湖南锡田岩体的岩浆混合成因:岩相学､岩石地球化学和U-Pb 年龄证据

南岭中段的锡田岩体燕山期岩石以斑状黑云母二长花岗岩为主,岩体中广泛发育暗色微粒包体?暗色微粒包体为岩浆结构,大多数具有塑性外形,发育淬冷边?反向脉,存在多种不平衡结构和矿物组合,如钾长石环斑?石英眼斑?针状磷灰石等,显示岩浆混合特征?岩石地球化学方面,暗色微粒包体具有比寄主岩贫硅?贫碱,富K?Fe?Mg?Ca?Ti 特征;暗色微粒包体及寄主岩富集轻稀土元素(LREE/HREE=2.6~8.8),具有中-强的铕负异常(δEu=0.09~0.74)以及具有相似的稀土元素配分曲线和微量元素蛛网图;在主要氧化物含量Harker 图解中投点多呈直线变异趋势,反映了两者具有密切的亲缘关系,利用共分母和不共分母图解进行判别,暗色微粒包体与寄主岩具岩浆混合特征,在MgO-TFeO判别图解中也指示包体为岩浆混合成因?上述岩相学和元素地球化学特征表明暗色微粒包体是基性岩浆侵入到酸性岩浆中淬冷形成的,指示锡田岩体存在两种岩浆的混合作用?通过LA-ICP-MS锆石U-Pb 定年,得到寄主岩形成年龄(150.04±0.52)Ma,暗色包体形成年龄(145.09±0.63)Ma,二者年龄在测试误差范围内一致,显示岩浆混合作用发生的时间大致为晚侏罗世?     

Geochemistry of mafic rocks and melt inclusions and their implications for the heat source of the 14.0°S hydrothermal field,South Mid-Atlantic Ridge

Fresh rocks sampled from the 14.0°S hydrothermal field of the South Atlantic Ridge can be divided into two categories： olivine-gabbro and basalt. The olivine-gabbro is composed mainly of three types of minerals： olivine, clinopyroxene and plagioclase, while a multitude of melt inclusions occur in the plagioclase phenocrysts of the basalts. We analyzed the whole-rock, major and trace elements contents of the basaks, the mineral chemistry of phenocrysts and melt inclusions in the basalts, and the mineral chemistry of olivine-clinopyroxene-plagioclase in the olivine-gabbro, then simulated magma evolution within the crust using the COMAGMAT program. The whole-rock geochemistry shows that all the basalts exhibit typical N-MORB characteristics. In addition, the mineral chemistry characteristics of the olivine-gabbro （low-Fo olivine, low-Mg# clinopyroxene, high-TiO2 clinopyroxene, low-An plagioclase）, show that strong magma differentiation occurred within the crust. Nevertheless, significant discrepancies between those minerals and phenocrysts in the basalts （high-Fo olivine, high-An plagioclase） reflect the heterogeneity of magma differentiation. High Mg# （-~0.72） melt inclusions isobaric partial crystallization simulations suggest that the magma differentiation occurred at the depth shallower than 13.03 km below the seafloor, and both the vertical differentiation column shows distinct discrepancies from that of a steady-state magma chamber. Instead, a series of independent magma intrusions probably occurred within the crust, and their corresponding crystallized bodies, as the primary high-temperature thermal anomalies within the off-axis crust, probably act as the heat source for the development of the 14.0°S hydrothermal system.     

Compositional Zoning of the Bishop Tuff

Compositional data for >400 pumice clasts, organized accordingto eruptive sequence, crystal content, and texture, providenew perspectives on eruption and pre-eruptive evolution of the>600 km³ of zoned rhyolitic magma ejected as the Bishop Tuffduring formation of Long Valley caldera. Proportions and compositionsof different pumice types are given for each ignimbrite packageand for the intercalated plinian pumice-fall layers that eruptedsynchronously. Although withdrawal of the zoned magma was lesssystematic than previously realized, the overall sequence displaystrends toward greater proportions of less evolved pumice, morecrystals (0·5–24 wt %), and higher FeTi-oxide temperatures(714–818°C). No significant hiatus took place duringthe 6 day eruption of the Bishop Tuff, nearly all of which issuedfrom an integrated, zoned, unitary reservoir. Shortly beforeeruption, however, the zoned melt-dominant portion of the chamberwas invaded by batches of disparate lower-silica rhyolite magma,poorer in crystals than most of the resident magma but slightlyhotter and richer in Ba, Sr, and Ti. Interaction with residentmagma at the deepest levels tapped promoted growth of Ti-richrims on quartz, Ba-rich rims on sanidine, and entrapment ofnear-rim melt inclusions relatively enriched in Ba and CO₂.Varied amounts of mingling, even in higher parts of the chamber,led to the dark gray and swirly crystal-poor pumices sparselypresent in all ash-flow packages. As shown by FeTi-oxide geothermometry,the zoned rhyolitic chamber was hottest where crystal-richest,rendering any model of solidification fronts at the walls orroof unlikely. The main compositional gradient (75–195ppm Rb; 0·8–2·2 ppm Ta; 71–154 ppmZr; 0·40–1·73% FeO*) existed in the melt,prior to crystallization of the phenocryst suite observed, whichincluded zircon as much as 100 kyr older than the eruption.The compositions of crystals, though themselves largely unzoned,generally reflect magma temperature and the bulk compositionalgradient, implying both that few crystals settled or were transportedfar and that the observed crystals contributed little to establishingthat gradient. Upward increases in aqueous gas and dissolvedwater, combined with the adiabatic gradient (for the 5 km depthrange tapped) and the roofward decline in liquidus temperatureof the zoned melt, prevented significant crystallization againstthe roof, consistent with dominance of crystal-poor magma earlyin the eruption and lack of any roof-rind fragments among theBishop ejecta, before or after onset of caldera collapse. Amodel of secular incremental zoning is advanced wherein numerousbatches of crystal-poor melt were released from a mush zone(many kilometers thick) that floored the accumulating rhyoliticmelt-rich body. Each batch rose to its own appropriate levelin the melt-buoyancy gradient, which was self-sustaining againstwholesale convective re-homogenization, while the thick mushzone below buffered it against disruption by the deeper (non-rhyolitic)recharge that augmented the mush zone and thermally sustainedthe whole magma chamber. Crystal–melt fractionation wasthe dominant zoning process, but it took place not principallyin the shallow melt-rich body but mostly in the pluton-scalemush zone before and during batchwise melt extraction. KEY WORDS: Bishop Tuff; ignimbrite; magma zonation; mush model; rhyolite     

Phase Equilibria Constraints on the Chemical and Physical Evolution of the Campanian Ignimbrite

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     

江西德兴斑岩铜矿石英闪长玢岩成因及成矿学意义

为探究石英闪长玢岩成因及幔源基性岩浆对斑岩铜矿的贡献,本文选取德兴矿床石英闪长玢岩开展了锆石U-Pb定年、Hf同位素和全岩地球化学研究。获得石英闪长玢岩LA-ICP-MS锆石U-Pb年龄为169 Ma,与成矿花岗闪长斑岩侵位时间一致,岩体为中侏罗世岩浆活动的产物。石英闪长玢岩具有低的SiO₂(58.41%~63.12%)和K₂O(1.68%~2.94%)含量及A/CNK值(0.85~1.04),富集大离子亲石元素和轻稀土元素,亏损高场强元素Nb、Ta、Ti和重稀土元素,属于钙碱性到高钾钙碱性系列岩石。具有相对亏损的锆石Hf同位素组成,εHf(t)=2.20~7.93(最大值7.93),指示其源区为岩石圈地幔。锆石稀土元素配分模式图显示出明显的正Ce异常,岩浆氧逸度(lg f_O2)为-20.05~-6.66,达到磁铁矿-赤铁矿氧逸度等级,指示石英闪长玢岩结晶自高氧逸度岩浆。全岩地球化学特征显示,德兴石英闪长玢岩与成矿花岗闪长斑岩及其暗色包体符合岩浆混合的演化趋势,说明成矿花岗闪长斑岩可能是中侏罗世幔源基性岩浆和地壳酸性岩浆大规模混合作用的产物,并且石英闪长玢岩代表了岩浆混合过程中的幔源基性端员。结合前人研究成果,认为在中侏罗世伸展构造背景下,软流圈物质上涌导致新元古代受交代的岩石圈地幔部分熔融形成幔源基性岩浆,基性岩浆的底侵作用诱发下地壳物质熔融并与之发生一定程度的岩浆混合作用,形成了花岗闪长斑岩的母岩浆。高氧逸度幔源岩浆的加入可抑制斑岩体系硫化物的过早饱和,同时为德兴矿床注入了成矿所需的部分挥发分和金属元素。     

江西印支期蔡江岩体中暗色微粒包体的发现及其地质意义

文章报道了江西蔡江花岗质岩体中发现暗色微粒包体,以及这些包体的地质、岩相学、LA-ICP-MS锆石U-Pb年代学和元素地球化学特征。包体多呈椭圆状,显示淬冷边和反向脉,具有典型的岩浆结构并含有针状磷灰石,有的包体含有长石捕虏晶。包体具有相对较低的SiO₂（低至57.05 wt%）和较高的MgO+Fe₂O₃（高达14.21 wt%）含量。LA-ICP-MS锆石U-Pb定年数据表明,包体形成于晚三叠世（224 Ma）,与寄主花岗岩（230~228 Ma）在误差范围内基本一致。上述特征表明,包体是离散的幔源偏基性岩浆团或者是幔源与寄主岩浆混合的产物。原始包体岩浆属于超钾质岩浆,可能是通过岩石圈地幔中交代成因的金云母辉石岩脉发生部分熔融而形成的。暗色微粒包体的发现为幔源岩浆底侵提供了直接证据,从而为蔡江花岗质岩石形成于较高温度提供佐证。该研究对于进一步探讨华南印支期花岗岩形成的热源机制具有意义。     

热力学计算模拟对初始月幔结构的约束SCIEI北大核心CSCD

月球岩浆洋结晶形成的初始月球内部结构是其后续演化过程的开端,其结晶过程受月球岩浆洋的初始深度和物质组成这两个参数的制约。由于缺少直接来自月球深部的岩石样品,目前关于月球岩浆洋演化过程的探讨主要依赖实验和计算模拟手段。岩浆洋模型中形成的月壳厚度是否与探测结果一致是月球岩浆洋演化模型合理性的重要约束。最新的GRAIL(Gravity Recovery and Interior Laboratory)探测数据推算月壳厚度为34~43km,低于阿波罗时期认为的约70km,这对已有的月球岩浆洋演化模型提出了挑战。本文采用并修正FXMOTR程序包,针对月球岩浆洋在不同的初始深度和物质组成情况下的结晶过程,进行了一系列热力学计算模拟。通过量化月球岩浆洋的初始深度和物质组成对月壳厚度的影响,结合关于月球内部微量元素分配的研究结果,对比了月球岩浆洋结晶后期的残余熔体与原始克里普组分(urKREEP)的成分。本文的模拟结果显示,一个全月幔熔融且初始成分为月球初始上月幔组成(LPUM)的岩浆洋将在其深部结晶2.5%石榴子石,形成的月壳厚度符合GRAIL的约束,并且结晶出了合适的urKREEP成分。在此模型的基础上获取了月球初始的内部成分和密度结构,并对后期月幔翻转(Overturn)的程度进行了探讨。     

西藏厅宫斑岩铜矿床地质、蚀变及矿化特征研究

本文对西藏厅宫大型铜矿进行了详细研究,矿床详细的地质岩相学-蚀变以及典型剖面填图表明,矿区存在2个岩浆事件高峰,即始新世的钾长花岗岩(~50 Ma)和中新世的斑状二长花岗岩、英云闪长斑岩及闪长玢岩(约13~17 Ma)。野外和室内研究发现,厅宫矿区存在2期重要的矿化事件,即始新世(~50 Ma)铜矿化及中新世(~15Ma)的铜钼矿化。始新世含矿岩体为钾长花岗岩,其最主要的特点是其成矿岩体结构的特殊性,表现在该矿床的成矿岩体没有典型的斑状结构,而是独特的细晶-似伟晶结构,说明含矿岩浆发生过骤冷,可能是流体突然逃逸,矿物结晶的固相点发生漂移所致。同时,该岩体还发育大量显微文象结构、显微晶洞构造等,均说明岩浆曾经富水,并且曾经流体饱和;中新世含矿岩体为具有埃达克岩特征的斑状二长花岗岩,主要以脉状的铜、钼矿化为主。该矿床蚀变分带类似于冈底斯带其他斑岩矿床。时间上,分别为早期的钾硅酸盐化、转换阶段的青磐岩化、随后的绢英岩化及最晚期的泥化蚀变;空间上,以含矿岩体为中心向外依次为钾硅酸盐化、绢英岩化、青磐岩化,最晚期的泥化呈补丁状或条带状叠加早期各类蚀变。铜矿化主要发生在始新世的黑云母化阶段和中新世的绢英岩化阶段,而钼矿化主要发生在中新世的钾硅酸盐化和绢英岩化的转换阶段。     

东疆二叠纪镁铁-超镁铁岩体中辉石的成分特征及其对成岩和Ni-Cu成矿的指示

新疆东部早二叠世镁铁-超镁铁岩体主要分布在天山东段觉罗塔格构造带、中天山地块和北山地区,与这类岩体相关的Ni-Cu矿床主要产出在觉罗塔格带和中天山地区,北山目前并未发现典型Ni-Cu矿床。这些岩体中的斜方辉石主要为古铜辉石,少量为紫苏辉石;单斜辉石属透辉石、次透辉石或普通辉石。矿物成分系统变化显示橄榄石Fo值北山最高、觉罗塔格带到中天山逐次降低的特点,橄榄石Fo值在78~86和Ni含量低于1800×10-6范围内更有利于Cu-Ni成矿;斜方辉石En端元和单斜辉石Wo端元极差值也显示北山最高、觉罗塔格带和中天山较低的规律,且相对小的极差值更有利于成矿。单斜辉石AlⅣ/AlⅥ比值结果显示北山岩体在矿物结晶过程中压力较低,硫溶解度较大,可能是其矿化程度弱于觉罗塔格带和中天山的一个重要因素。觉罗塔格带、中天山和北山镁铁-超镁铁质岩体的母岩浆为非碱性系列、大陆拉斑玄武质岩浆。根据北山和觉罗塔格带岩体单斜辉石微量元素成分估算的母岩浆具有LREE富集以及Nb、Ta、Zr、Hf负异常的特征,指示出两者源区为受俯冲板片交代的地幔,且坡北源区俯冲交代程度更低。觉罗塔格带和中天山单斜辉石Alz vs.Ti显示裂谷堆晶趋势向弧堆晶趋势演化,而北山单斜辉石Alz vs.Ti则显示明显的裂谷堆晶趋势,这说明俯冲交代作用在觉罗塔格带和中天山地区表现的更为强烈。北山镁铁-超镁铁岩体中发现单斜辉石Ti的高异常及矿物温压计算结果显示,表明北山地区具有比觉罗塔格带和中天山更高的岩浆温度,这可能与塔里木二叠纪地幔柱的活动有关。