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1.
Trace Elements and Sr, Nd Isotope Geochemistry of the Lajimiao Norite-Gabbro from the North Qinling Belt 总被引：1，自引：0，他引：1
S.R.Hart 《《地质学报》英文版》1994,68(2)
The Lajimiao norite-gabbro complex, as a part of the ophiolites on the southern side of the North Qinling belt, consists of gabbro and norite-gabbro. They were derived from different magma series: the gabbro was derived from tholeiitic magma series with higher TiO2, REE abundance and Fe3+/Fe2+ ratio ; norite-gabbro was derived from calc-alkali magma series with lower TiO2, Fe3+/Fe2+ ratio and REE abundance and much lower HREE abundance, which suggests that the source of the norite-gabbro magma was deeper and controlled by eclogite facies. Geochemical characteristics of both plutonic rocks are similar to those of island-arc basalts, such as relatively high contents of Ba, Pb and Sr and relatively low contents of Nb, Zr and N j.The Sr, Nd isotopic characteristics of the Lajimiao norite-gabbro complex are similar to those of ophiolites. Its εNd values are constant, about+2; whereas εst values have wide variation from - 6.4 to +31.2 and positively correlate with Na2O, H2O+ and CO2 contents and the Fe3+/Fe 相似文献
2.
Dengfeng He Yunpeng Dong Xueyi Xu Junlu Chen Xiaoming Liu Wei Li Xiangmin Li 《地学前缘(英文版)》2018,9(5):1399-1415
The Chinese Altai in northwestern Xinjiang has numerous outcrops of granitoids which provide critical information on accretionary orogenic processes and crustal growth of the Central Asian Orogenic Belt.Zircon U-Pb ages, Hf-isotopic compositions and whole-rock geochemistry of monzogranite and granodiorites in the Qinghe County are employed to elucidate Paleozoic tectonics of the Chinese Altai. Granodiorites have crystallization ages of 424.6 ± 3.1 Ma(MSWD = 0.23) and 404.0 ± 3.4 Ma(MSWD = 0.18);monzogranite was emplaced in the early Permian with a crystallization age of 293.7 ± 4.6 Ma(MSWD = 1.06). Both granodiorites and monzogranite are I-type granites with A/CNK ratios of 0.92 -0.97 and 1.03 -1.06, respectively. They also show similar geochemical features of high HREE and Y contents, low Sr contents and Sr/Y ratios, as well as enrichment of Cs, Rb, Th and U, and depletion of Nb, Ta, P and Ti.These geochemical features indicate that the monzogranite and granodiorites were formed in an arc setting related to subduction. The gneissic monzogranites display high SiO_2 and K_2 O contents, and belong to the high-K calc-alkaline series. In the chondrite normalized REE distribution pattern, the monzogranite samples exhibit enrichment of LREE with strong negative Eu anomalies(σE u =0.44 -0.53), zircon εHf(t) values from +7.24 to +12.63 and two-stage Hf model ages of 463 -740 Ma. This suggests that the monzogranite was generated from the mixing of pelitic and mantle material. The granodiorite samples are calc-alkaline granites with lower contents of Si O_2 and Na_2 O + K_2 O, higher contents of TiO_2, Fe_2O_3~t, MgO and CaO compared to the monzogranite samples. They also show enrichment of LREE and moderate negative Eu anomalies(σE u= 0.54 =0.81), as well as slightly higher differentiation of LREE than that of HREE. The425 Ma granodiorite has zircon εHf(t) values from -0.51 to +1.98 and two-stage Hf model ages of 1133 -1240 Ma, whereas the 404 Ma granodiorite displays those of +2.52 to +7.50 and 816 -1071 Ma.Geochemistry and zircon Hf isotopic compositions indicate that granodiorites were formed by partial melting of juvenile lower crust. Together with regional geology and previous data, the geochemical and geochronological data of the monzogranite and granodiorites from this study suggest long-lived subduction and accretion along the Altai Orogen during ca. 425 -294 Ma. 相似文献
3.
WANG Xiang CHEN Jianping XU Yanbo ZHENG Yongchun YAN Bokun WU Yunzhao 《《地质学报》英文版》2015,89(6):1882-1894
Spectra are sensitive in detecting main minerals on the lunar surface from visible light to infrared light. Since spectral characteristics of minerals are closely related to their compositions and the maturity level of soil on the Moon, studying the compositions and distribution of elements and minerals on the lunar surface can help to understand the evolution of the Moon through remote sensing technology. The correlation between the spectral characteristics of Chang’e-1 interference imaging spectrometry (IIM) reflectance images and the mineral contents of LSCC (Lunar Soil Characterization Consortium) lunar surface mineral samples was discussed and the spatial distributions of FeO and Al2O3 contained in both pyroxene and plagioclase on LQ-4 were studied using the improved angle parameter method, MNF, and band ratio statistics. A comparison of the mapping results of the optical models by Lucey, Shkuractov and other researchers on Clementine and the gamma ray spectrometry data shows that the content error is within 0.6% for lunar mare areas and close to 1% for the highland areas. The tectonic framework on the lunar surface was also investigated. And based on integrated analysis of previous findings on topography of the lunar surface, Chang’e LAM, CCD and LOLA images and the gravity anomalies data (Clementine GLGM-2), the tectonic unit subdivision was established for LQ-4, the idea of subdividing the lunar tectonic units was proposed, and this will provide a good foundation for studying the lunar tectonic evolution. 相似文献
4.
Melt glasses for seven types of rock ranging from acid to basic were prepared under 1.0 GPa on a multi-anvil pressure apparatus, YJ-3000 ton press. Densities and elastic properties of the melt glasses were compared with those described in previous studies. It was found that the glasses melted under 1.0 GPa were consistent in density with both naturally-occurring glassy rocks and artificially prepared glasses melted at ambient pressure. The densities of glasses are negatively correlated with the SiO2 contents and positively correlated with the （MgO＋FeO） contents. The compressive velocity （Vp） of glass tends to increase with decreasing SiO2 contents and increasing （MgO＋FeO） contents. The shear velocity （Vs） of glass tends to increase slightly with increasing SiO2 contents, which has little connection with the （MgO＋FeO） contents. It was calculated from densities and velocities that the elastic moduli of glasses are negatively correlated with the SiO2 contents and positively correlated with the （MgO＋FeO） contents. 相似文献
5.
The sediments atop the sequence of ophiolite usually contain Fe(-Mn-Si)exhalites,chemical sediments that aremainlycomposedofamorphousFe-Mn oxy-hydroxides and chert/jasper.They were precipitated from hydrothermal fluids produced by deep leaching of basalt particularly during volcano activity or seafloor spreading.These hydrothermal Fe exhalites provide a good record for the depositional environment and the ocean environment as well.A well-preserved Phanerozoic Fe deposit,Motuosala Fe-Mn deposit,resulted from hydrothermal exhalation,was investigated for its trace element and Fe isotope geochemistry.The deposit is located in Xinjiang province,China and is hosted in a suit of Carboniferous volcano-sedimentary clastic rocks.The Fe deposit is mainly composed of massive hematite Fe oreand banded hematite-jasper ore.The hematite ore/band and jasper band were subjected to be analyzed.They are both composed mainly of Fe2O3 and Si O2,with very low contents of Al2O3 and Ti O2(1%),indicating they werechemical precipitates with little detrital contamination.They both show slightly LREE depleted or near flat PAAS-normalised REE patterns,with positive Eu anomalies and Y anomolies,indicating that they were sourced from a mixture of high-temperature fluids and seawater.Compared to the hematite Fe ore/band,the jasper band shows higher EuSN/EuSN*but lower Y/Ho values.δ56Fe values for the hematite Fe ores are clustered around-0.3‰,similar to those for high-temperature fluids.The jasper samples show heavier Fe isotope compositions varying from-0.1‰to0.5‰,indicating that they were resulted from partial Fe precipitation.For all samples,δ56Fe values are related to Y/Ho and EuSN/EuSN*values.The results indicate that the hematite Fe ore and jasper were deposited in different environments.The jasper was deposited in a more anoxic condition with higher hydrothermal fluids/seawater ratio,probably when the hydrothermal activity was more intense;while the hematite Fe ore was deposited in a more oxic condition with lower hydrothermal fluids/seawater ratio,probably when the hydrothermal activity was weaker. 相似文献
6.
One of the most important tasks of evaluating natural resources of petroliferous basins is to determine the organic matter abundance of source rocks in the basin.The usual method for assessing the organic carbon content of source rocks is based on laboratory analyses.There is a deviation in calculating organic carbon content due to the heterogeneous distribution of organic matter and the artificial factors when sampling.According to the continuous characteristics of information logging,the conventional logging curves(mainly acoustics and resistivity,etc.) were calibrated with the organic carbon experimental data of cores,cuttings or sidewall cores.The organic carbon content of source rocks of the 4 th(Es 4) and 3 rd(Es 3) members of the Shahejie Formation in western sag in the Liaohe depression was estimated directly by a great amount of continuous data including resistivity and acoustic logging,etc.Comparison between the results from computer processing and lab analysis of logging data shows that the organic carbon contents derived from the computer processing of logging data have the same reliability and accuracy as the lab analysis results.The present data show that this method is suitable to evaluate the source rocks of western sag in the Liaohe depression and has great potential in evaluating natural resources of sedimentary basins in the future.On the basis of logging data of source rocks,experimental data and existing geochemical analyses of the Liaohe Oilfield,the corresponding total organic carbon(TOC) isograms of source rocks were plotted.The source rocks of Es 4 and Es 3 of the Shahejie Formation are thought to be beneficial to hydrocarbon accumulation due to the high TOC. 相似文献
7.
UKAEGBUV.U. EKWUEMEB.N. 《中国地球化学学报》2005,24(2):129-135
Rock samples representing various igneous and metamorphic rocks of southern Obudu Plateau were analyzed for rare-earth element ( REE ) behavior by ICP-MS. Results of the analyses indicate a range of REE abundances and distinctive patterns from highly fraetionated patterns with negative Eu anomalies in granitic rocks to relatively low abundances and less REE fractionated flat patterns with little Eu anomaly in some paragneisses, schists, enderbites and dolerites to unfractionated patterns with positive Eu anomalies in some paragneisses and charnockites. Over all, there are low to high ∑ REE contents with negative to positive Eu anomalies. The ratios of different parameters, especially La/Yb and Ce/Yb, show behaviors consistent with crustal to mantle derivation. The heterogeneity of REE abundances and REE patterns reflects mantle to crustal petrogenetic variations of different rock suites on the Plateau. The LREE content is higher than the HREE content in the highly differentiated rocks, as evidenced by their La/Yb,Ce/Yb and La/Sm ratios, which are normally higher in residual products than in primary melts. The dominantly intermediate nature of the source rock of the orthogneisses is suggested by the generally low ∑ REE. The granites enriched in LREE and depleted in HREE and some of the charnockites with negative Eu anomalies were probably formed by partial melting and crystallization. 相似文献
8.
KREEP Rocks 总被引：2，自引：1，他引：2
KREEP rocks with high contents of K, REE and P were first recognized in Apollo-12 samples, and it was confirmed later that there were KREEP rock fragments in all of the Apollo samples, particularly in Apollo-12 and -14 samples. The KREEP rocks distributed on the lunar surface are the very important objects of study on the evolution of the moon, as well as to evaluate the utilization prospect of REE in KREEP rocks. Based on previous studies and lunar exploration data, the authors analyzed the chemical and mineral characteristics of KREEP rocks, the abundance of Th on the lunar surface materials, the correlation between Th and REE of KREEP rocks in abundance, studied the distribution regions of KREEP rocks on the lunar surface, and further evaluated the utilization prospect of REE in KREEP rocks. 相似文献
9.
Daishe WU Baoshan ZHENG Xiuyi TANG Mingshi WANG Jun HU Shehong LI Binbin WANG Robert B. Finkelman 《中国地球化学学报》2006,25(B08):54-54
Three hundred and six coal samples were taken from the main coal mines of twenty-six provinces, autonomous regions, and municipalities of China. The method of Kjeldahl-Gunning Analysis was used to measure the nitrogen contents in the samples. Nitrogen in coals is principally of organic nature. A weak positive correlation between coal rank and nitrogen content is inferred in the study. The distribution of nitrogen in each geological age, coal-cumulating area and province＇s coals was studied. The contents of nitrogen in Chinese coals show approximately a normal distribution, and 90% of the values range from 0.52% to 1.41%, the average nitrogen content in Chinese coals is designated as the arithmetic mean, 0.98%. 相似文献
10.
The purpose of this study is to comparatively investigate the plant uptake, accumulation and translocation behaviors of polycyclic aromatic hydrocarbons (PAHs) as priority pollutants in soil contaminated with oily sludge. The influence of different oily sludge application doses on the uptake of contaminants was studied together with the profile of individual PAH in roots, straws and leaves of winter wheat. Pot experiments were conducted using oily sludge application doses of 0, 5, 10, 15 and 20 percent, respectively. The total PAHs contents of control soil and oily sludge were 16.96 and 3504.66 μg/g, respectively. Analysis for the contents of the 16 PAHs was carried out with a HPLC-UV using plant tissue samples obtained at the 265th day of growth. The total PAHs contents in treated winter wheat were 9.02-334.81 ng/g for roots, 8.45-336.52 ng/g for straws and 10.70-406.32 ng/g for leaves. In addition to 5% of oily sludge dose, the total PAHs content in leaves was always highest under other doses of oily sludge application. With respect to individual PAH, the content did not show a significant plant tissue related trend. However, both the total content and individual content of PAHs in treated winter wheat tissues did increase with increasing oily sludge application dose. Another analysis for the control soil indicates that the degradation rate of PAHs was significantly enhanced by winter wheat after 265 days of growth based on the residual concentrations of PAHs in planted and unplanted soils. 相似文献
11.
在大数据及信息共享时代,迫切需要构建系统矿物学数据库,为地学及相关领域的科技创新、人才培养及公众提供共享服务。本文通过系统矿物学理论和国家级数据库建设实践经验,提出了系统矿物学数据中矿物种的分级、分类、编码和矿物名称、化学成分、晶体形态、晶体结构、物理性质、化学性质以及矿物的成因和产状等基本数据项的构建方法和规范;设计了用于建立数据库的数据字典、数据类型和功能模块;介绍了系统矿物学数据库发布的软硬件环境以及整体技术架构,并在国家科技基础条件平台应用实践;最后探讨了矿物学数据挖掘和维基理念与技术在矿物学大数据库建设中的应用。 相似文献
12.
环境矿物学：矿物学在环境科学研究中的应用 总被引：6，自引：0，他引：6
矿物学在环境科学中的应用将是21世纪矿物学研究的一个主要方面。 作者所在实验室曾做过的一些环境矿物学研究的实例有：核废料的处置,矿物表面性质的研究,对有毒金属的还原和固定作用的微生物效应,大气烟尘微粒的研究,矿物表面阳离子的本征吸附常数之理论计算,等等。矿物-水-微生物体系在分子级别上之相互作用的定量研究,对于理解低温地球化学和生物地球化学过程将是重要的。 相似文献
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14.
月海玄武岩的矿物组成反映了岩浆源区的化学成分以及岩石形成时的物理和化学环境,对月球热演化研究以及月球资源的开发利用都具有重要意义。本文选择延展范围长的冷海为研究区,基于月球矿物成像光谱仪(Moon Mineralogy Mapper,简称M3)数据研究其矿物的空间变化特征。综合利用光谱、地形、元素等多源遥感数据将冷海划分为25个地质单元。提取169条新鲜坑光谱曲线,获取吸收中心波长、波段面积比等光谱参数。通过光谱吸收特征分析,获得冷海玄武岩铁镁质矿物变化特征。东部冷海地层较老,铁镁质矿物主要为单斜辉石,辉石钙含量较月球样品单斜辉石钙偏低,与澄海以及雨海老的地层矿物组成类似。西部冷海和露湾的地质单元较为年轻,富含橄榄石。风暴洋和雨海年轻玄武岩的矿物也富含橄榄石。这种富含橄榄石、大面积分布的玄武岩反映了月球晚期热演化的独特性。尽管地理上冷海为一个独立的月海,其东西部玄武岩矿物组成的差异以及与其同位置周围月海矿物组成的类似性反映了冷海玄武岩源区与周围月海具有联系。 相似文献
15.
我国名贵的田黄宝石,经X-射线衍射分析、红外光谱分析、差热分析及电子显微镜等研究,证实为一种罕见的珍珠石。田黄按宝石状态划分为三种:1.田黄冻,矿物成分主要为珍珠石,有时可见到一点伊利石。2.田黄石,是珍珠石与地开石成不同比例的混合物。3.银裹金,是纯白色半透明的地开石包裹着金黄色的冻状珍珠石。 这种宝石极为罕见难得,仅在我国寿山的坂田砾石层中偶然发现。文中探讨了寻找原生田黄的标志。 相似文献
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17.
The composition and structure of mineral substance in shells of three Jurassic ammonites (Cadoceras elatmae) from the Makar’ev South outcrop in Kostroma oblast, Russia, have been studied. The studied shells differ in degree of preservation.
The shell of one ammonite with partly retained internal structure has been replaced with quartz, carbonate-bearing apatite-(CaF),
and newly formed aragonite. Other shells without retained internal structure underwent phosphatization rather than replacement
with quartz. This difference serves as the basis for a discussion on fossilization conditions. Silicification of the shell
supports preservation of its wall and elements of the internal structure. It is suggested that quartz might be biogenic in
origin and was formed in cavities of phosphate substance, which had replaced the soft tissue of ammonites. 相似文献
18.
《International Geology Review》2012,54(11):1042-1050
Minerals of the stibnite-antimonselite series, in close association with tiemannite, clausthalite, kullerudite, Se-bearing stibioluzonite, native gold, quartz, and barite, were discovered in Cambrian stratabound gold deposits at La'erma and Qiongmo, western Qinling, China. Based on S/(S + Se) ratios of microprobe analyses, the binary stibnite-antimonselite system is divided into four series: stibnite, Se-stibnite, S-antimonselite, and antimonselite. Micro-hardness of the stibnite series (Sb = 58.47 to 72.99 wt%, S = 11.86 to 28.76, and Se = 0.00 to 29.12) and the antimonselite series (Sb = 48.94 to 59.13 wt%, Se = 29.20 to 46.86, S = 1.99 to 11.43) is 101.26 and 103 kg/mm2, respectively. Representative reflectivities of the four series are (470 nm) Rg'= 42.62 to 47.62%, Rp' = 30.83 to 40.55%; (550 nm) Rg' = 41.84 to 46.75%, Rp'= 31.48 to 38.85%; (590 nm) Rg' = 42.25 to 46.63%, Rp' = 30.73 to 39.46%; (650 nm) Rg' = 43.30 to 46.48%, Rp' = 30.01 to 41.56%. Cell parameters obtained from two stibnite samples (containing 3 to 5% Se) are a = 1.1209 to 1.1212 nm, b = 1.1299 to 1.1303 nm, c = 0.3847 to 0.3849 nm; and those of S-antimonselite and antimonselite are a = 1.1591 to 1.1593 nm, b = 1.1724 to 1.1747 nm, and c = 0.3941 to 0.3984 nm. 相似文献
20.
《矿物学报》2013,(Z1)
It has been over 40 years since scientists and engineers attempted to automate optical microscope and scanning electron microscope (SEM) to measure the mineral liberation characteristics of ores in order to predict their flotation responses. As early as 1963, the first optical instrument equipped with a video camera to analyse grain structure of a sample was produced by Metals Research Instrument Corporation (Image Analysis Company Ltd., 1970), which introduced Quantimet 720, a fully digital image analysis system, in 1969. Remarkably, Quantimet system is still widely used today. 相似文献