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1.
The Channagiri Mafic-Ultramafic Complex occupies lowermost section of the Neoarchaean Shimoga supracrustal group in the Western Dharwar Craton. It is a segmented body occupying the interdomal troughs of granitoids. The magnetite deposits occur in the northeastern portion; typically occupying the interface zone between gabbro and anorthositic. Mineralogically, the deposits are simple with abundant magnetite and ilmenite. Hogbomite is a consistent minor mineral. Magnetites are typically vanadiferous (0.7–1.25% V2O5). Ilmenite consistently analyses more MgO and MnO than coexisting magnetite. Chlorite, almost the only silicate present; lies in the range of ripidolite, corundophilite and sheridanite. The chromiferous suit occupying eastern side of Hanumalapur block (HPB) contains Fe-Cr-oxide analysing 37.8–11.9% Cr2O3 and 40.5–80% FeO t . In these too, chlorite, typically chromiferous (0.6–1.2% Cr2O3), is the most dominant silicate mineral. Geochemistry of V-Ti-magnetite is dominated by Fe, Ti and V with Al, Si, Mg and Mn contributing most of the remaining. Cr, Ni, Zn, Co, Cu, Ga and Sc dominate trace element geochemistry. The Cr-magnetite is high in Cr2O3 and PGE. Two separate cycles of mafic magmatism are distinguished in the CMUC. The first phase of first cycle, viz., melagabbro-gabbro, emplaced in the southeastern portion, is devoid of magnetite deposits. The second phase, an evolved ferrogabbroic magma emplaced in differentiated pulses, occupying northeastern portion of the complex, consists of melagabbro→gabbro-anorthosite→V-Ti magnetite→ferrogabbro sequence. Increase in oxygen fugacity facilitated deposition of V-Ti magnetite from ferrogabbroic magma pulse emplaced in late stages. The second cycle of chromiferous PGE mineralized suite comprises fine-grained ultramafite→alternation of pyroxinite-picrite→Crmagnetite sequence formed from fractionation of ferropicritic magma. HPB also includes >65m thick sill-like dioritic phase at the base of the ferriferous suit and a sinuous band of coarse-grained ultramafite enclosed within the chromiferous suit; both unrelated to the two mafic magmatic cycles.  相似文献   

2.
产于层状镁铁质-超镁铁质岩体中的太和岩浆型Fe-Ti氧化物矿床是峨眉山大火成岩省内带几个超大型Fe-Ti氧化物矿床之一。太和岩体长超过3km,宽2km,厚约1.2km。根据矿物含量和结构等特征,整个岩体从下向上可划分为下部岩相带、中部岩相带、上部岩相带。下部岩相带主要以(橄榄)辉长岩和厚层不含磷灰石的块状Fe-Ti氧化物矿层组成。中部岩相带韵律旋回发育,(磷灰石)磁铁辉石岩主要位于旋回的底部,旋回上部为(磷灰石)辉长岩。上部岩相带主要是贫Fe-Ti氧化物的磷灰石辉长岩。太和中部岩相带磷灰石磁铁辉石岩含有5%~12%磷灰石、20%~35%Fe-Ti氧化物、50%~60%硅酸盐矿物,且硅酸盐矿物与磷灰石呈堆积结构。磷灰石磁铁辉石岩中磁铁矿显示高TiO2、FeO、MnO、MgO,且变化范围与趋势接近于攀枝花岩体。钛铁矿FeO分别与TiO2、MgO显示负相关,而FeO分别与Fe2O3、MnO显示正的相关,且TiO2、FeO、MnO、MgO含量变化较大,这些特征都暗示磁铁矿和钛铁矿是从富Fe-Ti-P岩浆中分离结晶。因此,可以推断太和磷灰石磁铁矿辉石岩形成于矿物重力分选和堆积。太和下部岩相带包裹在橄榄石中磁铁矿含有相对较高Cr2O3(0.07%~0.21%),而中部岩相带包裹在橄榄石中磁铁矿Cr2O3(0.00%~0.03%)显著降低,且这些磁铁矿Cr2O3含量变化与单斜辉石Cr含量和斜长石An牌号呈正相关。这些特征印证了形成中部岩相带的相对演化的富Fe-Ti-P母岩浆可能是源自中部岩浆房的混合岩浆。上部岩相带磁铁矿和中部岩相带顶部少量磁铁矿显示较低Ti+V可能是由于岩浆房中累积的岩浆热液对磁铁矿成分进行了改造。  相似文献   

3.
《Applied Geochemistry》2002,17(7):885-902
An ancient saprolite has developed on the Palaeoproterozoic granulite, granite gneiss and amphibolite bedrock of the Vuotso–Tankavaara area of central Finnish Lapland. The present day climatic regime in Finnish Lapland lies within the northern boreal zone and so the saprolite there can be regarded as fossil. Cores of saprolite were collected from 4 sections (42 samples) and analyzed chemically and mineralogically. In the study area, progressive weathering of the rocks has been marked by gradual enrichment in Al, Fe and Ti; and depletion of Na, K and Ca. The higher concentration of Fe(III) and water and reduced Na and Ca in weathered bedrock in the 4 sections are indicative of oxidation, hydration and leaching processes involved during weathering. The primary minerals in the saprolite are plagioclase feldspar, K-feldspar, quartz, garnet (almandine) and hornblende; the common secondary minerals are kaolinite, halloysite, and vermiculite in addition to minor amounts of sericite. Intense weathering is indicated by: (1) the presence of kaolinite and halloysite in 4 sections of different bedrock types, and (2) the comparatively lower SiO2/Al2O3 (wt.%) ratio (2.30) of weathered granulites (3 sections) as compared to fresh granulite (4.33) and that of weathered amphibolite (2.68) as compared to fresh amphibolite (3.56). In general, kaolinite and halloysite have formed through the weathering of feldspars, garnet, and biotite. Vermiculite is the most probable alteration product of biotite. The formation of kaolinite and halloysite in Finnish Lapland indicates wetter and warmer climatic conditions during the time of their formation than at present. The possible time for formation of the saprolite is early Cretaceous–early Tertiary into Middle Miocene.  相似文献   

4.
徐则民  黄润秋 《中国地质》2013,40(6):1942-1948
提要:岩石化学风化程度评价指标应该同时满足以下三个基本条件,即与风化程度之间的关系简单明确、对风化程度变化具有足够的敏感性和易于确定和不易受到人为因素影响。作为铁镁质岩石的主要代表,(峨眉山)玄武岩风化程度评价除考虑可引起组分淋失与富集的水解反应外,还应充分考虑二价铁的氧化反应。新鲜峨眉山玄武岩中并存的二价铁和三价铁的含量总体稳定,910个样品的FeO、Fe2O3平均含量分别为8.45%和5.15%,以均匀、随机的方式赋存于辉石、橄榄石、杏仁体中的绿泥石、磁铁矿及火山玻璃中。风化玄武岩、玄武岩斜坡地下水及新鲜玄武岩浸泡液的地球化学研究结果表明,FeO及Fe2O3含量对峨眉山玄武岩风化程度的敏感性明显高于其他组分,同时铁又是玄武岩风化过程中活动性最差的元素之一。三价铁和二价铁的摩尔数比值(FF)适合于峨眉山玄武岩整个风化过程的风化程度判别,比既有风化指数具有更高的分辨率,尤其是对风化初期玄武岩。  相似文献   

5.
This work presents new field and petrological data on a poorly known lower crustal section from the Alpine Jurassic ophiolites, the Pineto gabbroic sequence from Corsica (France). The Pineto gabbroic sequence is estimated to be ~1.5 km thick and mainly consists of clinopyroxene-rich gabbros to gabbronorites near its stratigraphic top and of troctolites and minor olivine gabbros in its deeper sector. The sequence also encloses olivine-rich troctolite and mantle peridotite bodies at different stratigraphic heights. The composition and the lithological variability of the Pineto gabbroic sequence recall those of the lower crustal sections at slow- and ultra-slow-spreading ridges. The gabbroic sequence considered in this study is distinct in the high proportion of troctolites and olivine gabbros, which approximately constitute 2/3 of the section. In particular, the lower sector of the Pineto gabbroic sequence shows the existence of large-scale fragments of the deepest oceanic crust displaying a highly primitive bulk composition. The mineral chemical variations document that the origin and the evolution of the Pineto gabbroic rocks were mostly constrained by a process of fractional crystallisation. The clinopyroxenes from the olivine gabbros and the olivine-rich troctolites also record the infiltration of olivine-dissolving, Cr2O3-rich melts that presumably formed within the mantle, into replacive dunite bodies. Cooling rates of the troctolites and the olivine gabbros were evaluated using the Ca in olivine geospeedometer. We obtained high and nearly constant values of ?2.2 to ?1.7 °C/year log units, which were correlated with the building of the Pineto gabbroic sequence through multiple gabbroic intrusions intruded into a cold lithospheric mantle.  相似文献   

6.
The mineralogy and geochemistry of the massive pyrite-pyrrhotite mineralization, which contains minor magnetite, sphalerite and galena, the weathered profile and surface gossan at Mugga Mugga in Western Australia have been examined. Reactions between amphibolite wall rocks and acid waters from the oxidation of the iron sulfides have resulted in distinct mineralogical zonation of the weathered profile which is further modified near the surface by lateritization. At the base of the weathered zone an opaline chert (Opal-CT) has been precipitated from fluctuations of the water table. A gossanous zone from 25.14–68.80 m with boxworks after massive pyrite is modified by abundant kaolinite, dickite and an alunite-type mineral derived from amphibolite wall rocks, while above 25.14 m both plinthite and mottled clay zones of a laterite profile are evident. Some characteristics of a mature gossan profile – sulfate-phosphate-arsenate near the base, a carbonate zone higher in the profile, and an oxide zone near the surface – overprint the gross zonation.At the interface between sulfide and weathered rock Mg, Ca, K, S, Zn, Cd, Hg, Ba are depleted, As, Sb, Mo, Cr and V contents increase and in the weathered zone, SiO2, TiO2, P2O5, SO3, Pb, Zn, Hg, Sb, Co, Ni, W, Ba, Sr and Zr decrease up the profile whilst Al2O3, Fe2O3, CO2, Cu and As increase. Of the elements associated with the massive pyrite (Pb, Zn, Cu, Ag, As, Cd, Hg, Sb, Co, Ni) anomalous concentrations of Pb, Cu, Ag, As and Sb occur in the surface gossan despite the possibility of complete leaching by highly acidic solutions. These anomalies are similar to those found in gossans over pyrite mineralization elsewhere in the Yilgarn Block.  相似文献   

7.
Some of the most vanadium-rich silicate minerals known are present in green mica schist from the Hemlo gold deposit, Ontario, Canada. Vanadium-rich silicate minerals include green mica (up to 17.6 wt. % V2O3), phlogopite (10.1 wt. % V2O3), pumpellyite (25.7 wt. % V2O3), garnet (18.5 wt. % V2O3), epidote-group minerals (9.1 wt. % V2O3), antimonian vesuvianite (4.3 wt. % V2O3), and titanite (18.5 wt. % V2O5). In addition, minor amounts of V (<2 wt. % V2O3) are present in tourmaline, chlorite, talc and tremolite in other lithologies of the Hemlo deposit. The principal substitution that incorporates V into most of these silicate minerals is Al3+=V3+ in octahedral positions. Vanadium is incorporated into phlogopite mainly by the two substitutions: 3Mg2+ =2V3++ and VIMg2++IVSi4+=VIV3+ +IVAl3+, and all of the three substitutions Ti4++O2- =V3++(OH,F)-, Ti4+=V4+, and 5Ti4+=4V5+ + may have operated in titanite.Vanadium-enriched green mica schist from the Hemlo gold deposit is characterized by uniform Ti/Zr ratios, systematically low Ti, Ni, Co and Sc abundances, and low levels of incompatible elements Th, U, Hf and Zr and is distinct in these respects from its Cr-enriched counterpart. These geochemical features, along with textural evidence (relict quartz and oligoclase phenocrysts), indicate that the V-enriched green mica schist from Hemlo was most likely derived mainly from quartz-oligoclase porphyry. However, its anomalously high V and Cr contents were probably introduced metasomatically from local maficultramafic sources and were fixed in green mica and oxides during the waning of a second regional metamorphism. Vanadium was further remobilized, and its concentration probably enhanced, during the late hydrothermal alteration, which resulted in the formation of the characteristic V-rich calc-silicate minerals.  相似文献   

8.
Major element, Rb, Sr and Sr isotope abundances were examined in an ancient (Cambrian) weathering zone in the Butler Hill Granite, Missouri. Most of the major elements behaved predictably and systematically as a result of weathering intensity. MgO and the alkalis (Na2O and K2O) show highly erratic variations in both fresh and weathered rocks, suggesting considerable initial heterogeneity in the composition of biotite and feldspar. Rb predictably follows the behaviour of K during weathering (showing erratic variations similar to K), whereas Sr follows Ca (decreasing steadily as a result of weathering intensity). A method is postulated to date ancient weathering episodes using Rb-Sr data from a sequence of fresh to highly weathered samples. Data from the Butler Hill Granite (1185 m.y.) lend support to the proposed dating technique but show that more detailed sampling of the most intensely weathered regions is needed to produce more accurate results in future studies.  相似文献   

9.
磁铁矿中磁性物成分的测定及可选性评价   总被引:3,自引:3,他引:0  
对磁铁矿样品分别用磁选管和手工内磁选法进行磁选,并对原矿样品和样品的磁性物中TFe、P、S、V2O5、TiO2、SiO2、Al2O3、CaO、MgO、Sn、Cu、Pb、Zn的含量进行测定.分析结果表明,采用手工内磁选和磁选管对磁铁矿进行磁选所得的结果一致,为了简便操作,本文均采用手工内磁选法选出磁性物.A矿区磁性铁(mFe)含量(22.42%)比B矿区mFe含量(22.59%)低,但A矿区样品的磁性物中TFe含量(磁铁精矿品位)大于66%,比B矿区样品的磁性物中TFe含量(小于57%)高,A矿区的磁铁矿选矿效果明显好于B矿区,说明对磁性物中TFe含量的测定能够更好地反映矿石的可选性.原矿样品中P、S的含量分别为0.328%、0.271%,而样品的磁性物中P、S的含量为0.021%、<0.005%,均达到铁矿石冶炼标准;原矿样品中V2O5、TiO2的含量分别为0.156%、1.37%,而样品的磁性物中V2O5、TiO2含量分别为0.823%、13.62%,达到了铁矿石冶炼标准.原矿样品的(CaO+MgO)/(SiO2 +Al2O3)值为0.876,为自熔性矿石,而其磁性物的(CaO+ MgO)/(SiO2+Al2O3)值为0.453,为酸性矿石.由此说明,单纯测定原矿样品中的各成分尚不能对磁铁矿的可选性进行科学性评价,只有进一步测定磁铁矿的磁性物中各成分的含量,才能够对磁铁矿进行可靠的评价.本文通过对磁铁矿中磁性物成分的测定,为磁铁矿的选冶性能提供了新的评价方法.  相似文献   

10.
白水黄土-红粘土化学风化强度的剖面特征与粒度效应   总被引:16,自引:11,他引:5       下载免费PDF全文
白水剖面黄土-红粘土全样化学分析表明,以CIA指数为代表的化学风化强度从剖面下部往上逐步变弱,波动增大,总体趋势与深海氧同位素代表的全球冰量变化可以很好对比。分粒级组分化学分析则显示,黄土-红粘土主要元素迁移及化学风化强度与粒度强烈相关,CIA指数表征的化学风化强度变化在相当程度上受到粒度变化的控制。总体上,黄土-红粘土各粒级颗粒的风化程度都不高,而且沉积之后的成土风化作用对其主要元素含量的影响有限,黄土-红粘土化学成分的长期变化趋势主要受到物源的新加入和混合过程的影响。从剖面变化看,粗粒级部分(5~20μm和20~63μm)的风化指数的变化特征与细粒级部分(<5μm)不完全相同,表明不同粒级组分接受化学风化以及在物源区停留的历史不尽相同。1Ma以来,各粒级CIA指数都整体降低,显示物源区新鲜、弱风化碎屑影响到各粒级颗粒的混合过程。进一步对细粒级部分(<5μm)化学成分演化进行的分析显示,其元素含量呈现不同组分递次变化的"序列模式",从红粘土下部(约4.5Ma)到黄土上部(约0.6Ma),K2O/Al2O3,Na2O/Al2O3,CaO/Al2O3和MgO/Al2O3比率的变化依次出现转折,这很可能与晚新生代黄土-红粘土物源区构造抬升、冰川剥蚀能力不断加大,使得新鲜基岩不断被剥蚀、去顶,由此造成主要造岩矿物顺序剥蚀、接受风化,成为粉尘新物源有关。  相似文献   

11.
Elongated NE-SW trending bodies of iron-rich rock are exposed adjacent to pyroxenite dyke within Sukinda ultramafic complex, Odisha. Field study followed by optical and electron microscopy, XRD and EPMA investigation reveal the rocks to be fine grained, weathered, limonitised; containing quartz, magnetite, hematite/martite and goethite. The rock has suffered from deformation during intrusion of chromiferous magma. It rarely shows banding/lamination, but largely exhibits mylonitic fabric, resulting from magmatic intrusion. The stronger deformation is evident from sub-grain formation, deformed mineral grains; often with orientation, stretching (boudinage) and shortening (folding); presence of porphyroclasts, pull-apart structure, undulose extinction, dynamic recrystallisation etc. From the microstructure and mineral abundance, the rock is designated as “Mylonitic Magentite Quartzite” (MMQ).Enrichment of some elements like Ni, Mg, Cr in the magnetite phase of MMQ is attributed to solid state diffusion of these elements from chromiferous mafic magma during thermal metamorphism. This is determined from electron probe microanalysis of iron-rich phase in MMQ, which is found to contain 88-90 wt% of FeO(t) with ~1%, NiO, ~1%, MgO and 0.1% Cr2O3 having around 3 mole% of trevorite; 4-6% of magnesioferrite; 0.15-0.3% of chromite; 86-87% of magnetite and 3-4% of wustite. Considering presence of wustite as temperature indicator, the temperature of magma envisaged to be around 950-1100°C.In a later period, the MMQ has undergone oxidation and lateritisation owing to its prolonged exposure. During this process, new minerals like hematite and goethite substituted magnetite, resulting leaching of iron (FeO: 62-68%) and magnesium (MgO: 0.1-0.35) and enrichment of chromium (Cr2O3:4-7%) and nickel (NiO: 1.6-2.3%). The silica (SiO2: 4-5%), alumina (Al2O3:~1%) are contributed by kaolinite, formed during lateritisation.The field and laboratory studies confirm these iron-rich exposures to be enclaves of BIFs, banded magnetite quartzite (BMQ) in particular, within the Sukinda chromiferous ultramafic complex. Micro-structural features and microchemical composition of iron minerals in these exposures are interpreted as the influence of forceful ultramafic intrusion into the existing BMQ and effect of thermal metamorphism followed by oxidation, weathering/lateritisation.  相似文献   

12.
Analysis by optical, X-ray diffraction and microprobe methods, of essentially unzoned, disseminated spinels within cumulus picrites and olivine gabbros reveals an unbroken range of compositions from aluminian chromite (34% Cr2O3) to chromian magnetite (4% Cr2O3). TiO2 contents vary between 0.5 and 7.7%. Exsolution of ilmenite indicates originally higher TiO2 contents. Quenched contact-facies rocks with abundant olivine phenocrysts contain strongly zoned spinels in which a titaniferous chromian magnetite rim (16% Cr2O3, 10% TiO2) encloses cores of weakly titanian chromite (40% Cr2O3). Platy dendrites of exsolved spinel occur in abundance within cumulus olivines. The evidence suggests that crystallization of the disseminated spinels occurred under the influence of an increase in oxygen fugacity towards the interior of the intrusion, and that the compositional diversity has stemmed from the homogenization of originally zoned grains mantled to varying degrees by high-Ti, low-Cr rims.  相似文献   

13.
The ~2,752-Ma Weld Range greenstone belt in the Yilgarn Craton of Western Australia hosts several Fe ore deposits that provide insights into the role of early hypogene fluids in the formation of high-grade (>55 wt% Fe) magnetite-rich ore in banded iron formation (BIF). The 1.5-km-long Beebyn orebody comprises a series of steeply dipping, discontinuous, <50-m-thick lenses of magnetite–(martite)-rich ore zones in BIF that extend from surface to vertical depths of at least 250 m. The ore zones are enveloped by a 3-km-long, 150-m-wide outer halo of hypogene siderite and ferroan dolomite in BIF and mafic igneous country rocks. Ferroan chlorite characterises 20-m-wide proximal alteration zones in mafic country rocks. The magnetite-rich Beebyn orebody is primarily the product of hypogene fluids that circulated through reverse shear zones during the formation of an Archean isoclinal fold-and-thrust belt. Two discrete stages of hypogene fluid flow caused the pseudomorphic replacement of silica-rich bands in BIF by Stage 1 siderite and magnetite and later by Stage 2 ferroan dolomite. The resulting carbonate-altered BIF is markedly depleted in SiO2 and enriched in CaO, MgO, LOI, P2O5 and Fe2O3(total) compared with the least-altered BIF. Subsequent reactivation of these shear zones and circulation of hypogene fluids resulted in the leaching of existing hypogene carbonate minerals and the concentration of residual magnetite-rich bands. These Stage 3 magnetite-rich ore zones are depleted in SiO2 and enriched in K2O, CaO, MgO, P2O5 and Fe2O3(total) relative to the least-altered BIF. Proximal wall rock hypogene alteration zones in mafic igneous country rocks (up to 20 m from the BIF contact) are depleted in SiO2, CaO, Na2O, and K2O and are enriched in Fe2O3(total), MgO and P2O5 compared with distal zones. Recent supergene alteration affects all rocks within about 100 m below the present surface, disturbing hypogene mineral and the geochemical zonation patterns associated with magnetite-rich ore zones. The key vectors for identifying hypogene magnetite-rich Fe ore in weathered outcrop include textural changes in BIF (from thickly to thinly banded), crenulated bands and collapse breccias that indicate volume reduction. Useful indicators of hypogene ore in less weathered rocks include an outer carbonate–magnetite alteration halo in BIF and ferroan chlorite in mafic country rocks.  相似文献   

14.
The geochemistry of major and trace elements (including heavy metals and rare earth elements) of the fresh and weathered black shales, and the soils derived from black shales in the Ganziping mine area in western Hunan province (China) were studied using the following techniques: X-ray fluorescence (XRF), inductively coupled plasma mass spectrometer (ICP-MS) and X-ray diffraction (XRD). The results show that the black-shale soils are significantly enriched with Al2O3 and Fe2O3, and depleted of mobile elements CaO, Na2O and K2O. The soils are also highly enriched with heavy metals U, V, Ni, Ba, Cu, Zn and Pb, that may cause potential heavy-metal contamination of the soils. Composition of the soils is homogeneous compared to the weathered black shales, for which the concentrations of major elements except CaO and Na2O, and trace elements except heavy metals (U, V, Ni, Ba, Cu, Zn and Pb) as well as the mobile Sr, show lower variations than in the weathered black shales. Ratios of Zr/Hf, Ta/Nb, Y/Ho, Nd/Sm, and Ti/(Ti + Zr), of the soils are also less variable, with values constantly similar to that of the fresh and weathered black shales correspondingly. Thus, components of the soils are believed to be contributed from the parent black shales through weathering and pedogenesis. It is concluded that the soils were formed by at least two stages of geochemical processes: the early stage of chemical differentiation and the later stage of chemical homogenization. The chemical differentiation that was taken during black-shale weathering might have caused the depletion of CaO and Na2O, and the enrichment of Al2O3 and Fe2O3; while the chemical homogenization that was taken during pedogenesis led to the depletion of SiO2 and K2O, and to the further enrichment of Al2O3 and Fe2O3. The heavy-metal enrichment (contamination) of the soils was then genetically related to the enrichment of Al2O3 and Fe2O3 in the soils.  相似文献   

15.
The mineralogy of the transported Fe-Ni-Cr-laterite ore bodies from the Edessa area in Northern Greece was studied. The special emphasis was on the textural features and chemistry of chromite. The chromite was residually inherited in laterites from weathered ultramafic rocks and it displays zonation. Three main zones were optically distinguished: an inner chromite zone, an intermediate ferritechromite zone and a magnetite rim. These three zones have distinct compositions. The major oxides MgO and Al2O3 decrease from the chromite core to the ferritechromite zone, while FeOt increases and Cr2O3 either increases or decreases. A characteristic chemical feature of the chromite is the very high Mn-content in the ferritechromite zone, up to 20%wt MnO. Chemical zonation has, however, been detected in optically unzoned chromite cores rimmed by magnetite.The zoning and the high Mn-content of the chromite is a result of serpentinization in the presence of Mn-rich fluids, following lateritic weathering and finally Alpine low-grade metamorphism.  相似文献   

16.
An intrabasaltic red bole horizon is studied for its weathering characteristics with respect to the underlying and overlying basalts. The study indicates that all the three units have been considerably weathered; the red bole unit, however shows some distinctive characteristics. The red boles show a higher cation exchange capacity (CEC) and lower sodium adsorption ratio (SAR) and organic carbon (OC) as compared to the weathered basalts. The lower values of Al2O3, TiO2 and Fe2O3(T) in red boles indicate their lesser weathering than the underlying and overlying basalts, which is further corroborated by the weathering intensity measured by the indices like chemical index of alteration (CIA) and statistical empirical index of chemical weathering (W). It is also evident that the red bole samples show more retention of original mafic and felsic components. While K2O exhibits an erratic behaviour, the MgO and CaO do not show much leaching in red boles. Lesser leaching and salinity in the red boles is indicated by the higher values of calcification and lower values of salinization. The SiO2–Al2O3–Fe2O3 plot indicates that red bole samples are close to the basalt field, while the weathered upper basalt is more kaolinized than the weathered lower basalt. These observations reveal that the post-formational weathering processes have least affected the original palaeoweathering characters of the red bole horizon and hence the intrabasaltic palaeosols (weathering horizons) can effectively be used to constrain the palaeoweathering and palaeoclimates during the continental flood basalt episodes in the geologic past.  相似文献   

17.
西天山哈拉达拉辉长岩的Fe-Ti富集机制及其构造意义   总被引:4,自引:4,他引:0  
贺鹏丽  黄小龙  李洪颜  李洁  于洋  李武显 《岩石学报》2013,29(10):3457-3472
特克斯哈拉达拉辉长岩体是西南天山出露规模最大的层状基性-超基性侵入杂岩体,其富含Fe-Ti氧化物(含量高达15%)。哈拉达拉辉长岩中的橄榄石具有较低的Fo值(64~75),斜长石主要为中-拉长石,单斜辉石相对低Mg#(0.66~0.87),属于次透辉石或普通辉石,总体上显示出较高的岩浆演化程度。Fe-Ti氧化物以钒钛磁铁矿为主(TiO2=0.8%~20.6%;V2O3=0.10%~0.83%),常与钛铁矿呈矿物对共生或出溶钛铁矿。晚期的云母矿物均围绕他形的Fe-Ti氧化物生长,主要为富MgO的金云母,少量属于黑云母;大部分云母成分富含F、Cl(F+Cl高达3.14%),指示岩浆形成于贫水环境。哈拉达拉辉长岩体的主量元素成分变化很大(Mg#=0.48~0.73),橄榄辉长岩主要受橄榄石和斜长石的结晶分异/堆晶作用影响,而辉长岩的成分变化主要受控于斜长石和Fe-Ti氧化物的堆晶作用。哈拉达拉岩体的Fe-Ti氧化物主要为岩浆正常结晶分异作用的结果,该体系具有较低氧逸度、贫水的特点,其地幔源区的熔融程度较高,可能是塔里木地幔柱在天山造山带这一构造薄弱带的早期岩浆活动。  相似文献   

18.
Al_2O_3和Ti在风化和热液蚀变等地球化学过程中通常被认为是不活动元素,两者的比值Al_2O_3/Ti常被用来指示地球化学作用过程。通过对中国157件火成岩样品元素含量平均值的统计发现,火成岩样品中Al_2O_3/Ti与SiO_2含量值之间存在着较好的幂函数关系:ln(Al_2O_3/Ti)=0.073×SiO_2-0.89,式中Al_2O_3和SiO_2和Ti含量单位均为%。本文基于得到的经验方程和TAS图解构建了一个新的判别岩石类型的图解——Al_2O_3-Ti图解。该图解可以区分酸性岩、中酸性岩、中性岩、中基性岩-基性岩四类岩性。通过对三个火成岩风化剖面的研究发现,花岗岩风化剖面从新鲜基岩到风化形成的土壤在Al_2O_3-Ti图解中均落在酸性岩区,花岗闪长岩风化剖面从新鲜基岩到风化形成的土壤样品均落在中酸性岩区,玄武质安山岩风化剖面从新鲜基岩到风化形成的土壤样品均落在中基性岩-基性岩区。不同风化程度的风化产物与其母岩在Al_2O_3-Ti图解中所在的区域一致,即Al_2O_3-Ti图解可以用来追溯火成岩风化产物的母岩岩性。通过对胶东焦家金矿和豫西牛头沟金矿两个矿区岩石的研究发现,黑云母花岗岩从新鲜岩石到其蚀变岩及其形成矿石的样品在Al_2O_3-Ti图解中均落在酸性岩区。玄武质安山岩从新鲜岩石到其蚀变岩及其形成矿石的样品在Al_2O_3-Ti图解中均落在中基性岩-基性岩区。即不同蚀变程度的蚀变产物与其原岩在Al_2O_3-Ti图解中所在的区域一致,这表明新构建的Al_2O_3-Ti图解可以用来示踪蚀变岩的原岩性质。  相似文献   

19.
西天山智博铁矿床磁铁矿成分特征及其矿床成因意义   总被引:12,自引:7,他引:5  
智博大型磁铁矿床位于新疆西天山阿吾拉勒成矿带东段,赋存于石炭系大哈拉军山组玄武质安山岩、安山岩及火山碎屑岩中。智博铁矿床包括东、中、西以及13号矿体4个矿段。矿体主要呈层状、似层状、透镜状。金属矿物以磁铁矿为主,含少量浸染状黄铁矿,局部可见细脉赤铁矿及零星状黄铜矿。矿石构造以块状和浸染状构造为主,角砾状次之,局部为条带状构造、脉状-网脉状构造;矿石结构包括半自形-他形粒状结构、交代残余结构、板条状结构。智博矿区的蚀变矿物组合以透辉石、钠长石、钾长石、绿帘石、阳起石为主,含有少量方解石、石英、绿泥石及榍石。根据矿物共生组合、矿石结构的观察以及矿物化学分析,识别出岩浆期和热液期2个成矿期,进一步细分为3个成矿阶段:磁铁矿-透辉石-绿帘石阶段(a1),磁铁矿-钾长石-绿帘石阶段(b1),石英-硫化物阶段(b2)。磁铁矿的电子探针成分分析显示,岩浆期矿石中FeOT含量较高,而Al2O3、CaO、MgO、SiO2等氧化物含量较低,热液期矿石则相反。角砾状和部分浸染状磁铁矿中V2O5含量相对较高,与火山岩中含量类似,暗示该矿化阶段的铁质部分来源于围岩;块状以及浸染状磁铁矿FeOT含量大部分在90%以上;角砾状、网脉状、树枝状矿石中磁铁矿的w(FeOT)分布相对比较集中,多数在90%~92%之间;纹层状矿石的w(FeOT)则变化于88%~92%之间,其CaO、SiO2等氧化物平均含量相对增加。TiO2-Al2O3-MgO图解和Ca+Al+Mn vs Ti+V图解均表明智博铁矿床的形成与火山活动和岩浆热液的交代作用有关。  相似文献   

20.
In this study, an assessment of the lithogenic concentrations of trace metals in soils and saprolite over basement rock units in Ibadan, SW-Nigeria is presented in respect of bedrock types and geochemical controls on the weathering-associated release of trace metals. Consequently, soil, weathered and fresh rock samples from the Precambrian Basement of SW Nigeria were collected from three different bedrock units within Ibadan metropolis and subjected to mineralogical and geochemical analyses. The analytical results revealed major proportions of oxides in the range of 18–20% Al2O3, 2–6% Na2O and 1–6% K2O for weathered profiles over granite-gneiss and pegmatite units, compared to 2–3% Al2O3, <0.5% Na2O and <1.0% K2O over schist-quartzite. For the trace elements, weathered profiles on granite-gneiss and schist-quartzite settings exhibit similar enrichment trends (enrichment factor, EF l) for most of the trace elements, unlike the pegmatite bedrock. However, enrichments are relatively greater in the top soil unit compared to the intermediate saprolite unit, especially for Pb, Ni, Zn, Cr, Co, Rb, Sr and Ba, a situation attributed to leaching and redistribution within the weathered profiles through pedogenetic process and percolating groundwater.Furthermore, the estimated weathering indices using Ruxton Ratio (RR = {SiO2/Al2O3}) and Chemical Index of Alteration (CIA = 100{Al2O3/[Al2O3 + CaO + Na2O + K2O]}) revealed RR of 2.9–3.7 and CIA of 54–73% for granite-gneiss and pegmatite units, implying medium levels of weathering, compared to RR of 30.8–35.5 and CIA of >60% for schist-quartzite units, which suggest weak chemical weathering. Also, the estimated high percentage loss, especially for Pb, Rb, Sr, Ba relative to the bedrocks, shows that the trace elements can be mobilized within the weathering profiles even at a low degree of chemical weathering. Such weathering-induced release of trace metals is of environmental significance as natural lithogenic input sources and as background reference for future monitoring of possible human/anthropogenic impacts.  相似文献   

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