牟平邓格庄金矿地质特征及找矿方向

邓格庄金矿成因类型为中温热液充填式富硫含金黄铁矿石英脉型金矿床。通过对邓格庄金矿床的地质特征、控矿因素及矿床成因的系统研究,认为矿区NNE向断裂与其他方向断裂交汇部位为金矿的有利成矿部位,在分析找矿标志的基础上,提出应加大矿区深部及外围的找矿力度,进一步查证地球物理、化学异常,以期发现新的金矿远景区,进而指出了深部找矿的方向。     

广西佛子冲铅锌矿田成岩成矿时代研究

广西佛子冲铅锌矿田位于桂东南博白-岑溪多金属成矿带的NE端,区内发育燕山期花岗岩、花岗闪长岩、二长花岗斑岩和英安质凝灰熔岩等;其中花岗闪长岩和二长花岗斑岩与铅锌成矿关系密切,成矿岩体形成时代分别为156Ma和127Ma。     

New data on the correlation of skarn and gold mineralization at the Tardan deposit (northeastern Tuva)

Gold mineralization of the Tardan deposit is of different spatial occurrences and is related to different hydrothermal-metasomatic formations, the main ones being skarn-magnetite bodies, metasomatites of mineralized crush zones, and metasomatites of argillizitic-rock association. The formation of gold mineralization was a multistage process related to the repeated magmatism of the Tannu-Ola complex. It took place in a wide temperature range (400–150 °C), which determined the diversity of produced mineral assemblages. The gold mineralization associated with magnetite bodies shows a spatial correlation with magnesian and calcareous skarns and is localized in plagiogranites and gabbro-diorites of the Tannu-Ola complex intruded in the Late Ordovician. Gold mineralization that occurs in crush zones and along the fault sutures in moderate- and low-temperature hydrothermal-metasomatic rocks (propylites, beresites, serpentinites, and argillizites) formed somewhat later than skarns as a result of the intrusion of granite dike bodies. Comparative analysis of different types of gold mineralization showed both a change of mineral assemblages of the gold mineralization during the ore formation and some geochemical difference between gold and gold-bearing ores. In passing from early to late occurrences of native gold, its fineness decreases, the contents of admixtures correspondingly increase, and the gold composition changes. Gold of high-temperature rocks is rich in Cu (up to 17%), and gold of low-temperatures rocks has higher contents of Ag and Hg.     

天然气溶解过程中组分分馏模型及其应用

天然气不同组分在水中溶解度的差异,导致溶解相与残留游离相天然气组分组成不同,即发生组分的溶解分馏效应。溶解分馏效应在天然气水溶运移、溶解散失等过程中均有发生。揭示天然气组分的溶解分馏规律、建立定量分馏模型,有助于天然气气源对比和成藏过程示踪。以Henry定律为依据,对不同组分溶解特征分析,提出了溶解度分数的概念,并建立了溶解分馏模型。根据该模型和各组分的溶解度分数和天然气溶解量,可计算各组分的溶解分馏量,恢复天然气初始组成特征。计算表明,威远震旦系气藏初期的天然气组成为:CH4为72.70%,C2H6为0.09%,CO2为22.41%,N2为4.07%,干燥系数(C1/C1-5)为99.876%。溶解作用使天然气中CO2含量显著降低,烃类气体含量增加,而天然气干燥系数降低。结果有助于天然气成因判识和气源对比等。     

西藏冈底斯矿带成矿作用及远景分析

冈底斯带矿床众多,类型复杂,主要有斑岩型铜（金钼）矿床、矽卡岩型铁铜-铅-锌（银）矿床、层控铅-锌-银矿床、火山岩型金-银矿床及雄村式铜-金矿床。矿床地质特征和同位素年龄表明,冈底斯带南部的矿床与新特提斯洋壳向北俯冲-陆陆碰撞及碰撞期后的构造岩浆事件有关;冈底斯带北部的矿床与班公湖-怒江洋壳向南俯冲-陆陆碰撞及碰撞期后构造岩浆事件有关。冈底斯带与洋壳的俯冲-碰撞有关的岩浆活动强烈,成矿条件优越。西藏高原在碰撞后发生了快速抬升剥蚀,部分矿床顶部出现低温组合矿化,多数矿床保存良好。     

华南重要金属矿床的成矿规律——时代爆发性、空间分带性、基底继承性和热隆起成矿

华南热液矿床形成的时代爆发性、空间分带性及其成矿元素对前寒武纪基底的继承性表明,构成华南基底和含矿建造的前寒武纪地层（主要为元古界）是华南陆内热液成矿作用的主要成矿物质来源,燕山期花岗岩类是热液成矿作用的主要成矿能量来源;华南热液成矿的区域分布趋势、矿床形成过程和成矿岩体演化等,均表现出与构造热隆起动态有关的成矿特征。多期花岗岩类侵入和迅速块断隆升造成地温梯度增高,基底含矿建造提供成矿物质,以及有利的热液通道和扩容空间是造成构造隆起带或盆地“凹中隆”成矿的重要条件。燕山期花岗岩成岩成矿与大陆地壳的多旋回熔融或再循环有密切的成因关系;地震层析图像资料显示,华南中生代软流圈上涌是造成华南陆壳热隆起的动力学因素。但其成因不同于地幔柱机制,具有被动上涌特征,可能与太平洋板块俯冲形成的大型冷幔柱下沉和地幔过渡带崩溃有关。     

四川德格错阿金矿特征与矿床成因初析

错阿金矿床赋存于理塘义敦群上三叠统瓦能组变基性火山岩中,金矿体受次级北北西-近南北向韧性-脆韧性剪切变质带控制,与金矿化有关蚀变主要为黄铁矿化、辉锑矿化和硅化、碳酸盐化、金云母化及石墨化。矿床成因为蚀变构造型。甘孜-理塘断裂带北段嗄拉、错阿、海子口三个矿化集中区内大部份化探异常具有面积大、强度高、梯度变化大、元素组合好等特点,具有很好的找矿前景。     

New perspectives on Mars’ crustal magnetic field

The planet Mars lacks, today, a planetary, dynamic magnetic field, but strong, intense, localized magnetic fields of lithospheric origin, one to two orders of magnitude larger than the terrestrial lithospheric field, are present. This lithospheric magnetic field is the result of magnetization processes in the presence of a magnetic dynamo and of demagnetization processes after the dynamo shutdown, such as impact or volcanoes. This crude scenario can be more accurately specified by interpreting global and local models of the current magnetic field of Mars. Some specific areas are studied, including the intensely magnetized Terra Sirenum, as well as the magnetic anomaly associated with Apollinaris Patera. Magnetic minerals could be of primary and/or secondary origin; this latter would imply an early hydration of a basaltic crust. A scenario, in which Mars experienced a major polar wander due to the Tharsis bulge, prior to the cessation of its dynamo, is proposed and discussed.     

北武夷地区逆冲推覆构造的特征及其控矿作用

北武夷地区成矿地质条件优越,矿产资源分布广泛,而广泛发育的推覆构造深刻影响着矿床的成生与保存。区域性推覆构造是成矿前、成矿期还是成矿后的构造,其精细结构特征如何,是否具有控岩控矿作用,如果是破矿作用,是否造成矿体重复增大或者隐伏、缺失等问题,严重影响着地质找矿的效果。建议开展面积性、追索性的路线地质调查,查明逆冲推覆构造的区域分布、不同单元的产状、构造样式,分别采用40Ar-39Ar和Re-Os定年技术测定推覆构造和矿体的形成时代,结合定量化分析及精细构造解析,研究构造与矿床的成生联系,预测隐伏矿体可能的位置,进而为北武夷地区寻找隐伏矿床和扩大矿床远景提供参考。     

西藏札达盆地控盆断裂有限元数值模拟

札达盆地是喜马拉雅构造带中的一个山间断陷盆地,其演化过程与盆地两侧的控盆构造密切相关。对控盆断裂的构造应力场进行模拟计算,将有助于进一步深化对本区构造控盆的认识。因此,在对盆地构造地质进行详细调查的基础上,结合本区的深部地质与地球物理资料,对札达盆地控盆断裂的构造应力场进行了模拟。计算结果表明,札达盆地的演化明显受盆地两侧边界断裂的控制,札达盆地是在整体南北向挤压应力的作用下,不同块体差异隆升作用的结果。其南侧的控盆断裂为北倾的正断层,北侧的控盆断裂为南倾的逆断层,二者共同形成了南降北升的翘板式断陷盆地运动过程,是喜马拉雅地块在陆内汇聚挤压构造环境中构造应力场调整的一种方式。