超大型会泽富锗铅锌矿复合成因

会泽富锗铅锌矿。是近年老矿山深部找矿取得重大突破的典范,而其成因则是当前研究、讨论的热点。笔者认为该矿之形成,既非“MVT型”,亦非“VMS型”,而是与深部隐伏燕山期酸性岩有关的中温岩浆热液叠加、改造、富化的复成因矿床。自加里东期起长期处于张裂环境。深部昭通．弥勒硅镁层隆起,既是幔源玄武岩（热地幔柱）上涌的前奏,又为深部矿源上升创造畅通空间。与多旋回活动的小江深断裂相沟通的NE向矩形断裂网,是导矿、输矿、储矿的有利构造。继火山热液成矿之后,伴随燕山期褶皱、断裂和深部酸性岩浆的上升,发生第二期叠加矿化．矿石中伴生与酸性岩有关的元素组合．并以与酸性岩有关的锗富集为特征。     

Misconceptions about the Hubble recession law

Almost all astronomers now believe that the Hubble recession law was directly inferred from astronomical observations. It turns out that this common belief is completely false. Those models advocating the idea of an expanding universe are ill-founded on observational grounds. This means that the Hubble recession law is really a working hypothesis. One alternative to the Hubble recession law is the tired-light hypothesis originally proposed by Zwicky (Proc. Nat. Acad. Sci. 15:773, 1929). This hypothesis leads to a universe that is an eternal cosmos continually evolving without beginning or end. Such a universe exists in a dynamical state of virial equilibrium. Observational studies of the redshift-magnitude relation for Type Ia supernovae in distant galaxies might provide the best observational test for a tired-light cosmology. The present study shows that the model Hubble diagram for a tired-light cosmology gives good agreement with the supernovae data for redshifts in the range 0<z<2. This observational test of a static cosmology shows that the real universe is not necessarily undergoing expansion nor acceleration. An erratum to this article can be found at     

藏北昂吾地区超基性岩的蛇纹石化和磁铁矿化过程及影响因素

班公湖-怒江缝合带广泛分布超基性岩及蛇纹石化超基性岩,已有研究表明它们与区域成矿关系密切,其蛇纹石化过程使一些元素活化并具有一定的成矿潜力。位于班-怒带中段的昂吾地区蛇纹石化超基性岩主要矿物成分有橄榄石、单斜辉石、铬铁矿、利蛇纹石、磁铁矿和绿泥石等,原岩恢复表明该超基性岩为单辉橄榄岩。镜下鉴定、背散射电子图像、能谱成分分析和电子探针分析结果显示单辉橄榄岩的蛇纹石化及蚀变过程可分为三个阶段:(Ⅰ)以形成相对富铁蛇纹石(Mg#=75～88)为主,基本无磁铁矿析出;(Ⅱ)形成相对富镁的蛇纹石(Mg# 90),析出磁铁矿;(Ⅲ)蛇纹石进一步蚀变成绿泥石。热力学模拟及多组分矿物相平衡图表明,在蛇纹石化过程中,昂吾地区超基性岩中的辉石脱硅致使反应体系SiO_2活度升高,限制了磁铁矿的生成。同时也发现,在利蛇纹石稳定存在的温度区间内(100～300℃),本研究的蛇纹石化体系温度倾向高值区,不利于磁铁矿的析出。进而探讨了原岩成分、反应体系SiO_2活度及温度等因素对蛇纹石化过程中磁铁矿析出的影响。本研究有助于理解班-怒带内超基性岩的蛇纹石化过程及磁铁矿化机制。     

Geochronology and mineralogy of the Weishan carbonatite in Shandong province,eastern China

The Weishan REE deposit is located at the eastern part of North China Craton (NCC), western Shandong Province. The REE-bearing carbonatite occur as veins associated with aegirine syenite. LA-ICP-MS bastnaesite Th-Pb ages (129 Ma) of the Weishan carbonatite show that the carbonatite formed contemporary with the aegirine syenite. Based on the petrographic and geochemical characteristics of calcite, the REE-bearing carbonatite mainly consists of Generation-1 igneous calcite (G-1 calcite) with a small amount of Generation-2 hydrothermal calcite (G-2 calcite). Furthermore, the Weishan apatite is characterized by high Sr, LREE and low Y contents, and the carbonatite is rich in Sr, Ba and LREE contents. The δ¹³C_V-PDB (−6.5‰ to −7.9‰) and δ¹³O_V-SMOW (8.48‰–9.67‰) values are similar to those of primary, mantle-derived carbonatites. The above research supports that the carbonatite of the Weishan REE deposit is igneous carbonatite. Besides, the high Sr/Y, Th/U, Sr and Ba of the apatite indicate that the magma source of the Weishan REE deposit was enriched lithospheric mantle, which have suffered the fluid metasomatism. Taken together with the Mesozoic tectono-magmatic activities, the NW and NWW subduction of Izanagi plate along with lithosphere delamination and thinning of the North China plate support the formation of the Weishan REE deposit. Accordingly, the mineralization model of the Weishan REE deposit was concluded: The spatial-temporal relationships coupled with rare and trace element characteristics for both carbonatite and syenite suggest that the carbonatite melt was separated from the CO₂-rich silicate melt by liquid immiscibility. The G-1 calcites were crystallized from the carbonatite melt, which made the residual melt rich in rare earth elements. Due to the common origin of G-1 and G-2 calcites, the REE-rich magmatic hydrothermal was subsequently separated from the melt. After that, large numbers of rare earth minerals were produced from the magmatic hydrothermal stage.     

具相对性的特殊地理位置应用研究的基础理论与方法探讨

着重对具相对性的特殊地理应用研究的基础上理论与方法的进行探讨,主要探讨了地图投影选择与图形处理为核心心的定位研究,特殊地理位置旅游辐射区定区原则与广泛旅游区位类型系统及其应用分析等方面的内容。     

八庙-青山金红石矿床地球化学特征

金红石矿床含矿岩石常量元素总体上与玄武岩接近,但以低硅,高钛,高ＣＯ２,高碱度为特征。矿床微量元素与地壳的差别显著,稀土元素较高,分布模式呈轻稀土富集型,Ｅｕ一般为正常型与碧玄岩最接近,Ｔｉ与Ｂａ,Ｃｏ,Ｐｂ,Ｓｒ,Ｔｈ,Ｖ,Ｙ及稀土元素呈正相关与Ｃｒ和Ｎｉ呈负相关,δ＾３４Ｓ多数与（超）铁镁质岩石接近,最大值小于且靠近现代海水。     

江西银山铜多金属矿床成因再认识

从矿体形态、蚀变、矿化分带、稳定同位素和矿物包裹体等方面论述了矿床与本区岩浆活动在时间、空间和成矿物质来源等方面的关系,提出了银山铜多金属矿床是与燕山早期岩浆活动有关的火山—次火山热液矿床的新认识。     

南海西南次海盆岩石圈结构及其地质意义

南海地区岩石圈资料稀少,阻碍了其形成演化过程的研究.为此,本次研究结合大地热流、空间重力异常、高程、大地水准面和地震数据,在南海西南次海盆反演了两条2.5维岩石圈剖面.本次计算基于三种假设：岩石圈地幔的密度取决于岩石温度;研究区岩石圈处于热稳定状态;研究区处于重力均衡状态.在剖面A-E中,岩石圈底界面从珠江口盆地的105 km迅速抬升到西沙海槽处的50 km,在西沙海槽、西沙-中沙群岛和西南次海盆变化不大,为50~60 km.在剖面F-I中,岩石圈底界面从西沙群岛-中建地块处的88 km向海盆逐渐抬升,在西南次海盆处为46~50 km,到郑和隆起再逐渐变深至64 km.我们比较了西南次海盆岩石圈的冷却模型和热稳定模型,根据冷却模型由水深和热流数据所推断的西南次海盆年龄比实际年龄差很多,说明冷却模型不适用于西南次海盆.通过对比剖面A-E和剖面F-I,说明了剖面A-E经历了更长时间的拉伸,证明南海西南次海盆在形成演化过程中是从北东向南西逐步打开的渐进式扩张.最后,我们综合分析西南次海盆及其大陆边缘的岩石圈结构、减薄陆壳区范围、碳酸盐台地的分布、下地壳韧性流动、流变结构和沉积层特征等多方面资料,认为西南次海盆在形成演化过程中岩石圈地幔首先破裂而地壳后破裂,属于type Ⅱ型非火山型大陆边缘.     

Use of Magnet Technology for Phosphate Elimination from Municipal Sewage

The present report describes the set-up and first operation results of a novel carousel magnetic separator. This carousel magnetic separator is suitable for continuous separation of magnetized particles from water. Continuous operation is achieved by a segmented rotating separation matrix. This matrix also allows the use of low-cost permanent magnets, by means of which magnetic fields of up to 0.5 T can be generated without energy consumption. The suitability of a first prototype of this carousel magnetic separator was tested for elimination of magnetite-containing iron phosphate and iron hydroxide flocs. These flocs result from conventional precipitation/flocculation of municipal sewage with FeCl₃ and the addition of magnetite particles generated by wet-chemical processes. First results demonstrate that the carousel magnetic separator can reduce phosphate concentrations of up to 14 mg/L PO₄^3–-P in the inlet to below 1 mg/L PO₄^3–-P in the outlet at filtration rates of about 40 m/h. Magnetite dosage in the range of 50 mg/L affects phosphate precipitation positively via a slight reduction of the precipitant volume. However, the total amount of chemicals required for phosphate elimination is increased by the substances needed for magnetite production. Therefore, a further reduction of magnetite dosage must be achieved.     

新疆哈密卡拉塔格铜(锌)矿红石幅1∶50 000矿产地质图数据库

新疆哈密卡拉塔格铜(锌)矿红石幅(K46E009008)1∶50 000矿产地质图数据库是根据《固体矿产地质调查技术要求(1∶50 000)》(DD2019-02)和行业其他标准及要求,在充分利用1∶200 000、1∶50 000等区域地质调查工作成果资料的基础上,采用数字填图系统进行野外地质专项填图,并应用室内与室外填编图相结合的方法完成。本数据库将中-上奥陶统荒草坡群大柳沟组、下志留统红柳峡组和卡拉塔格组的建造类型进行了重新划分,把图幅内侵入岩时代划分为志留纪、泥盆纪、二叠纪等3期,建立了岩浆岩演化序列。图幅区内有大中小型矿床和矿点共8个,成矿时代集中分布在志留纪、石炭纪,赋矿围岩为火山碎屑岩和次火山岩,该区优势矿产以铜锌金为主,矿床类型以VMS型和次火山热液脉型矿床为主,分布在图幅东南一带。除金属矿产外,尚有膨润土矿床产出,具有较好的找矿潜力。本数据库包含5个地层单位和3期岩浆岩资料,数据量约为 15.1 MB。这些数据充分反映了该图幅 1∶50 000 矿产地质调查示范性成果,对该区矿产资源研究和勘查等具有参考意义。