Lambert problem solution in the hill model of motion

The goal of this paper is obtaining a solution of the Lambert problem in the restricted three-body problem described by the Hill equations. This solution is based on the use of pre determinate reference orbits of different types giving the first guess and defining the sought-for transfer type. A mathematical procedure giving the Lambert problem solution is described. This procedure provides step-by-step transformation of the reference orbit to the sought-for transfer orbit. Numerical examples of the procedure application to the transfers in the Sun–Earth system are considered. These examples include transfer between two specified positions in a given time, a periodic orbit design, a halo orbit design, halo-to-halo transfers, LEO-to-halo transfer, analysis of a family of the halo-to-halo transfer orbits. The proposed method of the Lambert problem solution can be used for the two-point boundary value problem solution in any model of motion if a set of typical reference orbits can be found.     

A search for previously unrecognized metal-poor subdwarfs in the Hipparcos astrometric catalogue

We have identified 317 stars included in the Hipparcos astrometric catalogue that have parallaxes measured to a precision of better than 15 per cent, and the location of which in the ( M _V ,( B − V ) _T ) diagram implies a metallicity comparable to or less than that of the intermediate-abundance globular cluster M5. We have undertaken an extensive literature search to locate Strömgren, Johnson/Cousins and Walraven photometry for over 120 stars. In addition, we present new UBV ( RI )_C photometry of 201 of these candidate halo stars, together with similar data for a further 14 known metal-poor subdwarfs. These observations provide the first extensive data set of R _C I _C photometry of metal-poor, main-sequence stars with well-determined trigonometric parallaxes. Finally, we have obtained intermediate-resolution optical spectroscopy of 175 stars.
47 stars still lack sufficient supplementary observations for population classification; however, we are able to estimate abundances for 270 stars, or over 80 per cent of the sample. The overwhelming majority have near-solar abundance, with their inclusion in the present sample stemming from errors in the colours listed in the Hipparcos catalogue. Only 44 stars show consistent evidence of abundances below [Fe/H]=−1.0 . Nine are additions to the small sample of metal-poor subdwarfs with accurate photometry. We consider briefly the implication of these results for cluster main-sequence fitting.     

山东英格庄金矿床构造控矿特征及深部预测

英格庄金矿床位于山东牟乳金矿带巫山断裂的南缘,其围岩主要以古老变质岩与昆嵛山花岗岩为主,为含金石英脉型金矿。文章通过对英格庄金矿床控矿断裂发展史以及断面几何形态与金矿体赋存位置关系的研究,发现矿体在断层带中的分布具有规律性。深部地球化学原生晕研究表明,英格庄金矿床Bi与Hg关系非常密切,是金矿化的最佳指示元素,且在已知矿体下方出现前缘晕与尾晕相互叠加的现象。结合矿体在断裂中分布的规律以及原生晕特点,对英格庄矿床深部第二富集段进行了预测,并预测在-220m下有第二金富集段存在,且具有很大的经济价值。     

新疆哈巴河县托库孜巴依金矿床26号矿脉盲矿预测的构造叠加晕实用模式

根据新疆哈巴河县托库孜巴依金矿床的地质特征及成矿规律,对矿床的26号脉及主要围岩进行了系统采样和多元素分析,结合矿区地球化学背景确定了各元素的分带标准;通过对26号矿脉(体)的地球化学特征及构造叠加晕特征研究,总结出金矿(体)单一次成矿的原生晕轴向分带,对矿体不同成矿阶段形成的晕在空间上的叠加形态进行了识别,建立了矿体形成的构造叠加晕实用模式(包括成矿构造叠加晕模式、预测标志及分带标准),利用该实用模式对矿脉深部以及外围进行找矿预测,提出了找矿预测靶位。     

甘肃李坝金矿床定位预测的叠加晕模式

李坝金矿具有多期多阶段叠加成矿成晕的特点,根据不同成矿阶段元素组合和单阶段形成原生晕的垂直分带规律（从上→下是As,Hg,Sb→Ag,Pb,Au,Cu,Zn→Bi,Mn)及不同成矿阶段形成矿体（晕）在空间上的叠加特点,建立了矿床的原生叠加晕模式,确定了盲矿定位预测标志。     

西藏隆子县恰嘎锑矿4号脉原生晕特征及深部找矿预测

西藏隆子县恰嘎锑矿位于藏南错美-隆子锑金成矿带中东部,该区成矿条件有利,是找锑铅锌的良好靶区。研究表明：①矿体原生晕发育,且分带明显。②结合原生异常分布态势及其与矿体的关系,成晕组分可以分为：前缘元素（Cd、Hg、As）、近矿元素（上部为Pb、Zn,中部为Sb,下部为Cu、Au、Ag）、尾晕元素（Mn、Bi、Mo、W、Sn）。③对该区利用浓集中心法和分带指数法分别求出了相近的分带序列：Pb-Zn-Mn-Bi-Mo-W-Sn-Cd-Hg-As-Sb-Cu-Au-Ag-Ba。④深部找矿方面,矿体很大可能向深部继续延伸或有盲矿体存在,且该矿床为热液型矿床。⑤在原生晕系统研究的基础上构建了深部矿体评价的指标（Cd×Hg×As×Sb）D/（Bi×Mo×W×Sn）D,数据表明该指标随深度的增加有规律地降低,是预测深部矿体资源潜力的有效指标。     

The globular cluster system of the Sagittarius dwarf spheroidal galaxy: the age of Terzan 8

We present deep V - and I -band CCD photometry of the globular cluster Terzan 8, recently found to be a member of the globular cluster system of the Sagittarius dwarf spheroidal galaxy. We accurately estimate the metallicity of Terzan 8, and provide the first direct determination of the colour excess toward this cluster. Our robust age estimate confirms that this cluster is indeed coeval with typical Galactic globulars of comparable metal content, and thus it is probably significantly older than at least two other Sagittarius clusters, Terzan 7 and Arp 2. The implications of this result on the star formation history of the Sagittarius galaxy are briefly discussed.     

广西岩溶区金属硫化物矿床风化与元素表生迁移特征

对广西岩溶区三个铅锌硫化物矿床风化带观测结果表明，中低山岩溶区硫化物矿床具有更强烈的风化淋滤作用，但次生晕面积较小；岩溶平原区硫化物矿床风化与元素表生迁移特征较相似于非岩溶区的情况，表现在可产生较宽的ｐＨ偏低带和较大面积的次生晕