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1.
Emelie Axelsson Jonas Pape Jasper Berndt Fernando Corfu Klaus Mezger Michael M. Raith 《Geostandards and Geoanalytical Research》2018,42(3):319-338
A new natural rutile reference material is presented, suitable for U‐Pb dating and Zr‐in‐rutile thermometry by microbeam methods. U‐Pb dating of rutile R632 using laser ablation ICP‐MS with both magnetic sector field and quadrupole instruments as well as isotope dilution‐thermal ionisation mass spectrometry yielded a concordia age of 496 ± 2 Ma. The high U content (> 300 μg g?1) enabled measurement of high‐precision U‐Pb ages despite its young age. The sample was found to have a Zr content of 4294 ± 196 μg g?1, which makes it an excellent complementary reference material for Zr‐in‐rutile thermometry. Individual rutile grains have homogeneous compositions of a number of other trace elements including V, Cr, Fe, Nb, Mo, Sn, Sb, Hf, Ta and W. This newly characterised material significantly expands the range of available rutile reference materials relevant for age and temperature determinations. 相似文献
2.
Rutile to Titanite Transformation in Eclogites and its Geochemical Consequences: An Example from the Sumdo Eclogite, Tibet 下载免费PDF全文
ZHAO Linghao ZENG Lingsen GAO Li’e HU Mingyue SUN Dongyang ZHANG Lifei 《《地质学报》英文版》2023,97(1):122-133
The formation of titanite coronae after rutile is common in retrograde high-to ultrahigh-pressure meta-mafic rocks, which provides a good opportunity to address the geochemical behavior of HFSE in crustal environments. In the Sumdo eclogite, titanite occurs either as a corona around rutile grains or as semi-continuous veins cross-cutting the major foliation, whereas rutile grains occur either as inclusions in garnet or omphacite or as a relict core surrounded by titanite. Textural relationships ... 相似文献
3.
Shyh‐Lung Hwang Pouyan Shen Hao‐Tsu Chu Tzen‐Fu Yui Yoshiyuki Iizuka Hans‐Peter Schertl 《Journal of Metamorphic Geology》2019,37(8):1079-1098
Metamorphic garnet commonly contains needle‐like rutile inclusions as well as equant rutile inclusions that surround quartz inclusions and range in size from submicrometer to nanometer. Although the origin of these equant rutile inclusions, that is, exsolution or non‐exsolution, has important implications for petrological and tectonic processes, the crystallographic characteristics of these inclusions have rarely been studied because of the small sizes and analytical difficulties involved. Here, we report the crystallographic characteristics pertinent to the genetic origin of minute equant rutile inclusions in cloudy, nearly spherically shaped garnet domains with Ti‐depleted compositions surrounding quartz inclusions in ultrahigh‐pressure garnet from several diamondiferous Erzgebirge quartzofeldspathic gneissic rock samples. TEM analyses show that the equant rutile crystals in cloudy garnet domains are partially bounded by the low‐energy {100}rt ± {110}rt ± {101}rt facets and have rather random crystallographic orientation relationships (CORs) with the garnet host, with preferential alignment of low‐energy lattice planes, for example, {100}rt//{112}grt, for some rutile crystals. Although the rather random CORs are unlikely to be attributed to solid‐state exsolution subjected to the stringent topotactic garnet lattice constraints, the characteristic subhedral {100}rt ± {110}rt ± {101}rt crystal forms of rutile can be rationalized by a metasomatic dissolution‐reprecipitation mechanism via a fluid phase. In this scenario, the quartz+fluid inclusions in garnet were first subjected to decompression microcracking during rock exhumation, followed by dissolution of Ti‐bearing garnet matrix at the crack tips or along the crack surfaces and subsequent reprecipitation of rutile, apatite, gahnite, akdalaite, and Ti‐depleted garnet. The rapid coalescence between rutile and garnet crystals in fluid or direct attachment of rutile crystals onto the dissolving crack surfaces would then yield the rather random CORs as reported here. These results, along with previous work on rutile needles, indicate rather diverse genesis of rutile inclusions in various crystal forms, thus shedding light on the controversial exsolution origin for other inclusion suite/microstructure in minerals. 相似文献
4.
Niobium and Ta concentrations in ultrahigh‐pressure (UHP) eclogites and rutile from these eclogites and associated high pressure (HP) veins were used to study the behaviour of Nb–Ta during dehydration and fluid‐rock interaction. Samples were collected through a ~2 km profile at the Bixiling complex in the Dabie orogenic belt, Central‐Eastern China. All but one eclogite away from veins (EAVs) display nearly constant Nb/Ta ratios ranging from 16.1 to 19.2, with an average of 16.9 ± 0.8 (2 SE), similar to that of their gabbroic protolith from the Yangtze Block. Nb/Ta ratios of rutile from the EAVs range from 12.7 to 25.3 among different individual grains, with the average values close to those of the corresponding bulk rocks. These observations show that Nb and Ta were not significantly fractionated by prograde metamorphism up to eclogite facies when no significant fluid‐rock interaction occurs. In contrast, Nb/Ta ratios of rutile from eclogites close to veins (ECVs) are highly variable from 17.8 to 49.8, which are systematically higher (by up to 17) than those of rutile from the veins. These observations demonstrate that Nb and Ta were mobilized and fractionated during localized fluid flow and intensive fluid‐rock interaction. This is strongly supported by Nb/Ta zoning patterns in single rutile grains revealed by in situ LA‐ICP‐MS analysis. Ratios of Nb/Ta in the ECV‐hosted rutile decrease gradually from cores towards rims, whereas those in the EAV‐hosted rutile are nearly invariable. Furthermore, the vein rutile shows Nb/Ta zoning patterns that are complementary to those in rutile from their immediate hosts (ECVs), suggesting an internal origin for the vein‐forming fluids. The Nb/Ta ratios of such fluids evolved from low values at the early stage of subduction to higher values at later supercritical conditions with increased temperature and pressure. Quantitative modelling was conducted to constrain the compositional evolution of metamorphic fluids during dehydration and fluid‐rock interaction focusing on Nb–Ta distribution. The modelling results based on our proposed multistage fluid phase evolution path can essentially reproduce the natural observations reported in the present study. 相似文献
5.
对云南因民铁铜矿区深部辉长岩类中金红石、黑云母、碳酸盐和绿泥石的矿物地球化学特征进行研究,以探讨赋存于辉长岩类中的铁氧化物铜金型矿(化)体的成岩成矿环境。金红石由岩浆结晶和多期蚀变作用形成,其结晶温度为820~1 082 ℃,多期蚀变温度为444~730 ℃,金红石与黑云母密切共生;黑云母可划分为原生高钛镁质黑云母、热液蚀变镁质黑云母和铁质黑云母,形成温度分别为653~750 ℃、525~619 ℃和551~577 ℃,氧逸度均位于Ni NiO缓冲剂附近,表明黑云母形成于高温强氧化环境,有利于金红石化;铁白云石-菱铁矿化揭示了强还原环境,交代蚀变金红石;绿泥石多由铁镁矿物蚀变形成,形成于中低温(174~243 ℃)、低氧逸度(-4468~-5142)和高硫逸度(-1442~-1976)的强还原环境,有利于金属硫化物形成。本区岩浆结晶演化和黑云母-金红石化蚀变具有高温强氧化地球化学岩相学特征,有利于钛、铁矿化,后期叠加中低温强还原地球化学岩相,为IOCG矿床成矿的有利地球化学岩相学类型。 相似文献
6.
藏南色如朗金红石矿床地质特征及控矿条件 总被引:1,自引:1,他引:0
藏南色如朗金红石矿床位于米拉山口断裂带东段北缘,矿床的赋矿岩石主要为绿片岩。由北向南圈定了3个矿体,矿体沿北东方向延伸,呈层状、似层状产出。矿石矿物以金红石为主,其他金属矿物有磁铁矿、赤铁矿、黄铁矿、黄铜矿、磁黄铁矿等。金红石主要为红褐色,少数为暗红褐色,呈自形-半自形柱状和他形粒状,粒径多为0.01~0.2mm,大者可达1~2mm。该矿床的形成主要受地层和变质作用控制,后期构造对矿床形态有一定的破坏作用。通过与中国典型金红石矿床地质特征对比,初步认为色如朗金红石矿床的成因类型为中低压变质型。 相似文献
7.
羊蹄子山-磨石山钛矿床的钛矿物主要为锐钛矿、金红石和钛铁矿。锐钛矿化学成分的特点是FeO含量明显比金红石要低;主要X光粉晶谱线为3.518(100)、2.377(14)和1.667(11);晶胞参数a()=3.786,c()=9.513;拉曼光谱谱线(cm-1)为516、395、195和143。金红石的主要X光粉晶谱线为3.250(100)、1.688(40)和2.488(29);晶胞参数为a()=4.595,c()=2.962;拉曼光谱谱线(cm-1)为610和446。钛铁矿的成分特点是富锰贫镁,与攀西地区岩浆型钒钛磁铁矿矿床中的钛铁矿正好相反。所有上述钛(铁)氧化物矿物学特征,进一步说明该矿床是在中元古代在海底与基性火山活动有关的热水沉积后经区域变质和局部又遭受后期热液改造而成。 相似文献
8.
本矿床是我国金红石矿床重要的成因及工业类型,为具有特定化学成分的岩石在特定变质条件下形成的。本文通过对大量数据的处理,查明了化学成分与成矿的关系:高Al2O3、MgO、Fe2O3+FeO、K2O、P2O5、H2O+、MnO,低SiO2、CaO、Na2O、CO2、S等,利于钛富集;高TiO2、MgO、P2O5、S,低SiO2、CaO、K2O、Al2O3、Fe2O3/FeO,利于金红石形成;高Sc、Zr、Ni、Zn及La/Yb,低Y、Nb、Th、Cd、Ba、Be、ΣREE,利于金红石纯度提高。对研究矿床成因及寻找新的同类矿床等有重要意义 相似文献
9.
Caledonian high-pressure metamorphism in the Strona-Ceneri Zone (Southern Alps of southern Switzerland and northern Italy) 总被引:3,自引:0,他引:3
The Strona-Ceneri Zone comprises a succession of polymetamorphic, pre-Alpidic basement rocks including ortho- and paragneisses,
metasedimentary schists, amphibolites, and eclogites. The rock pile represents a Late Proterozoic or Palaeozoic subduction
accretion complex that was intruded by Ordovician granitoids. Eclogites, which occur as lenses within the ortho-paragneiss
succession and as xenoliths within the granitoids record a subduction related high-pressure event (D1) with peak metamorphic
conditions of 710 ± 30 °C at 21.0 ± 2.5 kbar. After isothermal uplift, the eclogites experienced a Barrowtype (D2) tectonometamorphic
overprint under amphibolite facies conditions (570-630 °C, 7-9 kbar). U-Pb dating on zircon of the eclogites gives a metamorphic
age of 457 ± 5 Ma, and syn-eclogite facies rutile gives a 206Pb/238U age of 443 ± 19 Ma classifying the subduction as a Caledonian event. These data show that the main tectonometamorphic evolution
of the Strona-Ceneri Zone most probably took place in a convergent margin scenario, in which accretion, eclogitization of
MOR-basalt, polyphase (D1 and D2) deformation, anatexis and magmatism all occurred during the Ordovician. Caledonian high-pressure
metamorphism, subsequent magmatism and Barrow-type metamorphism are believed to be related to subduction and collision within
the northern margin of Gondwana.
Editorial handling: Edwin Gnos 相似文献
10.