北京石花洞第四纪钟乳石剖面的年代学研究          下载免费PDF全文

吕金波赵树森  李铁英汪训一 李红春 《中国地质》2007,34(6):993-1002

北京石花洞位于房山花岗岩体边缘向形带的东北扬起端,与北京猿人遗址南北相望。地层为460Ma前形成的中奥陶统马家沟组石灰岩,洞穴大形态从25Ma前的上新世开始形成,洞内钟乳石从0.37Ma前的中更新世开始形成。在中国岩溶洞穴中,北京石花洞的层数最多,洞穴钟乳石种类齐全,裂隙渗透水沉积的石盾多、体积大,滴水沉积的石笋叠置关系明显,池水沉积的月奶石发育好,全新世石笋微层理发育清晰。该洞的大形态反映了北京西山新构造运动的期次,可以同华北地文期和永定河阶地对比,洞内钟乳石记录了中更新世以来北京西山古环境的变化,可以建立第四纪剖面,与周口店洞穴群碎屑沉积物剖面进行对比。钙板的铀系年龄为334.99～366.74ka,可定名钙板组。粗犷石笋的铀系年龄为169～235ka,粗犷石笋的电子自旋共振年龄为130～518ka,为中更新世沉积,可定名云水洞组。杆状石笋的铀系年龄为14.9±2.1～100.3±11.1ka,为晚更新世沉积,可定名石花洞组。在全新世石笋中,微层与微层之间存在厚约1μm的条带状纹线,是划分微层层数的标志,具有微层理的石笋14C年龄为为0.58～2.50ka,AMS14C年龄为为130±100～670±130a,可定名守备支洞组。  相似文献   

Dark haloes of spiral galaxies: ISO photometry     

Gerard Gilmore  & M. Unavane 《Monthly notices of the Royal Astronomical Society》1998,301(3):813-826

We exclude hydrogen-burning stars, of any mass above the hydrogen-burning limit and any metallicity, as significant contributors to the massive haloes deduced from rotation curves to dominate the outer parts of spiral galaxies. We present and analyse images of four nearly edge-on bulgeless spiral galaxies (UGC 711, NGC 2915, UGC 12426, UGC 1459) obtained with ISOCAM (The CAMera instrument on board the Infrared Space Observatory ) at 14.5 and 6.75 μm. Our sensitivity limit for detection of any diffuse infrared emission associated with the dark haloes in these galaxies is a few tens of μJy per 6 × 6 arcsec² pixel, with this limit currently set by remaining difficulties in modelling the non-linear behaviour of the detectors. All four galaxies show zero detected signal from extended non-disc emission, consistent with zero halo-like luminosity density distribution. The 95 per cent upper limit on any emission, for NGC 2915 in particular, allows us to exclude very low mass main-sequence stars ( M  > 0.08 M⊙) and young brown dwarfs (≲1 Gyr) as significant contributors to dark matter in galactic haloes. Combining our results with those of the Galactic microlensing surveys, which exclude objects with M  < 0.01 M⊙, excludes almost the entire possible mass range of compact baryonic objects from contributing to Galactic dark matter.  相似文献   

江西省小龙钨矿深部地球化学找矿远景预测   总被引：2，自引：0，他引：2  

张艳宜  吴泳生 《地质与勘探》1998,34(3):34-37

运用岩石地球化学找矿方法预测了小龙钨矿区深部Ｃｕ、Ａｇ、Ｗ矿化富集规律及其找矿远景。认为矿区南涪７、１１勘探线八中段以下存在Ｃｕ、Ａｇ、Ｗ矿体可能;北部０勘探线六中段Ｃｕ、Ａｇ晕已收敛,深部存在Ｃｕ、Ａｇ矿体可能性不大,而Ｗ的强度和规模在八中段以下呈显著增大趋势,深部可能存在Ｗ矿体,为矿区深部部署坑道工程提供了准确的地球化学依据。  相似文献   

山东新城金矿床的叠加晕模式   总被引：6，自引：0，他引：6  

李惠  张文华  刘宝林  李富国  王敬臣  赵可广 《地质找矿论丛》1998,13(1):1-12

１９８７年研究了Ⅰ号矿体地球化学异常特征,下部异常显示有深部盲矿前缘晕叠加,１９９４年探明的Ⅴ号矿体正好与其对应。１９９７年继续研究和建立了新城金矿的原生叠架晕模式,并用模式进行了预测。  相似文献   

The globular cluster system of the Sagittarius dwarf spheroidal galaxy: the age of Terzan 8     

Montegriffo  Bellazzini  Ferraro  Martins  Sarajedini  & Fusi Pecci 《Monthly notices of the Royal Astronomical Society》1998,294(2):315-326

We present deep V - and I -band CCD photometry of the globular cluster Terzan 8, recently found to be a member of the globular cluster system of the Sagittarius dwarf spheroidal galaxy. We accurately estimate the metallicity of Terzan 8, and provide the first direct determination of the colour excess toward this cluster. Our robust age estimate confirms that this cluster is indeed coeval with typical Galactic globulars of comparable metal content, and thus it is probably significantly older than at least two other Sagittarius clusters, Terzan 7 and Arp 2. The implications of this result on the star formation history of the Sagittarius galaxy are briefly discussed.  相似文献   

上置晕与物质的“类气相”垂向迁移   总被引：19，自引：1，他引：18  

吴传璧  施俊法 《地学前缘》1998,5(2):185-194

阐明了上置晕的术语概念,指出文献中术语运用的失当之处,归纳出以上置晕为基础的各类隐伏矿化探方法。按传统的观念,上置晕主要是由不同形式的水迁移作用造成的。地气法、ＭＦＥ法和离子晕法的出现,揭示出在覆盖层中存在着一种新的元素迁移机制,即元素以非常细小的固相微粒随地气流迁移。一系列实验和实测结果表明,这种固相微粒可能是纳米粒径的物质,它们具有类气相的性状,故可将这种迁移机制称为物质的类气相垂向迁移。这一机制可以说明按传统机制难以解释的现象,对相应化探方法的研制、改善和应用有理论和实践上的指导意义。  相似文献   

浅析四道沟金矿矿床成因及找矿方向     

鲍玉学  孙立民  黄俊鹏 《国土资源》1999,(3)

四道沟金矿是地质条件较为复杂的矿床，对其成因问题前人观点众说不一。比较典型的主要有岩浆热液成因和沉积变质成因，成因不同直接影响着找矿方向。根据矿床地质特征和工作实践认为：该矿床成因应为沉积变质－ 岩浆热液叠加改造型矿床。所以沉积变质和岩浆热液成矿的有利条件均应成为找矿的主要方向。据此开展的找矿工作已初步获得突破性进展。  相似文献   

The effect of heterogeneous stress and strain on metamorphic fluid flow,Mary Kathleen,Australia, and a model for large-scale fluid circulation *     

N. H. S. OLIVER  R. K. VALENTA  V. J. WALL 《Journal of Metamorphic Geology》1990,8(3):311-331

In the Proterozoic Mary Kathleen Fold Belt, northern Australia, infiltration of large volumes of externally derived fluid occurred synchronously with regional amphibolite-facies metamorphism and deformation. This paper develops a model of structurally controlled fluid migration by comparing the distribution of fossil fluid pathways with the inferred stress and strain patterns during the deformation. Intense fluid flow was localized within strong, relatively brittle meta-intrusive bodies, and in discrete, veined, brecciated and altered zones around their margins. In metasediments folded in a ductile manner outside these areas, fluid infiltration was negligible. The direct correlation between structural styles and the magnitude of veining and metasomatism suggests control of permeability enhancement, and hence fluid flow, by deformation. Finite difference modelling of a strong body in a weaker matrix has been used to evaluate the variation of stresses during the deformation, from which it is clear that stress and strain heterogeneities have systematically influenced the development and maintenance of metamorphic fluid pathways. Particular regions in which mean stress may be significantly lower than the average lithostatic pressures include the ‘strain shadow’zones adjacent to the strong bodies, other dilatant zones around the bodies, and the bodies themselves. This geometry is favourable not only for localized brittle deformation under amphilobite facies conditions, but also for focused fluid flow in the low mean stress regions, as evidenced by the abundance of veins. Fluid access through these metamorphic aquifers occurred during tensile failure episodes, with particularly large dilations and decimetre-scale veining in areas of strain incompatibility. It appears likely that fluid circulated many times through the Fold Belt, with flow concentrated in the metamorphic aquifers. A model is developed that explains both the structurally focused fluid flow and the postulated multi-pass recirculation by dilatancy pumping, the ‘pump engines’comprising the low mean stress zones.  相似文献   

Numerical studies on the structure of the cosmic ray electron halo in starburst galaxies     

Shoko Miyake  Shohei Yanagita  Tatsuo Yoshida 《Astrophysics and Space Science》2007,309(1-4):151-155

The structure of the cosmic ray electron halo of a starburst galaxy depends strongly on the nature of galactic wind and the configuration of the magnetic field. We have investigated these dependencies by solving numerically the propagation of electrons originating in starburst galaxies, most likely in supernova remnants. The calculations are made for several models for the galactic winds and for the configuration of the magnetic fields for comparison with observations. Our simulation of a quasi-radio halo reproduces both the extended structure of ∼9 kpc and the subtle hollow structure near the polar region of the radio halo that are observed in the starburst galaxy NGC 253. These findings suggest the existence of strong galactic wind in NGC 253.   相似文献   

Distribution of Palaeozoic tectonic superimposed unconformities in the Tarim Basin,NW China: significance for the evolution of palaeogeomorphology and sedimentary response     

Hao Liu  Ian D. Somerville  Changsong Lin  Shengjie Zuo 《Geological Journal》2016,51(4):627-651

Seismic and drilling well data were used to examine the occurrence of multiple stratigraphic unconformities in the Tarim Basin, NW China. The Early Cambrian, the Late Ordovician and the late Middle Devonian unconformities constitute three important tectonic sequence boundaries within the Palaeozoic succession. In the Tazhong, Tabei, Tadong uplifts and the southwestern Tarim palaeo‐uplift, unconformities obviously belong to superimposed unconformities. A superimposed unconformity is formed by superimposition of unconformities of multiple periods. Areas where superimposed unconformities develop are shown as composite belts of multiple tectonic unconformities, and as higher uplift areas of palaeo‐uplifts in palaeogeomorphologic units. The contact relationship of unconformities in the lower uplift areas is indicative of truncation‐overlap. A slope belt is located below the uplift areas, and the main and secondary unconformities are characterized by local onlap reflection on seismic profiles. The regional dynamics controlled the palaeotectonic setting of the Palaeozoic rocks in the Tarim Basin and the origin and evolution of the basin constrained deposition. From the Sinian to the Cambrian, the Tarim landmass and its surrounding areas belonged to an extensional tectonic setting. Since the Late Ordovician, the neighbouring north Kunlun Ocean and Altyn Ocean was transformed from a spreading ocean basin to a closed compressional setting. The maximum compression was attained in the Late Ordovician. The formation of a tectonic palaeogeomorphologic evolution succession from a cratonic margin aulacogen depression to a peripheral foreland basin in the Early Caledonian cycle controlled the deposition of platform, platform margin, and deep‐water basin. Tectonic uplift during the Late Ordovician resulted in a shallower basin which was followed by substantial erosion. Subsequently, a cratonic depression and peripheral or back‐arc foreland basin began their development in the Silurian to Early–Middle Devonian interval. In this period, the Tabei Uplift, the Northern Depression and the southern Tarim palaeo‐uplift showed obvious control on depositional systems, including onshore slope, shelf and deep‐water basin. The southern Tarim Plate was in a continuous continental compressional setting after collision, whereas the southern Tianshan Ocean began to close in the Early Ordovician and was completely closed by the Middle Devonian. At the same time, further compression from peripheral tectonic units in the eastern and southern parts of the Tarim Basin led to the expansion of palaeo‐uplift in the Late Devonian–Early Carboniferous interval, and the connection of the Tabei Uplift and Tadong Uplift, thus controlling onshore, fluvial delta, clastic coast, lagoon‐bay and shallow marine deposition. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献