中国东部断陷湖盆细粒沉积岩岩相划分方案探讨——以渤海湾盆地南部古近系细粒沉积岩为例

细粒沉积岩岩相研究是烃源岩和页岩油、致密油储层研究的重要基础,鉴于我国陆相断陷湖盆环境多变和细粒沉积岩类型多样、岩石组合类型复杂的特点,需要进行细粒沉积岩岩相分类。以渤海湾盆地南部古近系细粒沉积岩发育段为研究对象,通过厘米级岩芯观察描述、岩石薄片鉴定、激光共聚焦显微镜观察分析等技术,研究细粒沉积岩基本特征。陆相断陷湖盆细粒沉积岩岩相划分可以按照(1)宏观岩芯精细观察描述,归纳垂向岩石类型组合;(2)分析沉积微环境;(3)对不同岩石类型组合进行X射线全岩矿物衍射和TOC测试,划分岩石类型和岩相大类;(4)微观镜下剖析纹层叠置关系;(5)分析成因和形成机制,对岩亚类细分等5步进行。岩相大类划分要简洁,是为满足油田勘探工作易于操作、建立与常规测井资料之间关系等要求;亚类细分是便于研究微观源储关系、分析沉积微环境和储层微观结构等。     

四川米易垭口地区前震旦纪五马箐组与其侵入岩体的锆石U-Pb年代学、Lu-Hf同位素特征及其地质意义SCIEI北大核心CSCD

在扬子板块西缘断续分布有多套变质沉积岩系,厘定区内不同岩石单元的时代对于探讨扬子西缘的构造演化具有重要意义。本文对出露于扬子板块西缘米易垭口地区的五马箐组变沉积岩以及侵入其中的片麻状黑云二长花岗岩体进行了锆石LA-ICP-MS U-Pb定年和Lu-Hf同位素分析。结果表明:区内五马箐组的沉积时代介于1.19~1.01Ga,其地层归属为会理群而非康定群,位于五马箐组之下的“冷竹关组”并非变沉积地层而是一套片麻状黑云二长花岗岩体。五马箐组碎屑锆石年龄存在~1.56Ga、~2.50Ga两个主要峰值以及~1.43Ga、~1.68Ga、~1.87Ga、~2.32Ga、~2.68Ga五个次要峰值,推断其物质来源主要为扬子板块西南缘的撮科杂岩、隐伏的或还暂未发现的太古代基底岩石、同时期岩浆岩和早期变沉积岩的再循环。碎屑锆石的ε_(Hf)(t)值在~1.7Ga发生了显著变化,暗示扬子板块西缘的构造体制由陆壳汇聚向裂谷活动转变,且在~1.56Ga处于裂谷岩浆活动的峰期。花岗岩体正的ε_(Hf)(t)值反映出扬子板块西缘在~1.0Ga有一次新生陆壳生长事件,可能是格林威尔造山后的伸展塌陷构造背景下裂谷岩浆活动的产物。     

CCSD主孔金红石与石榴子石中锆石包裹体的Hf元素地球化学特征

本文样品是采自中国大陆科学钻探(CCSD)主孔的含金红石榴辉岩,在这些样品中常常含有锆石副矿物,锆石可以呈粒间矿物存在,也可以包裹在其他矿物(如石榴子石、金红石)中。背散射电子图像(BSE)显示这些锆石包裹体的亮度较弱,颗粒较小(约10~30μm),发育多晶面,晶体内部结构和成分均匀。采用能谱分析(EDS)方法来测量锆石的元素成分含量,结果表明:1这些锆石具有很高的Hf含量,金红石中达到1.51%~2.45%,石榴子石中为1.77%~2.13%;2Zr/Hf值约为35.92,比一般的基性原岩中的锆石的Zr/Hf值明显要低,这些特征说明它们很可能是形成在超高压条件下的变质锆石。     

Timing of Magma Mixing in the Gangdisě Magmatic Belt during the India-Asia Collision： Zircon SHRIMP U-Pb Dating

Abstract  Abundant mafic microgranular enclaves (MMEs) extensively distribute in granitoids in the Gangdisê giant magmatic belt, within which the Qüxü batholith is the most typical MME‐bearing pluton. Systematic sampling for granodioritic host rock, mafic microgranular enclaves and gabbro nearby at two locations in the Qüxü batholith, and subsequent zircon SHRIMP II U‐Pb dating have been conducted. Two sets of isotopic ages for granodioritic host rock, mafic microgranular enclaves and gabbro are 50.4±1.3 Ma, 51.2±1.1 Ma, 47.0±1 Ma and 49.3±1.7 Ma, 48.9±1.1 Ma, 49.9±1.7 Ma, respectively. It thus rules out the possibilities of mafic microgranular enclaves being refractory residues after partial melting of magma source region, or being xenoliths of country rocks or later intrusions. Therefore, it is believed that the three types of rocks mentioned above likely formed in the same magmatic event, i.e., they formed by magma mixing in the Eocene (c. 50 Ma). Compositionally, granitoid host rocks incline towards acidic end member involved in magma mixing, gabbros are akin to basic end member and mafic microgranular enclaves are the incompletely mixed basic magma clots trapped in acidic magma. The isotopic dating also suggested that huge‐scale magma mixing in the Gangdisê belt took place 15–20 million years after the initiation of the India‐Asia continental collision, genetically related to the underplating of subduction‐collision‐induced basic magma at the base of the continental crust. Underplating and magma mixing were likely the main process of mass‐energy exchange between the mantle and the crust during the continental collision, and greatly contributed to the accretion of the continental crust, the evolution of the lithosphere and related mineralization beneath the portion of the Tibetan Plateau to the north of the collision zone.     

Successional stages of biological soil crusts and their microstructure variability in Shapotou region (China)

In order to investigate succession of biological soil crusts (BSCs) and their microstructure variability, we conducted this work in Shapotou revegetation region at the southeast edge of Tengger Deser. The results showed that BSCs generally succeeded as a pathway of “Algae crusts, algae–lichen crusts, lichen crusts, lichen–moss crusts and moss crusts”. Occasionally mosses directly occurred on algae crusts, and BSCs succeeded from algae crusts to moss crusts. Crust vertical stratification was a common phenomenon, from top to bottom an inorganic layer, algae-dense layer and algae-sparse layer were divided in algae crusts; a thallus layer, rhizoid layer and sub-rhizoid layer in lichen crusts; a “stem-leaf” layer, rhizoid layer and sub-rhizoid layer in moss crusts, respectively. The main crust binding organisms varied from filamental cyanobacteria (dominated by Microcoleus) in algae crusts to lichen rhizoids, free-living cyanobacterial filaments and fungal hyphaes in lichen crusts, and to moss rhizoids and fungal hyphaes in moss crusts. The dominant phototrophic organisms varied from Microcoleus (algae) in algae crusts to Collema (lichens) in lichen crusts, and to Bryum (or Didymodon and Tortula; mosses) in moss crusts. Total phototrophic biomass increased while the free-living algal biomass decreased with the succession of BSCs. In addition, exopolysaccharides and fine particles accumulated in the course of development and succession of BSCs, all of which lead to a gradual increase in crust thickness and porosity, while decrease in the bulk density.     

盐岩储气库注气排卤期剩余可排卤水分析

地下盐穴溶腔注气排卤过程中天然气和卤水共存,排卤管进入到卤水的深度及排卤速率决定了天然气是否会被卤水带出地表,如何调整后期排卤速率,降低排卤过程中带出天然气的风险,是注气排卤过程中的施工技术难题。针对该问题,采用流场分析理论对注气排卤后期盐岩储库腔底流场进行了模拟分析,得到排卤管外壁卤水向下流速;根据天然气气泡在卤水中的运移速率,分析确定了注气排卤后期不同剩余卤水深度下的安全排卤速率,为施工后期注气排卤速率调整提供了技术支撑。     

越南O Quy Ho钼矿床的成矿时代及成矿物质来源探讨

越南西北部O Quy Ho钼矿床为范士版成矿带的典型钼矿床之一,矿体以脉状形式就位于中生代花岗岩中,辉钼矿主要赋存于石英脉及长石石英脉中,与黄铁矿、黄铜矿、磁铁矿等共生。8件样品硫同位素分析结果表明,δ34S介于0.14‰～3.34‰之间,平均值为1.53‰,表明成矿物质具有深源特征。黄铁矿的206Pb/204Pb范围为18.583～22.355,207Pb/204Pb变化于15.632～15.812之间,208Pb/204Pb变化于38.989～39.199;辉钼矿的206Pb/204Pb、207Pb/204Pb、208Pb/204Pb分别为18.686～18.737、15.655～15.660和39.081～39.082,与范士版含角闪石花岗斑岩具有成因联系。辉钼矿Re-Os同位素等时线测年获得了(36±1)Ma的年龄,该年龄与金沙江-红河新生代斑岩铜钼矿成矿带岩浆-成矿活动的年龄一致,提出O Quy Ho钼矿床为金沙江-红河新生代斑岩铜钼矿带的一部分。     

冀东某地原生红刚玉矿床地质特征

冀东某地原生刚玉矿床具有埋藏浅,刚玉个体大、微红至暗红色、半透明至不透明等特点,经人工改善可生产低档红宝石。本文主要介绍该矿床的刚玉形态特征、物理性质、晶体结构、包裹体特征及矿床形成的地质条件。研究认为,本矿床应属深熔型混合岩化作用成因,即“混合岩型”刚玉矿床。     

准噶尔盆地结构及其圈闭类型

准噶尔盆地是复合叠加前陆盆地 ,其原型分别形成于板块俯冲、碰撞、造山带后期复活、拗拉槽回返和板内皱陷作用有关的大地构造环境。其古生代盆地的形成与相邻的阿尔泰山和东、西准噶尔山、天山及博格达山的造山作用相关。中新生代盆地的形成和改造与其南部特提斯域板块俯冲碰撞造山引起的盆地相邻造山带的复活有关。相邻造山带时空上不均一的造山作用对盆地的影响不同 ,形成了盆地独特的结构。各坳陷均由与其形成有关的造山带前缘冲断带、陡坡带、山前凹陷、缓坡带和前隆及前缘皱陷等构成 ,前隆之间的叠加构成了盆地的大型隆起 ,皱陷叠加构成了盆地的中央坳陷。不同类型的圈闭在坳陷中有规律地分布着     

白垩纪快速气候变化研究新进展——温室世界中的冰川证据

白垩纪被认为是两极无冰的典型温室气候时期,但近年来对于白垩纪存在短暂冰川甚至是极地冰盖的猜想引起了越来越多的关注。根据前人提出的冰川或气候变冷证据,如冰川遗迹、全球海平面快速下降事件以及δ18O正偏事件等,总结了白垩纪可能存在冰川的时期,包括Berriasian Valanginian之间、Valanginian晚期、Barremiana期、Aptian Albian之交、Albian Cenomanian之交、Cenomanian中期和末期、Turonian中期、Coniacian中期、Santonian早期、Campanian晚期、Campanian Maastrichtian之交和Maastrichtian末期等。对这些证据的有效性进行详细的讨论,同时也对白垩纪冰川的可能成因进行探讨。笔者认为,白垩纪即便存在冰川,也是小规模、短暂地存在,因此,精确的年代学约束是进行白垩纪冰川研究的前提;米兰科维奇旋回控制下的气候波动是白垩纪形成短暂冰川的可能成因。