麻江古油藏油源识别与油气运聚分析：来自油气地球化学的证据   总被引：1，自引：1，他引：0       下载免费PDF全文

杨平  汪正江  印峰 刘家洪  林家善  张娣  黄学平 《中国地质》2014,41(3):982-994

充分考虑热演化过程中烃源岩干酪根、族组分、固体沥青及正构烷烃碳同位素相互关系及变化规律,通过地球化学分析并结合前人碳同位素及芳烃标志物研究进行综合分析,结果表明古油藏各区域储层早期均存在下寒武统黑色泥岩来源,后期来源有较大差别,麻江古背斜以南各地沥青均不同程度与中寒武统都柳江组有关,北凯里液态原油及油苗为五峰组及龙马溪组印支期成藏产物,其保存环境为储层早期成岩过程中形成的独立封闭系统。在油源识别的基础上,结合构造地质背景、油气成藏条件及流体活动规律分析,认为黔南坳陷及邻区下寒武统、都柳江组、五峰组及龙马溪组烃源岩的分布控制了该区油气富集规律,黔南海西期断裂系统与加里东运动形成的不整合面构成不同期次油气运聚的输导系统,海西期形成的一系列正断裂是麻江古油藏成藏的关键。  相似文献   

The Solid-liquid Transformation of Low-grade Solid Potash Deposit in Dalangtan Basin and the Simplification of the Liquid Phase System     

WANG Xiaohan  ZHANG Chao  XIE Shaolei  JIA Yongzhong  YAO Ying 《《地质学报》英文版》2014,88(Z1):436-436

正We studied the solid-liquid transformation of low-grade solid potash deposit in Dalangtan Basin and simplified the liquid phase system.We did experiments to optimize conditions of the solid-liquid transformation.The Suitable  相似文献   

卡塔克隆起中1井储层沥青地球化学特征与成因   总被引：1，自引：0，他引：1  

唐友军  王铁冠  钱一雄 《沉积学报》2007,25(4):640-645

塔里木盆地海相原油的成因至今仍有争议,而对储层沥青的地球化学特征剖析,能为探索海相原油的成因提供依据。选取卡塔克隆起上的中1井不同层系储层沥青,详尽剖析了其地球化学特征。研究结果揭示,中1井储层沥青的Pr/Ph为1.14～1.39,CPI值 1.01～1.08,OEP值0.98～1.05,无奇偶优势或偶奇优势,伽玛蜡烷、C28甾烷丰度低,硫芴系列丰富。甾烷成熟度参数和Ts/(Ts+Tm)均指示中1井储层沥青处于成熟—高成熟热演化范畴。依据特征生物标志物的分布对沥青的成因示踪,中1井储层沥青与上奥陶统烃源岩有成因关系,而中1井储层沥青与塔东2井寒武系原油分子特征的迥异也佐证该认识。  相似文献   

The Petrology and Mineralogy Analysis of Noble Metal Alloys in the Inclusions of a Chondrite: An Implication on the Evolution of the Solar Nebula     

WU Yun-hua  XING Wei-fan  XU WEi-biao 《Chinese Astronomy and Astrophysics》2014

The calcium-aluminium-rich inclusions (CAIs) in chondrites are believed to be the most early solids formed in the solar system, and retain the original information of the early solar nebula. However, in-depth researches revealed that most inclusions had experienced a complex history of evolution, including partial melting and secondary alteration. Focused on the refractory and chemically stable noble metal particles in the CAI of a CV meteorite (NWA 2140), a study of astrochemistry is made in this paper. The petrology and mineralogy analysis as well as the composition determination have been made on the noble metal particles. Based on the result of composition analysis, the thermodynamic process experienced by the CAI is inferred, and two kinds of noble metal alloys are identified, which correspond to the early-stage condensation products and the secondary alteration products of primordial metals, respectively.  相似文献   

The effect of a dense atmosphere on the tidally induced potential of Titan     

Özgür Karatekin  Tim Van Hoolst 《Icarus》2006,183(1):230-232

The effect of the dense atmosphere of Titan on the tidal variations of the external gravitational potential of degree two is quantified. The atmospheric tides perturb the external gravitational potential of Titan in two ways. First, the atmosphere itself contributes directly to the external gravitational potential with a period of 15.945 days. Second, the variable loading of the atmosphere induces mass redistribution within Titan, which also changes the external gravitational potential. It is shown that the relative atmospheric contributions to the tides are most likely less than 2% and vanish almost completely for the most plausible models with a subsurface ocean. This suggest that atmospheric tidal perturbations will contribute only negligibly to Cassini measurements of Titan's gravitational field so that the tidal Love numbers derived from these observations can be directly interpreted in terms of the satellite's interior.  相似文献   

Propagation of elastic waves in a cylindrical bore in a liquidsaturated porous solid     

M. D. Sharma  M. L. Gogna 《Geophysical Journal International》1990,103(1):47-54

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Comment on the paper “Fast tidal cycling and the origin of life” by Richard Lathe     

P. Varga  K.R. Rybicki 《Icarus》2006,180(1):274-276

We show that the fast tidal cycling postulated by Lathe [Lathe, R., 2004. Icarus 168, 18-22] is not a plausible mechanism to explain the origin of life on Earth about 3.9 Ga ago. The value of LOD at this remote epoch was probably comprised between 15 to 17 h, and the Earth-Moon distance was only about 20% smaller than nowadays, implying that the tidal frequencies and amplitudes were not so dramatically different from the present ones as stated in Lathe's paper.  相似文献   

Dehydration melting of solid amphibolite at 2.0 GPa: Effects of time and temperature   总被引：3，自引：0，他引：3  

ZHOU Wenge  XIE Hongsen  LIU Yonggang  ZHENG Xiaogang  ZHAO Zhidan & ZHOU Hui . Laboratory of Material in the Earth’s Interior  Institute of Geochemistry  Chinese Academy of Sciences  Guiyang  China  . Department of Geology  China University of Geosciences  Beijing  China  . Department of Geology  Peking University  Beijing  China 《中国科学D辑(英文版)》2005,48(8):1120-1133

The dehydration melting of the natural rock at high pressure is important to investigating the magma formation in the earth’s interior. Since the 1970s, a lot of geological scientists have paid more atten- tion to the dehydration melting of the natural rock[1―5]. Previous experiments of dehydration melting and observations of fieldwork argued that the dehy- dration melting of the rock was probably the most important fashion for the melting of the lower crust rock[6―12]. The genesis of most …  相似文献   

The influence of obliquity on europan cycloid formation     

T.A. Hurford  A.R. Sarid  B.G. Bills 《Icarus》2009,202(1):197-215

Tectonic patterns on Europa are influenced by tidal stress. An important well-recognized component is associated with the orbital eccentricity, which produces a diurnally varying stress as Jupiter's apparent position in Europa's sky oscillates in longitude. Cycloidal lineaments seem to have formed as cracks propagated in this diurnally varying stress field. Maps of theoretical cycloid patterns capture many of the characteristics of the observed distribution on Europa. However, a few details of the observed cycloid distribution have not been reproduced by previous models. Recently, it has been shown that Europa has a finite forced obliquity, so Jupiter's apparent position in Europa's sky will also oscillate in latitude. We explore this new type of diurnal effect on cycloid formation. We find that stress from obliquity may be the key to explaining several characteristics of observed cycloids such as the shape of equator-crossing cycloids and the shift in the crack patterns in the Argadnel Regio region. All of these improvements of the fit between observation and theory seem to require Jupiter crossing Europa's equatorial plane 45° to 180° after perijove passage, suggestive of complex orbital dynamics that locks the direction of Europa's pericenter with the direction of the ascending node at the time these cycloids were formed.  相似文献   

The interior structure of Mercury and its core sulfur content     

A. Rivoldini  T. Van Hoolst  O. Verhoeven 《Icarus》2009,201(1):12-30

Depth-dependent interior structure models of Mercury are calculated for several plausible chemical compositions of the core and of the mantle. For those models, we compute the associated libration amplitude, obliquity, tidal deformation, and tidal changes in the external potential. In particular we study the relation between the interior structure parameters for five different mantle mineralogies and two different temperature profiles together with two extreme crust density values. We investigate the influence of the core light element concentration, temperature, and melting law on core state and inner and outer core size. We show that a sulfur concentration above 10 wt% is unlikely if the temperature at the core-mantle boundary is above 1850 K and the silicate shell at least 240 km thick. The interior models can only have an inner core if the sulfur weight fraction is below 5 wt% for core-mantle boundary temperature in the 1850-2200 K range. Within our modeling hypotheses, we show that with the expected precision on the moment of inertia the core size can be estimated to a precision of about 50 km and the core sulfur concentration with an error of about 2 wt%. This uncertainty can only be reduced when more information on the mantle mineralogy of Mercury becomes available. However, we show that the uncertainty on the core size estimation can be greatly reduced, to about 25 km, if tidal surface displacements and tidal variations in the external potential are considered.  相似文献