辽北开原岩群蛇绿混杂岩的特征

岩石化学、地球化学资料表明,中晚元古代开原岩群蛇绿混杂岩由蛇绿岩和岛弧拉斑玄武岩、钙碱玄武岩（斜长角闪岩、角闪石岩）、钙碱性基性—中性火山岩（变粒岩）、陆缘碎屑岩（浅粒岩）组成。蛇绿岩由绿泥滑石片岩（橄榄岩）、角闪岩类岩石（大洋拉斑玄武岩）、石英岩（远洋深海硅质岩）组成。与内蒙古温都尔庙群蛇绿岩,吉林色洛河群同时位于古华北陆块北缘,为陆缘活动带向古华北陆块俯冲形成。这表明古华北陆块北缘造山带在中晚元古代即已出现。     

内蒙古呼和浩特北部古元古代二道洼群的变质演化

出露于内蒙古呼和浩特北部的二道洼群 ,为一套陆源碎屑岩 碳酸盐岩夹中基性火山岩变质建造。岩石组合及其地球化学特征指示其形成于陆内裂陷槽或稳定陆缘盆地环境。研究表明 ,二道洼群是古元古代早期产物 ,2 4 50～ 2 4 0 0Ma开始接受沉积 ,大约在 2 2 0 0～2 10 0Ma之间开始褶皱回返 ,遭受了低角闪岩相变质作用 ,具有碰撞造山带的变质P T t轨迹。研究结果有助于华北陆台北缘古元古代的地壳演化研究 ,有助于乌拉山区二道洼群与孔兹岩系的相互关系的探讨。     

东昆仑西段托库孜达坂群中组火山岩岩石地球化学特征及构造环境分析

托库孜达坂群中组火山岩厚度大、分布广,由下而上包括3个火山活动旋回,下部为溢流相-次火山岩相-沉积相;中部为爆发相-溢流相-次火山岩相-沉积相;上部为溢流相-沉积相。中、上部旋回火山作用最强,形成时代为早石炭世早期。通过岩石学、岩石地球化学等综合研究,其岩石主要为英安质火山角砾岩、火山角砾凝灰岩、安山玢岩、安山岩、流纹英安质凝灰熔岩等;SiO2一般大于70%,Na2O-2相似文献   

广东南雄盆地的"南雄层"和"丹霞层"

本文沿用263地质队资料,将南雄红层底部出现的第Ⅰ沉积旋回划为松山组;重新厘定了南雄群的含义,阐明其间各岩石地层单位顶、底界线标志;沿用罗佛寨群;指出不必用丹霞群(组)表示南雄盆地边缘相的粗碎屑岩层,并认为丹霞盆地的丹霞组相当于南雄盆地的园圃组下段,建议南雄盆地弃用丹霞群(组)一名.在此基础上提出,粤北地区白垩系-古近系岩石地层序列是由松山组,南雄群(园圃组、主田组、浈水组),罗佛寨群(上湖组、浓山组、古城村组)组成.     

Discovery of Late Permian Jianshanzi volcanic rocks in Qinghe valley of northern Liaoning and its geologic significance

Jianshanzi volcanic rocks at Qinghe valley in the northern Liaoning were considered belonging to Early Proterozoie Gaojiayu Formation of Liaohe Group, or to Early Cambrian Beidagou Formation of Qinghezhen Group, or Middle-Late Proterozoic Shenjiapu Formation-Complex of Kaiyuan Group-complex. Dating the zircons from the dacite with schistosity is 2 506 Ma in method of U-Pb （SHRIMP）. This evidence indicates the rocks may be referred to Late Permian in age. Discovery of the rocks is significant to re-recognize stratigraphic property of ＂Liaohe Group＂, regional geoteetonie location and revolution of orogenic zone in Qinghe valley of the northern Liaoning.     

二郎坪群两点商议

二郎坪群的研究一直处于在不同认识的争论中，随着实际资料的积累，已逐步趋向一致。综合十多年来二郎坪群的不同认识，选择其中群的划分对比和大庙组的构造格局等两点再次提出商议。     

复州区金县群新观察

复州区金县群出露子复州城西瓦房、复州湾五行山和赵坎子地区。复州区金县群的剖面结构和地层特征和金州区金县群基本一致,其中十三里台组、马家屯组不仅岩性基本相同,而且含相同的叠层石组合,这表明复州—大连凹陷在晚先寒武纪时期为同一海盆地。复州区袁家沟—赵坎子一带缺失马家屯组以上沉积,寒武系大林子组直接覆于其上,表明复州湾区地壳曾一度抬升,出现了两凹夹一中隆的构造格局。     

熊耳群碲化物型金矿硫铅同位素及其成矿作用探讨

熊耳群火山岩中产出各种类型的金矿床，碲化物型（构造蚀变岩型）是金矿主要类型，该类型余矿以出现大量碲化物或富碲、硒为特征．硫化物δ￣（３４）Ｓ以较大的负值为特征，本文通过综合研究及与国内外行关矿床对比，认为该碲化物型金矿δ￣（３４）Ｓ负值的主要原因是地表水的渗透参与导致成矿热液物理化学条件改变，ｆｏ＿２升高、ｐＨ值降低，从而引起硫同位素强烈分馏形成的。有关铅同位素组成具深源壳幔混合（染）特征，显示成矿物质来源于熊耳群富钾火山岩系。该类型金矿床成矿作用为上升岩浆与下渗地表水共同作用形成浅成热液系统，在剪切带内氧化环境下液体的稀释和冷却是金沉淀的主要原因。其成因类型应属浅成低温热液富碲化物型金矿。     

Late superhumps and the stream–disc impact in IY UMa

We present two simple dynamical models for Sagittarius based on N -body simulations of the progressive disruption of a satellite galaxy orbiting for 12.5 Gyr within a realistic Galactic potential. In both models the satellite initially has observable properties similar to those of current outlying dwarfs; in one case it is purely stellar while in the other it is embedded in an extended massive halo. The purely stellar progenitor is a King model with a total velocity dispersion of 18.9 km s⁻¹, a core radius of 0.44 kpc and a tidal radius of 3 kpc. The initial stellar distribution in the other case follows a King profile with the same core radius, a slightly larger total velocity dispersion and similar extent. Both these models are consistent with all published data on the current Sagittarius system, they match not only the observed properties of the main body of Sagittarius, but also those reported for unbound debris at larger distances.     

Additional members of the local group of galaxies and quantized redshifts within the two nearest groups

Galaxies of redshiftz ≲ 1000 km s⁻¹ are investigated. In the South Galactic Hemisphere there are two large concentrations of these galaxies. One is in the direction of the centre of the Local Group, roughly aligned with M 31 and M 33. The other concentration is centred almost 80 degrees away on the sky and involves the next nearest galaxies to the Local Group, NGC 55, NGC 300 and NGC 253. The large scale and isolation of these concentrations, and the continuity of their redshifts require that they are all galaxies at the same, relatively close distance of the brightest group members. The fainter members of the group have higher redshifts, mimicking to some extent a Hubble relation. But if they are all at the same average distance the higher redshifts must be due to a cause other than velocity. The redshifts of the galaxies in the central areas of these groups all obey a quantization interval of δcz₀ = 72.4 kms⁻¹. This is the same quantization found by William Tifft, and later by others, in all physical groups and pairs which have been tested. The quantization discovered here, however, extends over a larger interval in redshift than heretofore encountered. The majority of redshifts used in the present analysis are accurate to ± 8 km s⁻¹. The deviation of those redshifts from multiples of 72.4 km s^-1 averages ±8.2 km s⁻¹. The astonishing result, however, is that for those redshifts which are known more accurately, the deviation from modulo 72.4 drops to a value between 3 and 4 km s⁻¹! The amount of relative velocity allowed these galaxies is therefore implied to be less than this extremely small value.