会泽超大型铅锌矿床成矿时代研究

云南会泽超大型铅锌矿床由麒麟厂和矿山厂两个独立的铅锌矿床组成。利用两组同源矿物组合Rb Sr等时线方法测定了麒麟厂6号矿体的成矿时代,测定结果分别为(225 1±2 9)Ma和(225 9±3 1)Ma,根据已知的分布于该矿床北部和西南部分布的峨眉山玄武岩成岩时代为250Ma左右,有多个火山喷发旋回,显示多期次的喷发活动,认为川—滇—黔成矿区内铅锌成矿作用与峨眉山玄武岩岩浆活动存在成因联系。     

个旧锡矿阿西寨矿段化探异常分带及找矿意义

通过对个旧锡矿阿西寨矿段地表基岩的地球化学勘查。发现其成矿元素的地球化学异常表现出明显的环状分带，并以测区内隐伏花岗岩凸起为中心，元素分带序列与元素本身的地球化学性质所决定的侧向迁移活动能力相符合。该现象再次证实个旧锡矿为花岗岩岩浆期后热液成矿，花岗岩是大多数成矿金属元素的物质来源，同时也是成矿热液活动的主要驱动营力。分析认为，阿西寨测区是一个相对较完整和独立的(凸起)成矿场，成矿热液活动以阿西寨凸起为中心。成矿热液活动体系受断裂导流影响，在以花岗岩凸起为中心的分带控制下，可能存在的工业矿体将在主干断裂附近和有利的构造岩性界面产出。     

我国主要金矿类型中黄铁矿"电子-空穴心"特征及影响因素

通过对我国主要金矿类型中黄铁矿导电类型的分析表明，黄铁矿“电子。空穴心”与金矿床的成因类型具有密切的联系，华北地台太古代变基性火山岩中的金矿床(绿岩带型)、热水淋滤型(卡林型)金矿床，黄铁矿多为单一的“电子心”型导电。大多数产于中生代岩体中的中深脉状金矿、火山次火山岩中的金矿床，黄铁矿为“电子心”、“空穴心”混合型导电，个别的为单一的“空穴心”导电。黄铁矿的“电子．空穴心”受杂质成分As、Co、Nl在成矿背景中的丰度，进入黄铁矿品格中的替代能力的差异、补偿类质同象现象、成矿时温度以及．f(S2)等多种因素的耦合制约。     

云南武定迤腊厂铜矿含矿石英脉40 Ar-39Ar年龄及其意义

对武定迤腊厂铜矿成矿期石英进行了40Ar-39Ar同位素年龄测定,得到马鞍形年龄谱,坪年龄为(784.25±0.95)Ma,等时线年龄为(783.93±8.59)Ma.地质特征研究表明该矿床后期改造作用明显,并非同生沉积或成岩作用早期成矿,而与晋宁期Rodina大陆裂解有关.武定迤腊厂铜矿的形成可能是在Rodinia大陆裂解时,从深部带来大量成矿物质,改造成岩时期初始的矿化,形成矿床的叠加富集和最终定位,晋宁-澄江期是该矿床的主成矿期.     

东川桃园式铜矿Ar-Ar同位素年龄及意义

通过对东川桃园铜矿与铜矿共生石英的40Ar/39Ar同位素年龄的测定,得到马鞍形年龄谱,其坪年龄为768.43Ma±0.58Ma,等时线年龄为770.00Ma±5.44Ma。该矿床后期改造作用明显,并非同生沉积或成岩作用早期成矿,而与晋宁期Rodina大陆裂解有关。东川铜矿的形成可能是在Rodinia大陆裂解时,从深部带来大量成矿物质改造成岩时期初始的矿化,形成矿床的叠加富集和最终定位,因此,晋宁-澄江期是东川铜矿的主成矿期。     

西秦岭三个典型金矿床稳定同位素地球化学特征

据八卦庙金矿、李坝金矿、小沟里金矿稳定同位素研究,金矿床δ34S比正常沉积岩变化范围窄,比岩浆-火山岩型矿床宽,硫源是海水硫酸盐还原硫与深部热液来源硫所组成的混合硫。石英包裹体流体氢、氧同位素分布于岩浆水、大气降水的重叠过渡区,更靠近岩浆水区,岩浆水的同位素特征更明显。八卦庙金矿石英脉3He/4He高于地壳3He/4He值(n×10-8),低于地幔3He/4He值(n×10-5),为壳-幔混合源。上述同位素地球化学证据表明,金成矿与岩浆岩有一定的成因关系。岩浆岩与金矿床空间关系密切,矿区内脉岩发育,脉岩为矿体的上下盘。含矿岩石中发育斑点构造,斑点为黄铁矿、磁黄铁矿、毒砂、绿泥石、石英、绢云母、黑云母、堇青石、红柱石、电气石、碳酸盐等热变质矿物和热液交代矿物,表明花岗岩为成矿提供热动力。据八卦庙金矿、李坝金矿、小沟里金矿稳定同位素地球化学研究,结合成矿地质背景分析和区域成矿地质特征对比,认为凤太、西成、礼岷地区金矿与微细浸染型(卡林型)金矿有明显的差别,该区金矿类似于岩浆热液矿床。     

镇旬铅锌矿田热水沉积硅岩研究

从镇(安)旬(阳)铅锌矿田热水沉积硅岩的产状、形态、岩石结构、构造、矿物成分、化学成分、微量元素、稀土元素、硫同位素、氧同位素等研究表明，本区硅岩具有以热液为主兼有生物和正常沉积的特征，并非典型热水沉积岩。     

石英脉型辉钼矿矿床多建造地球化学异常特征

通过对石英脉型辉钼矿床水系沉积物和区域成矿带多建造地球化学异常特征的研究,为寻找石英脉型钼矿床提供地球化学论据。     

The impact of hydrological changes on travertine deposits related to thermal springs in the Pamukkale area (SW Turkey)

Pamukkale thermal waters (35 °C), exhibiting calcium-bicarbonate-sulfate composition and high carbon dioxide concentration, are of a predominantly meteoric origin. The meteoric fluid, circulating through faults and fractures, is heated by magmatic intrusions at great depth, and ascends from deep reservoirs to the surface. Mixing with relatively cold groundwater in the near surface zone promotes different saturation conditions with respect to calcium carbonate that later precipitates at depth and/or the surface. Dissolution-deposition processes of calcium carbonate both at surface and depth environments may help to reconstruct past climate direction in the field. During wet climate conditions a high-rate of calcium carbonate accumulation would be expected to occur at the surface because thermal fluid would be under-saturated with respect to calcium carbonate at depth because of a relatively higher mixing ratio with cold groundwater. During dry climate conditions the thermal fluid would be super-saturated at depth because of the highly acidic environment. Hydrometeorological studies reveal that the annual precipitation at the Pamukkale hydrothermal field tends to decrease with time. This climatic change in the area was also detected from geological records. While humid climate conditions prevailed during the late Quaternary, the area has recently been affected by arid/semi-arid climate conditions, followed by some episodic transitions. This study has shown how the system has possibly reacted to different climate conditions since antiquity.     

Chemical Composition of Ores from the Takara Volcanogenic Massive Sulfide Deposit, Central Japan

Abstract. The Takara volcanogenic massive sulfide (VMS) deposit occurs in Miocene formation of the Misaka Mountain, the South Fossa Magna region, central Japan. The tectonic setting of the Misaka Mountain is reconstructed to be a part of the paleo Izu-Ogasawara arc which collided with the Honshu arc and to form accreted body in the present position. The Takara deposit, therefore, is considered to have formed in the paleo Izu-Ogasawara arc.
The ores from the Takara deposit are classified into pyrite-type ore, chalcopyrite-type ore, and sphalerite-type ore on the basis of chemical composition and their mineral assemblages. Some pyrite-type ores are characterized by their high Au content. The Au content is hardly recognized in the chalcopyrite-type and sphalerite-type ores.
The ores from the Takara deposit have intermediate bulk chemical composition between those from the Besshi-type deposits and the Kuroko-type deposits that are two representative VMS deposits. However, the bulk chemical composition is closer to that from the Kuroko-type deposits. And moreover, chemical composition of tetrahedrite-tennantite series minerals (tetrahedrite) is similar to that from the Kuroko-type deposits. The bulk chemical composition (Cu, Zn, Co, Pb, and As contents) of ores is affected by the chemical composition of volcanic rocks associated with VMS deposits.