我国油页岩的成分和品级划分

根据我国21个油页岩产地,26个样品的分析数据,讨论了油页岩的含油率、灰分产率,灰分成分和密度等品级的划分,指出我国缺少高含油率页岩,提出中、低含油率油页岩的标准。并认为含油率在3.5~5.0%称含油页岩,含油率低于3.5%不应当作油页岩。油页岩灰分成分大多是硅铝质,因而灰熔点偏高。提出了油页岩灰分成分的分类表。指出我国油页岩的密度高于国外样品,原因是钙质成分含量较低。     

The New Meteorite Fall of Yanzhuang—A Severely Shocked H6 Chondrite with Black Molten Materials

At 21:45 hr (Beijing time) on Oct. 31, 1990 the Yanzhuang meteorite hit the ground at the Yanzhuang village, Wenyuan County, Guangdong Province. Several fragments, totalling 3.5 kg, were recovered during the field survey. This meteorite is a rare one of its kind due to its heavily shocked features and thick veins made up of black molten materials. Olivine and low-calcium pyroxene are compositionally homogeneous with Fa=18.59, Fs=16.35 and Wo=1.29. The chemical composition (total Fe=28.0%) and recrystallized texture of the chondritic mass show that the Yanzhuang is an H6 chondrite. The black molten materials occur in the form of blocks (up to 2×3×4 cm in size) and veins (0.1–15 mm in width), and contain a lot of rounded and elliptic FeNi-FeS blobs (up to 6–10 mm in length). The metal in these blobs exhibits distinct dendritic structure characteristic of rapid cooling. Unmolten and molten samples are very similar in chemical composition, fitting well with the average H-chondrites. Partial melting and FeNi/FeS-silicate separation have not been observed in the molten materials of the Yanzhuang. This project was financially supported by the Science Foundation of Guangdong Province.     

新疆疏附6.0级地震震害与损失

新疆疏附６．０级地震震害与损失宋立军，张勇，朱令人（新疆维吾尔自治区地震局，乌鲁木齐）０前言１９９３年１２月１日凌晨４时３７分新疆疏附县境内发生６．０级地震，使喀什地区疏附县和克孜勒苏柯尔克孜自治州阿克陶县所辖５乡（镇）的５１个大队，５个直属场遭受不...     

河南熊耳山中生代花岗岩与成矿关系

熊耳山地区花岗岩出露面积约为404．8km^2，岩体围岩主要为太华群变质岩系和熊耳群火山岩系。这些岩体的年龄值在81-182．8Ma之间。据野外观察、室内岩矿鉴定、数据处理及计算机数学模型模拟，获知本区花岗岩系1型，物质来源于下部地壳太华群片麻岩结晶基底，     

第四章 地球化学特征及副矿物特征

第一节 地球化学特征 中祁连山西段中—晚元古代地层厚逾万米。我们在进行专题研究过程中,采集了岩石全分析样56个,半定量光谱分析样1379个。现根据各地层剖面中岩石化学分析资料及微量元素分配情况,简要分析各地层单元的地球化学特征。 一、常量元素地化特征 沉积岩石的化学成分,能反映沉积物的物质来源、搬运方式、沉积环境和变质程度。它不仅对探求元素富集规律有价值,而且对推断沉积年代的古地理、古气候、古环境、古构造和岩浆活动有意义。     

形成类地行星初始物质的探讨

不同类型陨石、内行星和外行星在主要元素或化学组成上的差异，表明从早期太阳星云内的凝聚作用开始，到吸积作用前后，曾发生过明显的化学分馏作用。随着与太阳的距离增大，难熔元素的丰度逐渐增高，温度和压力逐渐下降，据此可推测不同类型陨石形成的部位及类地行星的初始物质。