Fluid and source magma evolution of the Questa porphyry Mo deposit,New Mexico,USA   总被引：14，自引：1，他引：13  

Leonhard M. Klemm  Thomas Pettke  Christoph A. Heinrich 《Mineralium Deposita》2008,43(5):533-552

Combined fluid inclusion microthermometry and microanalysis by laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS) are used to constrain the hydrothermal processes forming a typical Climax-type porphyry Mo deposit. Molybdenum mineralisation at Questa occurred in two superimposed hydrothermal stages, a magmatic-hydrothermal breccia and later stockwork veining. In both stages, texturally earliest fluids were single-phase, of low salinity (~7 wt.% NaCl_equiv.) and intermediate-density. Upon decompression to ~300 bar, they boiled off a vapour phase, leaving behind a residual brine (up to 45 wt.% NaCl_equiv) at temperatures of ~420°C. The highest average Mo concentrations in this hot brine were ~500 μg/g, exceeding the Mo content of the intermediate-density input fluid by about an order of magnitude and reflecting pre-concentration of Mo by fluid phase separation prior to MoS₂ deposition from the brine. Molybdenum concentrations in brine inclusions, then, decrease down to 5 μg/g, recording Mo precipitation in response to cooling of the saline liquid to ~360°C. Molybdenite precipitation from a dense, residual and probably sulphide-depleted brine is proposed to explain the tabular shape of the ore body and the absence of Cu-Fe sulphides in contrast to the more common Cu-Mo deposits related to porphyry stocks. Cesium and Rb concentrations in the single-phase fluids of the breccia range from 2 to 8 and from 40 to 65 μg/g, respectively. In the stockwork veins, Cs and Rb concentrations are significantly higher (45–90 and 110–230 μg/g, respectively). Because Cs and Rb are incompatible and hydrothermally non-reactive elements, the systematic increase in their concentration requires two distinct pulses of fluid exsolution from a progressively more fractionated magma. By contrast, major element and ore metal concentrations of these two fluid pulses remain essentially constant. Mass balance calculations using fluid chemical data from LA-ICPMS suggest that at least 25 km³ of melt and 7 Gt of deep input fluid were necessary to provide the amount of Mo contained in the stockwork vein stage alone. While the absolute amounts of fluid and melt are uncertain, the well-constrained element ratios in the fluids together with empirical fluid/melt partition coefficients derived from the inclusion analyses suggest a high water content of the source melt of ~10%. In line with other circumstantial evidence, these results suggest that initial fluid exsolution may have occurred at a confining pressure exceeding 5 kbar. The source of the molybdenum-mineralising fluids probably was a particularly large magma chamber that crystallised and fractionated in the lower crust or at mid-crustal level, well below the shallow intrusions immediately underlying Questa and other porphyry molybdenum deposits. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献   

SHRIMP zircon dating and Sm/Nd isotopic investigations of Neoproterozoic granitoids, Eastern Desert, Egypt   总被引：2，自引：0，他引：2  

Ewais M.M. Moussa  Robert J. Stern  William I. Manton  Kamal A. Ali 《Precambrian Research》2008,160(3-4):341-356

There is an increasing evidence for the involvement of pre-Neoproterozoic zircons in the Arabian–Nubian Shield, a Neoproterozoic crustal tract that is generally regarded to be juvenile. The source and significance of these xenocrystic zircons are not clear. In an effort to better understand this problem, older and younger granitoids from the Egyptian basement complex were analyzed for chemical composition, SHRIMP U–Pb zircon ages, and Sm–Nd isotopic compositions. Geochemically, the older granitoids are metaluminous and exhibit characteristics of I-type granites and most likely formed in a convergent margin (arc) tectonic environment. On the other hand, the younger granites are peraluminous and exhibit the characteristics of A-type granites; these are post-collisional granites. The U–Pb SHRIMP dating of zircons revealed the ages of magmatic crystallization as well as the presence of slightly older, presumably inherited zircon grains. The age determined for the older granodiorite is 652.5 ± 2.6 Ma, whereas the younger granitoids are 595–605 Ma. Xenocrystic zircons are found in most of the younger granitoid samples; the xenocrystic grains are all Neoproterozoic, but fall into three age ranges that correspond to the ages of other Eastern Desert igneous rocks, viz. 710–690, 675–650 and 635–610 Ma. The analyzed granitoids have (+3.8 to +6.5) and crystallization ages, which confirm previous indications that the Arabian–Nubian Shield is juvenile Neoproterozoic crust. These results nevertheless indicate that older Neoproterozoic crust contributed to the formation of especially the younger granite magmas.  相似文献   

Chemical and boron-isotope variations in tourmalines from an S-type granite and its source rocks: the Erongo granite and tourmalinites in the Damara Belt,Namibia   总被引：3，自引：0，他引：3  

R. B. Trumbull  M.-S. Krienitz  B. Gottesmann  M. Wiedenbeck 《Contributions to Mineralogy and Petrology》2008,155(1):1-18

Tourmaline is widespread in metapelites and pegmatites from the Neoproterozoic Damara Belt, which form the basement and potential source rocks of the Cretaceous Erongo granite. This study traces the B-isotope variations in tourmalines from the basement, from the Erongo granite and from its hydrothermal stage. Tourmalines from the basement are alkali-deficient schorl-dravites, with B-isotope ratios typical for continental crust (δ¹¹B average −8.4‰ ± 1.4, n = 11; one sample at −13‰, n = 2). Virtually all tourmaline in the Erongo granite occurs in distinctive tourmaline-quartz orbicules. This “main-stage” tourmaline is alkali-deficient schorl (20–30% X-site vacancy, Fe/(Fe + Mg) 0.8–1), with uniform B-isotope compositions (δ¹¹B −8.7‰ ± 1.5, n = 49) that are indistinguishable from the basement average, suggesting that boron was derived from anatexis of the local basement rocks with no significant shift in isotopic composition. Secondary, hydrothermal tourmaline in the granite has a bimodal B-isotope distribution with one peak at about −9‰, like the main-stage tourmaline, and a second at −2‰. We propose that the tourmaline-rich orbicules formed late in the crystallization history from an immiscible Na–B–Fe-rich hydrous melt. The massive precipitation of orbicular tourmaline nearly exhausted the melt in boron and the shift of δ¹¹B to −2‰ in secondary tourmaline can be explained by Rayleigh fractionation after about 90% B-depletion in the residual fluid. Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献   

西天山特克斯达坂库勒萨依序列埃达克岩的确立及钼找矿意义   总被引：9，自引：6，他引：3  

李永军  辜平阳  庞振甲  栾新东  佟丽莉 《岩石学报》2008,24(12):2713-2719

库勒萨依序列斑岩体δ平均3.05,属于钙碱性系列岛弧浅成岩。 SiO₂含量为57.06％~70.74％,高Al₂O₃、Na₂O、Sr和相对富集LREE,低MgO、Y、Yb,强烈亏损HREE。Na₂O/K₂O＞1,Sr/Y平均57.67,正Eu异常,因而具有典型O型埃达克岩特征。库勒萨依序列斑岩体与Mo异常套合好,已发现钼矿体,找矿前景良好。该埃达克岩的确立,对深化西天山区域成矿规律和指导今后找矿具有借鉴和指导意义。  相似文献   

郯庐断裂带张八岭隆起南段花岗岩LA-ICP MS锆石U-Pb年龄及其构造意义   总被引：10，自引：8，他引：2  

牛漫兰  朱光  谢成龙  柳小明  曹洋  谢文雅 《岩石学报》2008,24(8)

本文利用LA-ICP MS方法,对零星分布于郯庐断裂带张八岭隆起南段肥东-巢湖地区的一些花岗岩体进行了锆石U-Pb同位素年代学研究.结果表明,西徐村北岩体、尖山岩体、西花村岩体、永丰岩体和锦张村岩体的形成年龄分别为126.9 ±1.0Ma、114.8±1.3Ma、108.1 ±1.6Ma、103.0 ±0.9Ma和120.3 ±0.7Ma,这些花岗岩体均形成于早白垩世,但侵位时间有一定差异.与郯庐断裂带西侧的鲁西、徐淮、蚌埠地区同时代克拉通内部侵入岩相比,断裂带内岩浆活动持续的时间更长(～27Ma).这一结果不但指示郯庐断裂带上的岩浆活动是不均一的,各地岩浆在活动的强烈程度和时间特征上均有很大的差异,而且显示了断裂带内比克拉通内部岩浆活动结束时间较晚,暗示其下岩石圈可能有更为强烈的减薄程度和更长的减薄历史.  相似文献   

花岗岩研究的误区——关于花岗岩研究的思考之五   总被引：3，自引：3，他引：0  

张旗  潘国强  李承东  金惟俊  贾秀勤 《岩石学报》2008,24(10):2212-2218

本文在对花岗岩四大基石(混合作用、结晶分离作用、构造环境和源区)问题分析的基础上,指出花岗岩研究存在的三大误区: (1)不恰当地仿效玄武岩的理论和研究方法,忽视了花岗岩的复杂性。(2)不恰当地用板块构造学说解释大陆花岗岩问题。板块构造是地球演化到一定阶段的产物,并成功解释了与板块边界相联系的岩浆活动,但是,它不能解决主要来源于大陆的花岗岩的地质问题。(3)太过重视花岗岩的地球化学研究而忽视了对花岗岩基础地质的研究。作者指出,地球化学方法在花岗岩中的使用应当是有限制的,花岗岩研究陷入误区是我们缺少扎实的基础研究、对板块构造的理解不深和对花岗岩复杂性认识不足等三个方面的原因造成的。文中还批评了学术界存在的人云亦云的奴性思想,指出它严重地阻碍了我们的创新思维,是当前亟待改进和克服的。  相似文献   

21世纪的花岗岩研究, 路在何方？——关于花岗岩研究的思考之六     

张旗  潘国强  李承东  金惟俊  贾秀勤 《岩石学报》2008,24(10):2219-2236

21世纪的花岗岩怎样研究是一个需要探索的问题。作者认为,应当对现有的花岗岩理论、流行的说法以及术语等进行清理和反思,汲取其精华,剔除其糟粕,抛弃那些不科学、不符合实际、不符合逻辑的部分。例如,在花岗岩研究中摈弃结晶分离的理论,缩小花岗岩混合作用的意义,限制花岗岩构造环境理论的应用,取消幔源、壳源和壳幔混合源的术语等。作者指出,今后花岗岩研究应当着重解决两个问题: (1)花岗岩是怎样的？(2)它何以是这样的？文中提出5个方面的任务作为今后研究的重点,即: 开展花岗岩立典式的研究,将花岗岩研究与古老地壳的研究结合起来,将花岗岩物理性质研究与地球化学究结合起来,开展广泛的实验岩石学研究和创建新的“大陆构造学”理论。鉴于花岗岩研究目前存在的严重误区,现有的花岗岩理论几乎全面崩溃,由四大基石支撑的花岗岩大厦行将坍塌,花岗岩研究正面临全球大洗牌。为此,作者建议开展一场关于花岗岩的大辩论,目的是清理思路,认清问题,明确方向,找到出路。作者呼吁,我们应当加强学习,加速引进人才,克服急躁情绪和浮夸的学风,摈弃从众思想和奴性思想,不以SCI论英雄,改进我们的学习,改善我们的制度,以推进花岗岩研究迈上新台阶。  相似文献   

大理宾川小龙潭斑岩型铜矿     

王列  陈梁  孙德瑜 《云南地质》2008,27(2):253-256

矿体赋存于不同构造过渡带断裂侧,控矿岩石为喜马拉雅期浅成—超浅成相的富钾碱性系列的中酸性侵入体,属于斑岩型铜矿。  相似文献   

Heat flow and crustal thermal structure in the Late Archaean Closepet Granite batholith,south India     

Sukanta Roy  Labani Ray  Anurup Bhattacharya  R. Srinivasan 《International Journal of Earth Sciences》2008,97(2):245-256

The Late Archaean Closepet Granite batholith in south India is exposed at different crustal levels grading from greenschist facies in the north through amphibolite and granulite facies in the south along a ∼400 km long segment in the Dharwar craton. Two areas, Pavagada and Magadi, located in the Main Mass of the batholith, best represent the granitoid of the greenschist and amphibolite facies crustal levels respectively. Heat flow estimates of 38 mW m⁻² from Pavagada and 25 mW m⁻² from Magadi have been obtained through measurements in deep (430 and 445 m) and carefully sited boreholes. Measurements made in four boreholes of opportunity in Pavagada area yield a mean heat flow of 39 ± 4 (s.d.) mW m⁻², which is in good agreement with the estimate from deep borehole. The study, therefore, demonstrates a clear-cut heat flow variation concomitant with the crustal levels exposed in the two areas. The mean heat production estimates for the greenschist facies and amphibolite facies layers constituting the Main Mass of the batholith are 2.9 and 1.8 μW m⁻³, respectively. The enhanced heat flow in the Pavagada area is consistent with the occurrence of a radioelement-enriched 2-km-thick greenschist facies layer granitoid overlying the granitoid of the amphibolite facies layer which is twice as thick as represented in the Magadi area. The crustal heat production models indicate similar mantle heat flow estimates in the range 12–14 mW m⁻², consistent with the other parts of the greenstone-granite-gneiss terrain of the Dharwar craton.  相似文献   

The transition from peraluminous to peralkaline granitic melts: Evidence from melt inclusions and accessory minerals     

R. Thomas  J.D. Webster  D. Rhede  W. Seifert  K. Rickers  H.-J. Frster  W. Heinrich  P. Davidson 《Lithos》2006,91(1-4):137-149

Fractional crystallization of peraluminous F- and H₂O-rich granite magmas progressively enriches the remaining melt with volatiles. We show that, at saturation, the melt may separate into two immiscible conjugate melt fractions, one of the fractions shows increasing peraluminosity and the other increasing peralkalinity. These melt fractions also fractionate the incompatible elements to significantly different degrees. Coexisting melt fractions have differing chemical and physical properties and, due to their high density and viscosity contrasts, they will tend to separate readily from each other. Once separated, each melt fraction evolves independently in response to changing T/P/X conditions and further immiscibility events may occur, each generating its own conjugate pair of melt fractions. The strongly peralkaline melt fractions in particular are very reactive and commonly react until equilibrium is attained. Consequently, the peralkaline melt fraction is commonly preserved only in the isolated melt and mineral inclusions.

We demonstrate that the differences between melt fractions that can be seen most clearly in differing melt inclusion compositions are also visible in the composition of the resulting ore-forming and accessory minerals, and are visible on scales from a few micrometers to hundreds of meters.  相似文献