Phase Equilibria Constraints on the Chemical and Physical Evolution of the Campanian Ignimbrite   总被引：5，自引：1，他引：4  

Fowler  Sarah J.; Spera  Frank J.; Bohrson  Wendy A.; Belkin  Harvey E.; De Vivo  Benedetto 《Journal of Petrology》2007,48(3):459-493

The Campanian Ignimbrite is a > 200 km³ trachyte–phonolitepyroclastic deposit that erupted at 39·3 ± 0·1ka within the Campi Flegrei west of Naples, Italy. Here we testthe hypothesis that Campanian Ignimbrite magma was derived byisobaric crystal fractionation of a parental basaltic trachyandesiticmelt that reacted and came into local equilibrium with smallamounts (5–10 wt%) of crustal rock (skarns and foid-syenites)during crystallization. Comparison of observed crystal and magmacompositions with results of phase equilibria assimilation–fractionationsimulations (MELTS) is generally very good. Oxygen fugacitywas approximately buffered along QFM + 1 (where QFM is the quartz–fayalite–magnetitebuffer) during isobaric fractionation at 0·15 GPa ( 6km depth). The parental melt, reconstructed from melt inclusionand host clinopyroxene compositions, is found to be basaltictrachyandesite liquid (51·1 wt% SiO₂, 9·3 wt%MgO, 3 wt% H₂O). A significant feature of phase equilibria simulationsis the existence of a pseudo-invariant temperature, 883 °C,at which the fraction of melt remaining in the system decreasesabruptly from 0·5 to < 0·1. Crystallizationat the pseudo-invariant point leads to abrupt changes in thecomposition, properties (density, dissolved water content),and physical state (viscosity, volume fraction fluid) of meltand magma. A dramatic decrease in melt viscosity (from 1700Pa s to 200 Pa s), coupled with a change in the volume fractionof water in magma (from 0·1 to 0·8) and a dramaticdecrease in melt and magma density acted as a destabilizingeruption trigger. Thermal models suggest a timescale of 200kyr from the beginning of fractionation until eruption, leadingto an apparent rate of evolved magma generation of about 10^–3km³/year. In situ crystallization and crystal settling in density-stratifiedregions, as well as in convectively mixed, less evolved subjacentmagma, operate rapidly enough to match this apparent volumetricrate of evolved magma production. KEY WORDS: assimilation; Campanian Ignimbrite; fractional crystallization; magma dynamics; phase equilibria  相似文献   

Pressures of Crystallization of Icelandic Magmas   总被引：1，自引：0，他引：1  

Kelley  Daniel F.; Barton  Michael 《Journal of Petrology》2008,49(3):465-492

Iceland lies astride the Mid-Atlantic Ridge and was createdby seafloor spreading that began about 55 Ma. The crust is anomalouslythick (20–40 km), indicating higher melt productivityin the underlying mantle compared with normal ridge segmentsas a result of the presence of a mantle plume or upwelling centeredbeneath the northwestern edge of the Vatnajökull ice sheet.Seismic and volcanic activity is concentrated in 50 km wideneovolcanic or rift zones, which mark the subaerial Mid-AtlanticRidge, and in three flank zones. Geodetic and geophysical studiesprovide evidence for magma chambers located over a range ofdepths (1·5–21 km) in the crust, with shallow magmachambers beneath some volcanic centers (Katla, Grimsvötn,Eyjafjallajökull), and both shallow and deep chambers beneathothers (e.g. Krafla and Askja). We have compiled analyses ofbasalt glass with geochemical characteristics indicating crystallizationof ol–plag–cpx from 28 volcanic centers in the Western,Northern and Eastern rift zones as well as from the SouthernFlank Zone. Pressures of crystallization were calculated forthese glasses, and confirm that Icelandic magmas crystallizeover a wide range of pressures (0·001 to 1 GPa), equivalentto depths of 0–35 km. This range partly reflects crystallizationof melts en route to the surface, probably in dikes and conduits,after they leave intracrustal chambers. We find no evidencefor a shallow chamber beneath Katla, which probably indicatesthat the shallow chamber identified in other studies containssilica-rich magma rather than basalt. There is reasonably goodcorrelation between the depths of deep chambers (> 17 km)and geophysical estimates of Moho depth, indicating that magmaponds at the crust–mantle boundary. Shallow chambers (<7·1 km) are located in the upper crust, and probablyform at a level of neutral buoyancy. There are also discretechambers at intermediate depths (11 km beneath the rift zones),and there is strong evidence for cooling and crystallizing magmabodies or pockets throughout the middle and lower crust thatmight resemble a crystal mush. The results suggest that themiddle and lower crust is relatively hot and porous. It is suggestedthat crustal accretion occurs over a range of depths similarto those in recent models for accretionary processes at mid-oceanridges. The presence of multiple stacked chambers and hot, porouscrust suggests that magma evolution is complex and involvespolybaric crystallization, magma mixing, and assimilation. KEY WORDS: Iceland rift zones; cotectic crystallization; pressure; depth; magma chamber; volcanic glass  相似文献   

Global Correlations of Ocean Ridge Basalt Chemistry with Axial Depth: a New Perspective   总被引：4，自引：0，他引：4  

Niu  Yaoling; O'Hara  Michael J. 《Journal of Petrology》2008,49(4):633-664

The petrological parameters Na₈ and Fe₈, which are Na₂O andFeO contents in mid-ocean ridge basalt (MORB) melts correctedfor fractionation effects to MgO = 8 wt%, have been widely usedas indicators of the extent and pressure of mantle melting beneathocean ridges. We find that these parameters are unreliable.Fe₈ is used to compute the mantle solidus depth (P_o) and temperature(T_o), and it is the values and range of Fe₈ that have led tothe notion that mantle potential temperature variation of T_P= 250 K is required to explain the global ocean ridge systematics.This interpreted T_P = 250 K range applies to ocean ridges awayfrom ‘hotspots’. We find no convincing evidencethat calculated values for P_o, T_o, and T_P using Fe₈ have anysignificance. We correct for fractionation effect to Mg^# = 0·72,which reveals mostly signals of mantle processes because meltswith Mg^# = 0·72 are in equilibrium with mantle olivineof Fo_89·6 (vs evolved olivine of Fo_{88·1–79·6}in equilibrium with melts of Fe₈). To reveal first-order MORBchemical systematics as a function of ridge axial depth, weaverage out possible effects of spreading rate variation, local-scalemantle source heterogeneity, melting region geometry variation,and dynamic topography on regional and segment scales by usingactual sample depths, regardless of geographical location, withineach of 22 ridge depth intervals of 250 m on a global scale.These depth-interval averages give Fe₇₂ = 7·5–8·5,which would give T_P = 41 K (vs 250 K based on Fe₈) beneathglobal ocean ridges. The lack of Fe₇₂–Si₇₂ and Si₇₂–ridgedepth correlations provides no evidence that MORB melts preservepressure signatures as a function of ridge axial depth. We thusfind no convincing evidence for T_P > 50 K beneath globalocean ridges. The averages have also revealed significantcorrelations of MORB chemistry (e.g. Ti₇₂, Al₇₂, Fe₇₂,Mg₇₂, Ca₇₂, Na₇₂ and Ca₇₂/Al₇₂) with ridge axial depth. Thechemistry–depth correlation points to an intrinsic linkbetween the two. That is, the 5 km global ridge axial reliefand MORB chemistry both result from a common cause: subsolidusmantle compositional variation (vs T_P), which determines themineralogy, lithology and density variations that (1) isostaticallycompensate the 5 km ocean ridge relief and (2) determine thefirst-order MORB compositional variation on a global scale.A progressively more enriched (or less depleted) fertileperidotite source (i.e. high Al₂O₃ and Na₂O, and low CaO/Al₂O₃)beneath deep ridges ensures a greater amount of modal garnet(high Al₂O₃) and higher jadeite/diopside ratios in clinopyroxene(high Na₂O and Al₂O₃, and lower CaO), making a denser mantle,and thus deeper ridges. The dense fertile mantle beneath deepridges retards the rate and restricts the amplitude of the upwelling,reduces the rate and extent of decompression melting, givesway to conductive cooling to a deep level, forces melting tostop at such a deep level, leads to a short melting column,and thus produces less melt and probably a thin magmatic crustrelative to the less dense (more refractory) fertile mantlebeneath shallow ridges. Compositions of primitive MORB meltsresult from the combination of two different, but geneticallyrelated processes: (1) mantle source inheritance and (2) meltingprocess enhancement. The subsolidus mantle compositional variationneeded to explain MORB chemistry and ridge axial depth variationrequires a deep isostatic compensation depth, probably in thetransition zone. Therefore, although ocean ridges are of shalloworigin, their working is largely controlled by deep processesas well as the effect of plate spreading rate variation at shallowlevels. KEY WORDS: mid-ocean ridges; mantle melting; magma differentiation; petrogenesis; MORB chemistry variation; ridge depth variation; global correlations; mantle compositional variation; mantle source density variation; mantle potential temperature variation; isostatic compensation  相似文献   

赣东北前寒武纪港边杂岩体的岩浆混合（和）作用及其地质意义   总被引：8，自引：0，他引：8  

李昌年  廖群安 《岩石矿物学杂志》2006,25(5):357-376

赣东北地区沿江绍断裂北缘和江南造山带南侧有大量的前寒武纪火山侵入杂岩呈带状分布,主要由大面积的陆相火山岩和若干长英质镁铁质火成杂岩体组成,后者中出露面积最大的港边杂岩体在填图尺度上可划分为长英质岩、镁铁质岩和过渡性岩3大组成部分,长英质岩颗粒锆石U_Pb谐和不一致曲线上交点年龄为822±4Ma,代表杂岩体中岩浆混合作用发生的时间。港边岩体中长英质岩石的Nd模式年龄为1·49~1·68Ga,镁铁质岩中玄武质岩石为1·51~2·21Ga,辉长岩的Nd模式年龄与玄武质岩石基本相同,为1·54~2·13Ga,经计算的过渡性岩石的Nd模式年龄为1·58~1·90Ga,因此认为镁铁质岩石从源区分离的时间要远早于长英质岩石,而过渡性岩石含有前两个端员岩浆相互混合(和)的信息。长英质岩石的εNd(t=822Ma)值为-0·8~-4·4,87Sr/86Sr(822)比值为0·70368~0·70549;玄武质岩石的εNd(822)值为-2·6~+2·3,87Sr/86Sr(822)比值为0·70387~0·70527,这反映了镁铁质岩浆的源区接近总地球,长英质岩浆则来自具壳幔混合性质的EMⅠ型地幔的源区。可以推测,赣东北前寒武纪也曾发生过岩浆底侵作用。底侵作用对港边火成杂岩体岩浆的形成起着重要的作用。底侵于壳幔边界的玄武质岩浆使地壳熔融形成长英质岩浆并聚集于浅部岩浆房。随着长英质岩浆房降温,长英质岩浆的结晶度和粘度增加,其物理状态发生液态→(固+液)混合态→固态的变化;当玄武质岩浆穿透下地壳并不断进入物理状态变化的长英质岩浆房时,持续地发生两种岩浆的化学混合作用或两岩浆的机械混合作用或玄武质岩浆的侵入,其混合作用的时间以长英质岩锆石的U_Pb谐和不一致曲线上交点年龄822±4Ma界定。根据Nd模式年龄(tDM)和Nd富集系数(fSm/Nd)分布特征,可以确定中元古代江南造山带为太古宙扬子古陆核的横向增生体,而新元古代陆相火山侵入杂岩带则横向增生于江南造山带南缘。至此,扬子古陆横向增生作用结束,开始与华夏古陆拼贴,包括港边火成杂岩体在内的新元古代火山侵入杂岩带则成为两古陆连结的纽带。  相似文献   

富金斑岩型铜矿床的基本特征、成矿物质来源与成矿高氧化岩浆-流体演化   总被引：17，自引：12，他引：17  

李金祥秦克章  李光明 《岩石学报》2006,22(3):678-688

第三纪富金斑岩型铜矿床主要发育于板块汇聚边缘与俯冲作用相关的火山-岩浆弧以及陆缘弧中,而大多数较古老的富金斑岩型铜矿床则主要发育于向大陆边缘增生的岛弧环境中.含矿斑岩的岩性变化范围从低钾钙碱性闪长岩、石英闪长岩和英云闪长岩到高钾钙碱性石英二长岩到碱性的二长岩及正长岩,通常侵位于地壳浅部l～2km处,与同期的火山岩密切共生,并常见热液爆破角砾岩.其围岩蚀变从早到晚依次可分为Ca-Na硅酸盐蚀变、K硅酸盐蚀变、中级泥质蚀变、绢云母化、高级泥质蚀变,而浅部的高级泥质蚀变可以与早期K硅酸盐蚀变同期形成.Cu、Au矿化主要发育在K硅酸盐蚀变带中,矿化与A型脉密切相关,贫钼而富铂族元素.控制富金斑岩型铜矿床形成的几个关键过程包括：（1）源区有大量的Cu、Au等成矿元素;（2）能使Cu、Au等成矿物质有效进入岩浆熔体的机制;（3）合成矿元素的岩浆熔体在从地幔上升到地壳高侵位而形成斑岩体的过程中没有Cu、Au等成矿物质损失;（4）在岩浆上升演化过程中,岩浆挥发份能有效的逸出,并且逸出的时间越早,对成矿越有利;（5）Cu、Au等成矿元素能有效进入岩浆挥发份;（6）在成矿斑岩体上部发育有利的相对封闭机制,阻止岩浆挥发份的逃逸;（7）含Cu、Au成矿流体的有效沉淀机制;（8）具有一个地壳上部的岩浆房,能够不断提供成矿物质和驱动热液循环的热能.要形成大型矿床一般需要多期岩浆脉动侵位与多期矿化热液蚀变事件的叠加.现多倾向认为交代的地幔楔可能是其主要物质来源.而有利于富金斑岩型铜矿床形成的岩浆有钾质钙碱性岩浆、埃达克质岩浆、碱性弧岩浆.俯冲板片脱水形成的流体或者熔融产生熔体提供了上覆地幔楔熔融的高氧逸度条件,这种高氧逸度特征是地幔源区Cu、Au成矿元素能否进入岩浆熔体的重要条件之一.最近研究表明流体的冷却可能是Cu、Au沉淀成矿最主要的因素.本文扼要介绍了富金斑岩型铜矿的矿床地质特征、矿床成因等方面的研究进展,分析了存在的主要问题并对其发展趋势作了展望.  相似文献   

湘东南志留纪彭公庙花岗岩体的地质地球化学特征及其构造环境   总被引：15，自引：1，他引：15  

柏道远  黄建中  马铁球  王先辉 《现代地质》2006,20(1):130-140

志留纪彭公庙岩体地处湘东南,岩石类型主要为黑云母花岗闪长岩、黑云母二长花岗岩、二云母二长花岗岩。各岩石单元从早至晚,w(S iO2)总体由低变高,变化在65.30%~73.42%之间;w(K2O)平均为4.34%,w(Na2O+K2O)为6.46%~8.32%,平均为7.09%;w(K2O)/w(Na2O)平均为1.58;岩石富铝,w(A l2O3)平均为14.13%。岩体总体属铁质、强过铝质高钾钙碱性花岗岩。Ba、Nb、Sr、P、Ti相对于原始地幔为负异常,Rb、(Th+U)、(La+Ce)、Nd、(Zr+H f+Sm)、(Y+Yb)等则相对富集。w(ΣREE)平均为221.85×10-6;轻稀土富集,w(La)N/w(Yb)N值平均为8.66;Eu弱亏损,δ(Eu)平均为0.53。ISr值为0.712 30~0.718 31,εSr(t)为110.7~196.1,εNd(t)为-8.0~-8.7,t2DM为1.81~1.87 Ga。上述地球化学特征表明彭公庙岩体为S型花岗岩。在C/MF-A/MF图解中,样品点部分落入基性岩区,部分落入变质碎屑岩区;在岩体氧化物比值的Harker图解中,各样点构成良好的线性关系;在w(La)/w(Sm)-w(La)图解中样品点分布散乱;酸性程度最高的晚期恩垄岩石单元的轻稀土相对富集更为明显;岩石中发育镁铁质岩浆包体等,表明彭公庙岩体具岩浆混合成因。地球化学构造环境判别图解、岩体侵位地质特征以及区域构造演化背景等表明彭公庙岩体形成于后造山构造环境。岩体各岩石单元侵位的先后次序可能与岩浆的粘度密切相关,基性程度相对较高的岩浆向上运移速度更快,因而侵位更早。  相似文献   

新疆阿尔泰山南缘泥盆纪弧型苦橄岩铂族元素地球化学特征及其地质意义     

张招崇  周刚  闫升好  陈柏林  贺永康  柴凤梅  何立新 《现代地质》2006,20(4):519-526

全球岛弧火山岩的铂族元素数据非常少。本研究对新疆阿尔泰山南缘中泥盆世北塔山组地层中的苦橄岩的铂族元素进行了分析,结果表明:其铂族元素的含量总体变化不大,其原始地幔标准化曲线总体上和已经报道的大西洋Lesser Antilles岛弧的G renada苦橄岩相似,均以富集钯组铂族元素(PPGE)为特征,但总体含量比后者高,而比大火成岩省的苦橄岩低。一些铂族元素的特征比值指示了苦橄岩和富辉玄武岩起源于软流圈地幔,而高的w(Os)/w(Ir)比值则暗示了源区中有深海沉积物的加入。w(Pd)/w(Ir)-w(N i)/w(Cu)图解说明本区的苦橄岩不是原始岩浆,而是原始的高镁玄武岩中有过剩橄榄石的加入,而w(Pd)-w(Cu)图解则说明原始岩浆硫不饱和。IPGE在俯冲带流体中相对稳定,而PPGE在俯冲带流体中的活动性相对较高。  相似文献   

广西姑婆山里松花岗岩中闪长质包体的地球化学特征及其成因探讨   总被引：8，自引：0，他引：8  

杨策  朱金初  张佩华  谢才富 《高校地质学报》2006,12(3):310-318

广西姑婆山里松花岗岩中广泛发育有大量的闪长质包体，包体的野外地质特征、显微结构、矿物组合及化学组成等特征显示其岩浆快速结晶成因。它们的主量元素在相关图上呈不同程度的直线变异关系。在微量元素方面，包体和寄主花岗岩都富含大离子亲石元素和高场强元素。用锆石饱和温度和角闪石成分估算了包体和寄主花岗岩结晶的温度和压力表明，它们的结晶温度和压力条件相近，分别在793—824℃和（3．5—5．1）×10^8Pa范围内。岩石学和同位素地球化学特征也表明，里松包体和寄主花岗岩基本同时结晶，但壳幔比例和来源有所不同。这些特征总体上说明了里松闪长质包体可能是两种岩浆混合时不完全消化的产物  相似文献   

金伯利岩中“熔离小球”的特征及其成因     

路凤香  张宏福  陈美华  郑建平  尹作为  任迎新  赵崇贺  叶德隆 《现代地质》2007,21(2):241-246

在金伯利岩人工重砂中发现的“熔离小球”,直径多数<1 mm,除个别出现微晶外,均为非晶质,属于熔体淬火冷却产物。提供了29个小球的主元素分析和3件微量元素分析结果。“熔离小球”按成分可分为3种类型:(1)高铁钛小球;(2)硫铁镍小球;(3)浅色硅铝质小球。其中高铁小球w(FeO)高达99.39%,高钛小球w(TiO2)达45.90%,它们含MnO也偏高,最高达23.75%。Fe、Mn、Ti都属于高负电性元素,在熔体中与氧结合的键强度大,容易发生熔离。硫铁镍小球的w(SO3)变化于38.27%~51.95%,w(FeO)为0.31%~23.10%,w(NiO)为25.24%~61.05%。浅色小球w(SiO2)变化范围为24.01%~52.64%,Al2O3、CaO含量高但变化范围大,总体成分接近基性—超基性硅酸盐熔浆。主元素、微量元素特征以及硫铁镍小球中发现了高镁(Fo=0.95)橄榄石捕虏晶表明,小球形成于金伯利岩岩浆的介质环境。此外高铁及硅铝质两种成分呈交生结构的两相小球的发现,暗示二者为熔离作用成因。小球的熔离作用可以应用SiO2-FeS-FeO的液态不混溶相图做出解释。认为小球形成于岩浆结晶的晚期阶段,相对富含CO2、SO3、FeO、MnO、TiO,在岩浆快速上升、快速降温、降压、熔体中出现了多种局部有序区的条件下发生的。  相似文献   

The influence of viscous and latent heating on crystal-rich magma flow in a conduit     

Alina J. Hale  Geoff Wadge  Hans B. Mühlhaus 《Geophysical Journal International》2007,171(3):1406-1429

  相似文献