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Haitaite-(La), (La, Ce)(U4+, U6+, Fe2+)(Fe3+, Al)2(Ti, Fe2+, Fe3+)18O38, is a new member of the crichtonite group. It is named after the Haita Village in the Miyi County of Sichuan Province, China, where the mineral was discovered. The mineral occurs as black opaque centimeter-sized aggregates in the external contact zone between the Neoproterozoic (~800 Ma) alkali feldspar granite and the Mesoproterozoic (~1700 Ma) micaschist. In the studied sample, haitaite-(La) is associated with other minerals, including ilmenite, magnetite, rutile, zircon, brannerite and uraninite. The new mineral is a black, metallic phase and has a Mohs hardness of 6, with a density of 4.99 g/cm3 (calculated) and 5.03 g/cm3 (measured). Haitaite-(La) is opaque in transmitted light and grayish-white under reflected light, with a reflectivity between 22.5% and 16.42% in the 400–700 nm band (SiC, in the air). The compositions of the mineral were measured by EPMA, the U4+/U6+ ratio was determined by X-ray photoelectron spectroscopy and the Fe2+/Fe3+ ratio was determined by M?ssbauer spectroscopy. Haitaite-(La) is trigonal, belongs to R3ˉ and has unit-cell parameters a = 10.3678(5) ?, c = 20.8390(11) ?, V = 1939.9(2) ?3, Z = 3. The crystalline structure is composed of octahedra with 9 layers of close-packed octahedra (M1, M3, M4, M5), tetrahedra (M2) and contains large 12-coordinated M0 sites. 相似文献
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大河坝石墨矿是川北米仓山南缘石墨矿带新发现的大型显晶质石墨矿床。研究了该矿床的地质特征和矿石主量、微量及稀土元素地球化学特征,结果表明:含矿岩层为副变质岩,矿区石墨矿体原岩沉积于缺氧的还原环境,原岩为一套含碳质黏土质细—粉砂岩及含碳质泥灰岩组合。微量元素特征指示矿体原岩由近海陆源碎屑物沉积形成,沉积水体主要为盐度较低的、混合不均匀的淡水—半咸水。矿石ΣREE平均值为150×10-6,与泥灰岩相近;δCe值平均为0.91,呈弱负异常,δEu值平均为0.67,呈负异常,具滨海潮坪相沉积特征。含矿岩石δ13C值为-21.4‰~-19.0‰,平均为-19.86‰,表明成矿碳质来源主要为有机碳,并混合了部分无机碳。矿床成因类型为沉积变质型,其变质作用可能包括多次区域变质作用并叠加了混合岩化作用。 相似文献
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四川省同德石墨矿床是近年来在扬子板块西缘发现的大型中-大鳞片晶质石墨矿之一。为研究同德石墨矿地质特征及矿床成因,本文采用系统的野外地质调查、地球物理与地球化学等方法,并开展山地取样工程、岩矿测试研究工作。研究认为:同德石墨矿产于古元古代前震旦系康定岩群冷竹关组变质岩层中,赋矿岩石为云母石英片岩。矿体主要呈层状、似层状近南北向展布。矿石矿物为石墨,脉石矿物主要为石英、白云母、黑云母、斜长石及少量铁质矿物等。矿石自然类型为云母石英片岩型,工业类型为中-大鳞片晶质石墨矿。其原岩为一套含碳质泥岩、泥质粉砂岩、砂岩;碳质主要来源为有机物。物探自然电位梯度呈正负相伴,最低电位和梯度值为零的位置往往指示了石墨矿体的顶面中心;音频大地电磁测深呈带状向深部延伸的低阻异常指示了石墨矿体的深部赋存形态。矿床的形成经历了沉积成岩-区域变质阶段,属沉积变质型矿床。 相似文献
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A methodology for regionalizing 3‐D effective porosity at watershed scale in crystalline aquifers 下载免费PDF全文
Benoît Dewandel Yvan Caballero Jérôme Perrin Alexandre Boisson Fabrice Dazin Sylvain Ferrant Subash Chandra Jean‐Christophe Maréchal 《水文研究》2017,31(12):2277-2295
An innovative approach for regionalizing the 3‐D effective porosity field is presented and applied to two large, overexploited, and deeply weathered crystalline aquifers located in southern India. The method derives from earlier work on regionalizing a 2‐D effective porosity field in that part of an aquifer where the water table fluctuates, which is now extended over the entire aquifer using a 3‐D approach. A method based on geological and geophysical surveys has also been developed for mapping the weathering profile layers (saprolite and fractured layers). The method for regionalizing 3‐D effective porosity combines water table fluctuation and groundwater budget techniques at various cell sizes with the use of satellite‐based data (for groundwater abstraction), the structure of the weathering profile, and geostatistical techniques. The approach is presented in detail for the Kudaliar watershed (983 km2) and tested on the 730 km2 Anantapur watershed. At watershed scale, the effective porosity of the aquifer ranges from 0.5% to 2% in Kudaliar and between 0.3% and 1% in Anantapur, which agrees with earlier works. Results show that (a) depending on the geology and on the structure of the weathering profile, the vertical distribution of effective porosity can be very different and that the fractured layers in crystalline aquifers are not necessarily characterized by a rapid decrease in effective porosity and (b) that the lateral variations in effective porosity can be larger than the vertical ones. These variations suggest that within a same weathering profile, the density of open fractures and/or degree of weathering in the fractured zone may significantly vary from a place to another. The proposed method provides information on the spatial distribution of effective porosity that is of prime interest in terms of flux and contaminant transport in crystalline aquifers. Implications for mapping groundwater storage and scarcity are also discussed, which should help in improving groundwater resource management strategies. 相似文献
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This study is concerned with the tectono‐thermal history of the Kathmandu nappe and the underlying Lesser Himalayan sediments (LHS) that are distributed in eastern Nepal. We carried out zircon fission‐track(ZFT) dating and obtained 16 ZFT ages from the eastern extension of the Kathmandu nappe, the Higher Himalayan Crystalline, Kuncha nappe, and the Main Central Thrust (MCT) zone. The ZFT ages of the frontal part of the Kathmandu nappe range from 13.0 ±0.8 Ma to 10.7 ±0.7 Ma and exhibit a northward‐younging tendency. These Middle Miocene ZFT ages indicate that the frontal part of the Kathmandu nappe remained at a temperature above 240 °C until the termination of its southward emplacement at 12–11 Ma. The ZFT ages of the LHS range from 11.1 ±0.9 Ma in the southern part of the Okhaldhunga Window to 2.4 ±0.3 Ma of the augen gneiss in the northern margin and also exhibit a northward‐younging age distribution. The ZFT ages show the northward‐younging linear distribution pattern (?0.16 Ma/km) along the across‐strikesection from the frontal part of the Kathmandu nappe to the root zone, without a significant age gap. This distribution pattern indicates that the Kathmandu nappe, the underlying MCT zone, and the Kuncha nappe cooled from the frontal zone to the root zone as a thermally united geologic body at a temperature below 240 °C. An older ZFT age (456.3 ±24.3 Ma), which was partially reset at the axial part of the Midland anticlinorium in the central part of the Okhaldhunga Window, was explained by downward heating from the “hot” Kathmandu nappe. The above evidence supported a model that southward emplacement of the hot Kathmandu nappe resulted in a thermal imprint on the upper part of the LHS; however, the lower part did not reach 240 °C. 相似文献
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M. Aulinas M. Garcia‐Valles J. L. Fernandez‐Turiel D. Gimeno J. Saavedra G. Gisbert 《地球表面变化过程与地形》2015,40(4):447-458
The characteristics of rock varnish from the Campo de Piedra Pomez (CPP, Andes Argentina) provides new insights into the development of rock varnish under severe dusty conditions. The CPP varnish has been analysed using SEM‐EDAX and Raman techniques. The rock coating is tens of microns in thickness and under the microscope shows a micro to cryptocrystalline appearance and a general granular texture. Silica (quartz, cristobalite and amorphous silica) is the main phase forming these coverings followed by Al, K and Na compounds. Minor Fe oxides and Mn oxides are the source for the orange (Fe) and brown (Fe and Mn) hues of the coating. The results obtained for the CPP coating show that desert varnish developed under dusty circumstances does not have the appearance of typical rock varnish. Textural characteristics include high crystallinity and granular arrangement of the components. Moreover the absence of typical microlaminations is related to the presence of aeolian mineral grains which inhibit their development. The main mechanism of formation of rock varnish under such environmental circumstances is the direct incorporation of aeolian mineral grains into the varnish. However, other physicochemical processes are also required to explain the formation of varnish components such as amorphous silica or iron oxides phases. Although the development of the desert varnish may act as a protector of the underlying pyroclastic rock, the extreme and persistent windy conditions in the CPP field are high enough to weather and erode not only the rock coating but also the original ignimbrite. As other warm desert sites on Earth, the CPP area can also be considered as possible terrestrial analogue to Mars. Some environmental attributes might be similar to those expected on the Martian surface and thus, textural similarities between the CPP varnish and the rock varnish‐like coating of Mars are likely. Copyright © 2014 John Wiley & Sons, Ltd. 相似文献
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吉林省集安地区是晶质石墨矿的主要产地,晶质石墨矿矿床赋存于集安群荒岔沟组中,层控特征明显,同时也是其直接找矿标志。 相似文献