橄榄岩相带。根据岩体中部带橄榄石和铬铁矿的成分,计算得到母岩浆的Mg#值为0.63,MgO/FeO摩尔比值为1.72,w(Al2O3)为10.2%~11.7%,w(Ni)为476×10-6,说明其为高镁玄武质岩浆;岩体中部带原生铬铁矿和粒间相铬铁矿核部的Cr2O3和Al2O3呈正相关关系,说明铬铁矿与粒间硅酸盐熔体发生了平衡交换,铬铁矿的高w(TiO2) 和Cr#值与拉张环境中层状岩体的铬铁矿特征一致;根据辉石温压计得到岩体中部单斜辉石和斜方辉石的共结温度为1 017~1 077℃,压力为(3.6~4.5)×108 Pa,暗示形成岩体的浅部岩浆房深度约为12 km。岩体上部和中部带的橄榄石Fo值大部分集中在80 mol%~85 mol%,w(Ni)介于2 255×10-6~4 455×10-6,说明这些橄榄石是从没有经过强烈分离结晶和硫化物熔离的岩浆中结晶出来的。岩体下部带橄榄石的Fo值(67 mol%~68 mol%)和w(Ni) (1 500×10-6~2 000×10-6)都低于岩体上部和中部带的橄榄石相应值,说明岩体下部带的橄榄石可能形成于演化程度较高、并经历了硫化物熔离的岩浆。因此,笔者认为周庵岩体是由相对原始的和演化了的高镁玄武质岩浆两期侵位形成的。 相似文献