X射线荧光光谱－点滴麦勒膜制片法测定金标准样品中金银铜锌

酸分解试样，点滴麦勒膜制片，Ｎｉ元素作内标，使用Ｘ射线荧光光谱法同时测定金银标准样品中Ａｕ、Ａｇ、Ｃｕ和Ｚｎ，分析范围为０．２％～１００％。对于Ａｕ、Ａｇ、Ｃｕ和Ｚｎ含量为８３％、８．Ｏ％、６．２％、３．０％的试样，其Ｒ８Ｄ（ｎ＝６）分别为０．１％、１．１％、０．９％和１．１％。     

川西丹巴地区磨子沟金矿床金、银赋存状态及成因

磨子沟金矿床位于四川省丹巴县,大地构造位置位于扬子准地台西缘,松潘-甘孜造山带东缘,泥盆系危关组炭质千枚岩、板岩是主要的赋矿围岩。成矿过程分为沉积成矿期、热液成矿期和表生风化期,其中热液期是金的主要成矿期。通过显微镜观察,扫描电镜、电子探针成分分析,矿物晶体化学式计算等手段和方法,研究了矿床中Au、Ag的赋存状态和主要载金矿物的特征。金以裂隙金、包裹体金、粒间金为主,银主要以类质同像赋存于方铅矿和硫盐矿物中。载金矿物黄铁矿生物结构发育,表明生物成矿作用是金矿床形成过程中的重要作用。矿体受特定层位和断裂的控制,围岩蚀变强烈。 根据矿床产出的大地构造环境、赋矿围岩特征、构造控矿、层位控矿、矿物共生特点等分析结果,丹巴磨子沟金矿床为沉积-热液改造型金矿床。     

Gold Deposits of the Yenisei Ridge (Russia) and Age of Its Formation

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Eclogites from the Obnazhennaya Kimberlite Pipe,Yakutia, Russia

Mineralogy and petrography of six eelogite xenoliths from the Obnazhennaya kimberlite pipe ar e described. Based upon modal and mineral compositions, these eclogites can be divided into Group A (five samples) and Group B (one sample), as per Coleman et al. (1965) and Shervais et al. (1988). Group-A eclogites are orthopyroxene-bearing, and their constituent minerals have high Mg# and Cr₂O₃ content. The clinopyroxenes in this type of eelogite have low jadeite component. The geochemical features of Group-A eclogites are similar to garnet pyroxenite, and e believed to be the product of high-pressure fractionates from an alkaline basaltic melt in thear upper mantle. Group-B eelogite (0-82/91) contains higher Al₂O₃ and FeO and lower MgO and Cr₂O₃; its composition is similar to a high-aluminum basalt or gabbro. This eelogite could have crystallized under high pressure in the upper mantle from a basaltic melt, without significant fractionation. Alternatively, it also could be the relict of subducted oceanic crust. However, no evidence exists at present that definitively indicates a crustal origin for this Group-B eelogite xenolith.     

Petrography and geochemistry of eclogites from the Mir kimberlite,Yakutia, Russia

 Diamond-bearing eclogites are an important component of the xenoliths that occur in the Mir kimberlite, Siberian platform, Russia. We have studied 16 of these eclogite xenoliths, which are characterized by coarse-grained, equigranular garnet and omphacite. On the basis of compositional variations in garnet and clinopyroxene, this suite of eclogites can be divided into at least two groups: a high-Ca group and a low-Ca group. The high-Ca group consists of high-Ca garnets in equilibrium with pyroxenes that have high Ca-ratios [Ca/(Ca+Fe+Mg)] and high jadeite contents. These high-Ca group samples have high modal% garnet, and garnet grains often are zoned. Garnet patches along rims and along amphibole- and phlogopite-filled veins have higher Mg and lower Ca contents compared to homogeneous cores. The low-Ca group consists of eclogites with low-Ca garnets in equilibrium with pyroxenes with a low Ca-ratio, but variable jadeite contents. These low-Ca group samples typically have low modal% of garnet, and garnets are rarely compositionally zoned. Three samples have mineralogic compositions and modes transitional to the high- and low-Ca groups. We have arbitrarily designated these samples as the intermediate-Ca group. The rare-earth-element (REE) contents of garnet and clinopyroxene have been determined by ion microprobe. Garnets from the low-Ca group have low LREE contents and typically have [Dy/Yb]_n < 1. The high-Ca group garnets have higher LREE contents and typically have [Dy/Yb]_n > 1. Garnets from the intermediate-Ca group have REE contents between the high- and low-Ca groups. Clinopyroxenes from the low-Ca group have convex-upward REE patterns with relatively high REE contents (ten times chondrite), whereas those from the high-Ca group have similar convex-upward shapes, but lower REE contents, approximately chondritic. Reconstructed bulk-rock REE patterns for the low-Ca group eclogites are relatively flat at approximately ten times chondrite. In contrast, the high-Ca group samples typically have LREE-depleted patterns and lower REE contents. The δ¹⁸O values measured for garnet separates range from 7.2 to 3.1‰. Although there is a broad overlap of δ¹⁸O between the low-Ca and high-Ca groups, the low-Ca group samples range from mantle-like to high δ¹⁸O values (4.9 to 7.2‰), and the high-Ca group garnets range from mantle-like to low δ¹⁸O values (5.3 to 3.1‰). The oxygen isotopic compositions of two of the five high-Ca group samples and four of the eight low-Ca group eclogites are consistent with seawater alteration of basaltic crust, with the low-Ca group eclogites representative of low-temperature alteration, and the high-Ca group samples representative of high-temperature hydrothermal seawater alteration. We interpret the differences between the low- and high-Ca group samples to be primarily a result of differences in the protoliths of these samples. The high-Ca group eclogites are interpreted to have protoliths similar to the mid to lower sections of an ophiolite complex. This section of oceanic crust would be dominated by rocks which have a significant cumulate component and would have experienced high-temperature seawater alteration. Such cumulate rocks probably would be LREE-depleted, and can be Ca-rich because of plagioclase or clinopyroxene accumulation. The protoliths of the low-Ca group eclogites are interpreted to be the upper section of an ophiolite complex. This section of oceanic crust would consist mainly of extrusive basalts that would have been altered by seawater at low temperatures. These basaltic lavas would probably have relatively flat REE patterns, as seen for the low-Ca group eclogites. Received: 10 July 1995 / Accepted: 17 May 1996     

Mineral inclusions in diamonds from the Sputnik kimberlite pipe, Yakutia

The Sputnik kimberlite pipe is a small “satellite” of the larger Mir pipe in central Yakutia (Sakha), Russia. Study of 38 large diamonds (0.7-4.9 carats) showed that nine contain inclusions of the eclogitic paragenesis, while the remainder contain inclusions of the peridotitic paragenesis, or of uncertain paragenesis. The peridotitic inclusion suite comprises olivine, enstatite, Cr-diopside, chromite, Cr-pyrope garnet (both lherzolitic and harzburgitic), ilmenite, Ni-rich sulfide and a Ti-Cr-Fe-Mg-Sr-K phase of the lindsleyite-mathiasite (LIMA) series. The eclogitic inclusion suite comprises omphacite, garnet, Ni-poor sulfide, phlogopite and rutile. Peridotitic ilmenite inclusions have high Mg, Cr and Ni contents and high Nb/Zr ratios; they may be related to metasomatic ilmenites known from peridotite xenoliths in kimberlite. Eclogitic phlogopite is intergrown with omphacite, coexists with garnet, and has an unusually high TiO₂ content. Comparison with inclusions in diamonds from Mir shows general similarities, but differences in details of trace-element patterns. Large compositional variations among inclusions of one phase (olivine, garnet, chromite) within single diamonds indicate that the chemical environment of diamond crystallisation changed rapidly relative to diamond growth rates in many cases. P-T conditions of formation were calculated from multiphase inclusions and from trace element geothermobarometry of single inclusions. The geotherm at the time of diamond formation was near a 35 mW/m² conductive model; that is indistinguishable from the Paleozoic geotherm derived by studies of xenoliths and concentrate minerals from Mir. A range of Ni temperatures between garnet inclusions in single diamonds from both Mir and Sputnik suggests that many of the diamonds grew during thermal events affecting a relatively narrow depth range of the lithosphere, within the diamond stability field. The minor differences between inclusions in Mir and Sputnik may reflect lateral heterogeneity in the upper mantle.     

北山成矿带霍勒扎德盖金矿床碲化物的发现及其地质意义

甘肃省霍勒扎德盖大型金矿床位于北山造山带的黑鹰山弧内,含金石英脉主要赋存在早石炭世英云闪长岩内的裂隙或断裂中。流体成矿过程从早到晚划分为Ⅰ、Ⅱ、Ⅲ三个阶段,分别形成(磁铁矿)-黄铁矿-石英脉、石英-多金属硫化物脉和石英-方解石脉。本次研究通过矿相学观察、扫描电镜/能谱及电子探针分析,在该矿床Ⅱ阶段矿石样品中首次发现大量碲化物,该矿物系列主要产出在黄铁矿、石英中或其裂隙内。矿区已发现的碲化物包括碲金矿、斜方碲金矿、针碲金银矿、碲金银矿、碲银矿、碲铅矿、碲汞矿、碲铋矿等;金银矿物仅以碲化物的形成存在。Ⅰ阶段流体的硫逸度(logfS2=-11.1~-9.5)较高、碲逸度(logf Te2≤-12.8)较低,Ⅱ阶段流体显示低硫逸度(logfS2=-13.5~-10.2)、高碲逸度(logfTe2=-11.1~-7.8)特征。碲化物的发现揭示了矿床与深部幔源的紧密联系,但同时不能排除矿区英云闪长岩提供成矿物质的可能。     

Gold and silver minerals in low-sulfidaton ores of the Julietta deposit (northeastern Russia)

Gold- and silver-containing pyrites of the Tikhii area at the Julietta deposit (Engteri ore cluster, Magadan Region) were studied by optical and scanning electron microscopy and electron probe microanalysis. One- or two-phase rounded microinclusions consisting of electrum (450-680%c) and/or galena or of petrovskaite and/or uytenbogaardtite, galena, and sphalerite have been found in early pyrites. Later As-pyrites (up to 2.6 wt.% As) contain multiphase xenomorphic microinclusions of acanthite, uytenbogaardtite, freibergite, argentotetrahedrite-tennantite, naumannite, petzite, selenopolybasite-selenostephanite, tellurocanfieldite, and other ore minerals localized in pores, cracks, and interstices. Pyrites that underwent hypergene alterations have rims and veinlets formed by acanthite, goethite, anglesite, plattnerite, and native silver. The presence of rounded ore mineral microinclusions and large pores in the early pyrites suggests the participation of volatiles in the mineral formation and the uptake of large amounts of impurities by pyrite under high-gradient crystallization conditions. The thermobarogeochemical studies of fluid inclusions in quartz have shown that the ore zone formed under boiling-up of hydrothermal medium-concentration NaCl solutions at 230-105 °C. The results of thermodynamic calculations evidence that Ag-Au-S-Se minerals formed under decrease in temperature and fugacity of sulfur (log₁Q/S₂ = -22 to -9) and selenium (log₁Q/S_e2 = -27 to -14) and change of reducing conditions by oxidizing ones in weakly acidic to near-neutral solutions.     

Cl-bearing lizardite in metamorphosed kimberlites from the Udachnaya Vostochnaya Pipe,Yakutia

Anhydrite-bearing dolomites and kimberlites from the contact zone of the Udachnaya Vostochnaya pipe, northern part of the Eastern Siberian Platform, were affected by low-grade metamorphism to the zeolite facies. The kimberlites are serpentinized and carbonatized and contain metasomes of anhydrite and saponite pockets. Twenty lizardite pseudomorphs after olivine (Fo _91–82) in the kimberlites were examined on an electron microprobe. The lizardite is rimmed by saponite and contains dolomite, calcite, magnetite, and anhydrite inclusions. Lizardite in the central parts of the pseudomorphs contains 1.5–1.9 wt % Cl and 6–9 wt % Fe₂O₃, and this mineral in the outer portions of the pseudomorphs bears 0.7–1.0 wt % Cl and 2–6 wt % Fe₂O₃ (the paper presents nine microprobe analyses and images showing the distribution of Cl, Mg, Al, Si, S, Ca, Ti, and Fe obtained in characteristic X-ray radiation). The amounts of Fe³⁺ in octahedrally and tetrahedrally coordinated sites of the Cl-bearing lizardite are roughly equal. Cl was borrowed in the course of serpentinization from the host Early Paleozoic evaporites and brines contained in them. The Cl concentration in our lizardite from the metamorphosed kimberlites from the Eastern Siberian Platform (continental lizardite) is much higher than the Cl concentration in oceanic lizardite from serpentine replacing peridotites (0.03–0.2 wt % Cl). This is likely explained by differences in the Cl concentrations in the metamorphic fluids, their salinity (3% for oceanic water and 65% for brines in the platform cover).     

Structure and sedimentary formations of the northern Yana-Kolyma Fold System, Yakutia

The structure, geodynamics, and sedimentary formations of the northern Yana-Kolyma Fold System and the adjacent part of the Verkhoyansk Fold System are considered on the basis of the published sheets of the State Geological Map on a Scale of 1: 200000, field observations of the authors, and literature sources. The important structure-forming role of the frontal uplift of the Kolyma-Omolon Superterrane that was thrust over in the northwestern direction is shown. The at-least-twofold shortening, thrust faulting, and large-scale offsets of the large blocks of the distal part of the Verkhoyansk continental margin and the Nagondzha paleotrough are related to this effect. An attempt is made to settle some debatable questions concerning the tectonic position of the Kular Uplift, the cause of the inconsistent structural patterns of the Jurassic and Triassic sequences at the southwestern margin of the Polousnyi Synclinorium, the counter vergence of folds in its northern and southern zones, the regional tectonic evolution in the Late Jurassic, and the eastward change in the composition of the heavy clastic mineral assemblages contained in the Upper Triassic and Jurassic rocks.     

Neoproterozoic Alkaline Igneous Rocks,Carbonatites and Gold Deposits of the Yenisei Ridge,Central Siberia: Evidence of Mantle Plume Activity and Late Collision Shear Tectonics Associated with Orogenic Gold Mineralization

This paper discusses the plausible genetic relationship between disseminated Au‐sulfide mineralization and mantle plume‐related magmatism in the context of the tectonic evolution of the Yenisei ridge in central Siberia. The relationship is inferred based on structural and geochemical studies of the Blagodat Au deposit, and the Transangara alkaline syenite and Penchenga fenite‐carbonatite complexes. Analyses of Nd, Sr and Ar isotopic compositions of samples from these geological features show their possible close temporal relationships but different sources. Nevertheless, the present data sets suggest that thermal effects of mantle plume activity likely controlled hydrothermal fluid mobilization in metamorphic suites and further enrichment of gold. The structural setting of the Blagodat Au deposit demonstrates the typical example of Au‐sulfide mineralization controlled by late collisional shear deformations. The present example of Au deposit associated temporally and spatially with carbonatites and alkaline rock complexes is an exclusive case in the Earth's history supporting a plausible genetic relationship between mantle plume‐related magmatism and orogenic‐Au mineralization.     

Olivine in the Udachnaya-East Kimberlite (Yakutia, Russia): Types, Compositions and Origins

Olivine is the principal mineral of kimberlite magmas, and isthe main contributor to the ultramafic composition of kimberliterocks. Olivine is partly or completely altered in common kimberlites,and thus unavailable for studies of the origin and evolutionof kimberlite magmas. The masking effects of alteration, commonin kimberlites worldwide, are overcome in this study of theexceptionally fresh diamondiferous kimberlites of the Udachnaya-Eastpipe from the Daldyn–Alakit province, Yakutia, northernSiberia. These serpentine-free kimberlites contain large amountsof olivine (50 vol.%) in a chloride–carbonate groundmass.Olivine is represented by two populations (olivine-I and groundmassolivine-II) differing in morphology, colour and grain size,and trapped mineral and melt inclusions. The large fragmentalolivine-I is compositionally variable in terms of major (Fo_85–94)and trace element concentrations, including H₂O content (10–136ppm). Multiple sources of olivine-I, such as convecting andlithospheric mantle, are suggested. The groundmass olivine-IIis recognized by smaller grain sizes and perfect crystallographicshapes that indicate crystallization during magma ascent andemplacement. However, a simple crystallization history for olivine-IIis complicated by complex zoning in terms of Fo values and traceelement contents. The cores of olivine-II are compositionallysimilar to olivine-I, which suggests a genetic link betweenthese two types of olivine. Olivine-I and olivine-II have oxygenisotope values (+ 5·6 ± 0·1 VSMOW, 1 SD)that are indistinguishable from one another, but higher thanvalues (+ 5·18 ± 0·28) in ‘typical’mantle olivine. These elevated values probably reflect equilibriumwith the Udachnaya carbonate melt at low temperatures and ¹⁸O-enrichedmantle source. The volumetrically significant rims of olivine-IIhave constant Fo values (89·0 ± 0·2 mol%),but variable trace element compositions. The uniform Fo compositionsof the rims imply an absence of fractionation of the melt'sFe²⁺/Mg, which is possible in the carbonatite melt–olivinesystem. The kimberlite melt is argued to have originated inthe mantle as a chloride–carbonate liquid, devoid of ‘ultramafic’or ‘basaltic’ aluminosilicate components, but becameolivine-laden and olivine-saturated by scavenging olivine crystalsfrom the pathway rocks and dissolving them en route to the surface.During emplacement the kimberlite magma changed progressivelytowards an original alkali-rich chloride–carbonate meltby extensively crystallizing groundmass olivine and gravitationalseparation of solids in the pipe. KEY WORDS: kimberlite; olivine; partial melting; carbonatitic melt; oxygen isotopes; H₂O     

Bonanza-grade accumulations of gold tellurides in the Early Cretaceous Sandaowanzi deposit,northeast China

The Sandaowanzi epithermal gold deposit (0.5 Moz or ca. 14 tons), located at the northern edge of the Great Xing'an range, NE China, is unique in that nearly all the gold (> 95%) is contained in gold tellurides mostly in bonanza grade ore shoots (the highest grade being up to 20,000 g/t). The bonanza ores are hosted in the central parts of large-scale (> 3 m wide, 200 m long) quartz veins which crosscut Early Cretaceous andesitic trachyte and trachytic andesite, and are, in turn, crosscut by diabase dykes of similar age. There are two ore types: low-grade disseminated ores and high-grade vein ores. In the former, very fine grains of Ag-rich tellurides (mainly hessite and petzite) coexist with sulfides (pyrite, sphalerite, galena and chalcopyrite), occurring as disseminated grains or sometimes as grain aggregates. In the high-grade vein ores, coarse-grained Au–(Ag)–tellurides (calaverite, sylvanite, krennerite, and petzite) form a major part of quartz–telluride veins. Chalcopyrite forms separate monomineralic veins emplaced within the quartz–telluride veins. Spectacular textures among coarse-grained (up to 3 cm in diameter) tellurides, and micron-scale bamboo shoot-like grains are observed. Two- and three-phase telluride symplectites are common in the vein ores.Fluid inclusion studies suggest that the mineralizing fluids are a mixture of magmatic and meteoric fluids, that homogenized in the temperature range of 260–280 °C. Sulfur isotope compositions of pyrite and chalcopyrite (δ³⁴S − 1.64 to 1.91‰) support the origin of fluids from a deep source. It is suggested that faulting, temperature changes and variation in fS₂ and fTe₂ were major factors contributing to the two main types of mineralization and the differences between them. Early rapid cooling and subsequent slow cooling of the later fluids along fault and fracture zones were instrumental in formation of the two superposed ore types. Open-space filling and crack-sealing along fractures predominates over replacement during telluride mineralization. The Sandaowanzi deposit is a unique bonanza-grade accumulation of gold tellurides genetically related to subalkaline magmatism, which was genetically associated with Early Cretaceous regional extension.     

Continental crust in the Lomonosov Ridge,Mendeleev Ridge,and the Makarov basin. The formation of deep-water basins in the Neogene

The northeast of the Russian Arctic is a deep-water basin underlain by the Lomonosov and Mendeleev Ridges, with the Makarov basin in between. In most of this area, the water depth is ~1–4 km and the crust is thick (20–30 km), with a well-pronounced granitic layer. Therefore, some researchers regard this crust as continental. Others think that this is the oceanic crust, the same as that on the hotspots like Iceland in the Atlantic or Ontong Java in the Pacific. After their activity stops, such structures must subside as a result of the crust and mantle cooling, in the same way as the oceanic crust on a spreading axis. As regards the Lomonosov and Mendeleev Ridges, they subsided in quite a different way. In the absence of volcanism, they remained near sea level, almost not subsiding, for a long time (at least 70 and 190 myr, respectively). Since the late Early Miocene, these areas subsided rapidly and deep-water sediments overlay shallow-water ones. In the same epoch, the Makarov basin subsided rapidly, which also used to lie near sea level. Its subsidence was several times that which could have taken place over the same period of time as a result of lithosphere cooling on an extinct hotspot. Such tectonic movements were possible only for the continental crust. The data on the structure of the sedimentary cover preclude considerable lithospheric stretching in these areas. Therefore, the rapid subsidence is accounted for by the transformation of gabbro in the lower crust into denser rocks (garnet granulites and eclogites), catalyzed by infiltration of a mantle-derived fluid flows. Dense, deeply metamorphosed mafic rocks with a thickness of up to 10–20 km and P-wave velocities of ~8 km/s underlie the Moho in the area under study.     

Gold Mineralization in Listvenite, the Sayi Gold Deposit, Xinjiang

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