EURONEAR—Recovery, follow-up and discovery of NEAs and MBAs using large field 1–2 m telescopes     

O. Vaduvescu  M. Birlan  A. Tudorica  A. Sonka  F.N. Pozo  A.D. Barr  D.J. Asher  J. Licandro  J.L. Ortiz  E. Unda-Sanzana  M. Popescu  A. Nedelcu  D. Dumitru  R. Toma  I. Comsa  C. Vancea  D. Vidican  C. Opriseanu  T. Badescu  M. Badea  M. Constantinescu 《Planetary and Space Science》2011,59(13):1632-1646

We report on the follow-up and recovery of 100 program NEAs, PHAs and VIs using the ESO/MPG 2.2 m, Swope 1 m and INT 2.5 m telescopes equipped with large field cameras. The 127 fields observed during 11 nights covered 29 square degrees. Using these data, we present the incidental survey work which includes 558 known MBAs and 628 unknown moving objects mostly consistent with MBAs from which 58 objects became official discoveries. We planned the runs using six criteria and four servers which focus mostly on faint and poorly observed objects in need of confirmation, follow-up and recovery. We followed 62 faint NEAs within one month after discovery and we recovered 10 faint NEAs having big uncertainties at their second or later opposition. Using the INT we eliminated four PHA candidates and VIs. We observed in total 1286 moving objects and we reported more than 10,000 positions. All data were reduced by the members of our network in a team effort, and reported promptly to the MPC. The positions of the program NEAs were published in 27 MPC and MPEC references and used to improve their orbits. The O−C residuals for known MBAs and program NEAs are smallest for the ESO/MPG and Swope and about four times larger for the INT whose field is more distorted. For the astrometric reduction, the UCAC-2 catalog is recommended instead of USNO-B1. The incidental survey allowed us to study statistics of the MBA and NEA populations observable today with 1–2 m facilities. We calculate preliminary orbits for all unknown objects, classifying them as official discoveries, later identifications and unknown outstanding objects. The orbital elements a, e, i calculated by FIND_ORB software for the official discoveries and later identified objects are very similar with the published elements which take into account longer observational arcs; thus preliminary orbits were used in statistics for the whole unknown dataset. We present a basic model which can be used to distinguish between MBAs and potential NEAs in any sky survey. Based on three evaluation methods, most of our unknown objects are consistent with MBAs, while up to 16 unknown objects could represent NEO candidates and four represent our best NEO candidates. We assessed the observability of the unknown MBA and NEA populations using 1 and 2 m surveys. Employing a 1 m facility, one can observe today fewer unknown objects than known MBAs and very few new NEOs. Using a 2 m facility, a slightly larger number of unknown than known asteroids could be detected in the main belt. Between 0.1 and 0.8 new NEO candidates per square degree could be discovered using a 2 m telescope.  相似文献   

Mafic dykes derived from Early Cretaceous depleted mantle beneath the Dabie orogenic belt: implications for changing lithosphere mantle beneath Eastern China     

Ling Chen  Chang Q. Ma  Jin Y. Zhang  Roger Mason  Chao Zhang 《Geological Journal》2011,46(4):333-343

SHRIMP zircon U–Pb geochronological, elemental and Sr–Nd isotopic data from Early Cretaceous mafic dykes in North Dabie orogenic belt elucidate a change of Mesozoic lithospheric mantle in eastern China. The dykes are predominantly dolerite with the major mineral assemblage clinopyroxene + hornblende + plagioclase and yield a SHRIMP zircon U–Pb age of 111.6 ± 5.3 Ma. They have a narrow range of SiO₂ from 46.16% to 49.78%, and relative low concentrations of K₂O (1.07−2.62%), Na₂O (2.45−3.54%), Al₂O₃ (13.04−14.07%), and P₂O₅ (0.42−0.55%) but relatively high concentration of MgO (5.94–6.61%) with Mg^# 52–54. All the samples are characterized by enrichment of large ion lithophile elements (LILE, e.g., Ba, Th) and high field strength elements (HFSE, e.g., Nb, Ti). (⁸⁷Sr/⁸⁶Sr)_i ratios from 0.704 to 0.705, ε_Nd values from 3.36 to 4.33 and mantle‐depletion Nd model ages (T_2DM) in the range 0.56–0.64 Ga indicate that the magma of the Baiyashan mafic dykes was derived from a young depleted mantle source. This finding is different from previous research on mafic dykes in the age range 120–138 Ma that revealed enrichment of LILE and depletion of HFSE, high initial Sr isotopic ratios and negative ε_Nd, value which represents an old enriched mantle source. Ours is the first report of the existence of Early Cretaceous depleted mantle in eastern China and it implies that changing of enriched mantle to depleted mantle occurred at ca. 112 Ma, associated with back‐arc extension which resulted from the subduction of the Palaeo‐Pacific Plate towards the Asian Continent. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   

百58井区地震数据高分辨率成像与断裂带构造特征     

赵玉莲  李录明  王海燕  胡自多  马建华  李斐 《吉林大学学报(地球科学版)》2011,41(4):1219-1225

准噶尔盆地西北缘百口泉地区百58井区是一个被多条断裂切割的复杂断块区,地层倾角变化大;现有的三维地震资料成果剖面上地震波组连续性差,断裂带附近资料成像模糊,地层接触关系不清楚,很难进行精细构造解释。为获得研究区沉积盖层精细结构,在详细分析原始地震资料特点和存在问题的基础上,有针对性地采用叠前多域去噪和非线性叠前时间偏移等多种处理技术,对已有的三维地震资料进行了高分辨率精细成像处理。新的成果剖面揭示出该区百－乌断裂带发育特征、空间展布及平面组合关系。根据地层厚度、构造特征、地震反射波组特征等,划分该区地层为二叠系、三叠系、侏罗系－白垩系三大构造层,以三大构造层不同的构造特征为依据确定了研究区分为西部推覆构造带、中部断阶构造带和东部斜坡构造带3个构造单元。  相似文献   

An Overview on the Composition and Age of Upper Crust of Proto-Tethyan Lajishan Intra-oceanic Arc, NE Tibet Plateau     

FU Changlei  HE Xiaohu  YAN Zhen  Jonathan C. AITCHISON  XIAO Wenjiao  WANG Bingzhang  LI Wufu  LI Yusen 《《地质学报》英文版》2024,98(2):285-302

Identification and anatomy of oceanic arcs within ancient orogenic belt are significant for better understanding the tectonic framework and closure process of paleo-ocean basin. This article summarizes the geological, geochemical, and geochronological characteristics of upper crust of Proto-Tethyan Lajishan intra-oceanic arc and provides new data to constrain the subduction evolution of the South Qilian Ocean. The intra-oceanic arc volcanic rocks, including intermediate–mafic lava, breccia, tuff, and minor felsic rocks, are distributed along southern part of the Lajishan ophiolite belt. Geochemical and isotopic compositions indicate that the intermediate–mafic lava were originated from depleted mantle contaminated by sediment melts or hydrous fluids, whereas the felsic rocks were likely generated by partial melting of juvenile mafic crust in intra-oceanic arc setting. Zircons from felsic rocks yield consistent and concordant ages ranging from 506 to 523 Ma, suggesting these volcanic rocks represent the relicts of upper crust of the Cambrian intra-oceanic arc. Combined with the Cambrian forearc ophiolite and accretionary complex, we suggest that the Cambrian intra-oceanic arc in the Lajishan ophiolite belt is belonging to the intra-oceanic arc system which was generated by south-directed subduction in the South Qilian Ocean at a relatively short interval between approximately 530 and 480 Ma.  相似文献   

武夷山成矿带及邻区上地幔速度结构及其对燕山期岩浆-成矿活动的启示     

徐峣  张永谦  严加永  徐志伍  陈淼  王栩  陈昌昕  张文文 《岩石学报》2022,38(2):529-543

武夷山成矿带燕山期岩浆-成矿活动的深部动力学机制一直是学者们研究的热点.已有的研究结果表明,武夷山成矿带及邻区的上地幔存在着显著的低速异常,可能与地表的岩浆-成矿活动存在着密切的联系.本研究利用分布在华夏地块98个固定地震台站以及59个流动地震台站所记录到的278个远震事件,采用远震层析成像方法构建了武夷山成矿带及邻区...  相似文献   

华北板块北缘东段中元古代造山带地质特征及构造演化     

刘锦  李东涛  蒯兵  李玉超  彭游博  赵辰  杨仲杰  刘文彬 《地质与资源》2013,22(6):435-443

研究区内的中元古代魏家沟岩群原岩为一套碳酸盐岩、陆缘碎屑岩及火山岩建造,形成于大陆裂谷-活动大陆边缘阶段,并于1036 Ma左右遭受变质变形.通过岩浆岩形成构造环境的判别,研究区中元古代岩浆活动贯穿于板块碰撞前、同碰撞及碰撞后.伴随着造山带的演化,本区中元古代经历了3期韧性变形,分别形成于大陆裂谷、活动大陆边缘及碰撞造山阶段.通过上述研究,确定了本区中元古代造山带的存在,并经历了大陆裂谷-被动大陆边缘-活动大陆边缘-碰撞造山的地质演化过程,证实了格林维尔造山运动在华北板块北缘的存在和对中元古代末期Rodinia超大陆拼合的响应.  相似文献   

青海省都兰县果洛龙洼金矿成矿流体   总被引：2，自引：0，他引：2  

丁清峰  金圣凯  王冠  张本龙 《吉林大学学报(地球科学版)》2013,43(2):415-426

果洛龙洼金矿是青海东昆仑地区最典型、最具规模的金矿床之一。在前人资料基础上,将果洛龙洼金矿热液成矿期划分为4个成矿阶段：贫矿化石英阶段、石英-多金属硫化物阶段（主要成矿阶段）、石英-贫硫化物阶段（次要成矿阶段）和石英-碳酸盐阶段。随后对主要和次要成矿阶段石英脉开展流体包裹体显微测温和H-O同位素研究。结果表明：原生流体包裹体主要包括气液两相、富CO₂三相、纯CO₂两相共3类;成矿流体总体以CO₂-NaCl-H₂O体系为主,均一温度为130.0~357.3 ℃,盐度（w(NaCl)）为1.83%~20.11%。石英-多金属硫化物阶段石英δ¹⁸O_V-SMOW值为14.8‰~17.2‰,据此计算流体的δ¹⁸O_H2O值为5.5‰~8.5‰,流体的δD_V-SMOW值为-61‰~-96‰;而石英-贫硫化物阶段石英δ¹⁸O_V-SMOW值为15.7‰~16.9‰,据此计算流体的δ¹⁸O_H2O值为4.1‰~5.3‰,流体的δD_V-SMOW值为-84‰~-101‰。由此认为：主要成矿阶段成矿流体可能为高温低盐度富CO₂变质热液和低温中高盐度岩浆热液两个端元组成的混合流体;次要成矿阶段成矿流体主要为混合后更均匀的中低温中低盐度热液,但后期明显有大气降水混入。总之,成矿流体的来源、性质及其演化等方面的研究结果进一步证明果洛龙洼金矿为造山型金矿。  相似文献   

南天山库车褶皱-冲断带喀拉玉尔滚构造带新生代变形特征及其控制因素   总被引：1，自引：0，他引：1  

李世琴  唐鹏程  饶刚 《地球科学》2013,38(4):859-869

喀拉玉尔滚构造带是南天山库车褶皱-冲断带的变形前缘, 其地下深层变形特征仍然不清楚.结合野外地质调查结果、数字高程模型数据、钻井数据和高品质二维地震反射剖面, 厘定喀拉玉尔滚构造带背斜的平面展布、几何学和运动学特征及变形时间, 并结合前人研究成果探讨喀拉玉尔滚构造带新生代变形控制因素.喀拉玉尔滚构造带为典型的挤压构造带, 近EW向延伸约165km, 由一系列带状背斜组成, 且背斜核部发育多条隐伏逆冲断层.喀拉玉尔滚构造带新生代变形特征主要表现为5个方面: (1)北喀背斜为盐枕构造; (2)中喀背斜和南喀背斜的几何形态不对称、背斜倾伏方向相反, 分别为向北和向南, 二者交汇处发生了位移转换; (3)羊塔克背斜和英买力背斜为基本对称的低幅度滑脱褶皱; (4)背斜幅度整体上从西往东逐渐降低; (5)背斜变形时间从西往东逐渐变新.研究结果表明, 喀拉玉尔滚构造带新生代变形主要受区域挤压作用、盐层和基底构造共同控制.   相似文献   

桂东大瑶山成矿带新坪矿区花岗斑岩与金多金属成矿作用关系   总被引：1，自引：0，他引：1  

王新宇  刘名朝  周国发  黄锡强  王瑞湖 《现代地质》2013,27(3):585-592

新坪花岗斑岩位于桂东大瑶山成矿带中部新坪金矿区内。在野外地质观察的基础上,报道了在该新坪斑岩体接触带附近发现金矿体并首次在岩体内部发现石英脉型辉钼矿(化)体,认为新坪花岗斑岩体与金多金属矿化关系密切。新坪花岗斑岩LA-ICP-MS锆石U-Pb同位素定年结果表明,该斑岩体形成于早古生代奥陶纪(462.9±6.4) Ma,属加里东期花岗岩类,因此与岩体有关的金矿化、铜钼矿化时间不会早于奥陶纪。岩体稀土元素分析结果显示,新坪花岗斑岩与邻近的古袍、圆珠顶、大黎矿区花岗斑岩体具有相似的稀土元素分布特征,可能为同源岩浆不同阶段的演化产物,说明新坪花岗斑岩体具有一定的金、钼等多金属成矿潜力。通过以上综合研究分析,初步认为新坪矿区具有寻找斑岩型金矿以及钼矿床的找矿前景。  相似文献   

中国大陆与各活动地块、南北地震带实测应力特征分析   总被引：16，自引：3，他引：13  

杨树新  姚瑞  崔效锋  陈群策  黄禄渊 《地球物理学报》2012,55(12):4207-4217

本文以"中国大陆地壳应力环境基础数据库"为基础,补充了迄今为止查阅到的中国大陆水压致裂法与应力解除法的实测地应力数据,在1474个测点上得到3586条数据,研究区经度范围75°E－130°E,纬度范围18°N－47°N,深度范围0~4000 m,基本覆盖了中国大陆的各活动地块与南北地震带各段等研究区.本文采用等深度段分组归纳的方法解决了实测地应力数据样本数量沿深度分布的不均匀问题,给出了中国大陆与各研究区地壳浅层测量深度范围内应力量值、方位特征.结果显示:(1)中国大陆地壳浅层最大水平应力、最小水平应力、垂直应力随深度呈线性增加;(2)中国大陆地区侧压系数随深度的变化特征为:浅部离散,随着深度增加而集中,并趋向0.68,D=465 m是水平作用为主导向垂直作用为主导的转换深度,K_av=1;(3)中国大陆水平差应力在地表为3 MPa左右,随深度增加以5.8 MPa/km的梯度增大;(4)在测量深度范围内,中国大陆各研究区最大水平应力中间值(深度为2000 m时的统计回归值)从大到小的顺序是:青藏地块63.6 MPa、南北带北段57.3 MPa、华南地块51.4 MPa、华北地块50.5 MPa、南北带中段47.9 MPa、西域地块47.5 MPa、南北带南段45.4 MPa、东北地块44.8 MPa,总体表现为"西强东弱"的基本特征,反映了印度板块与欧亚板块的强烈碰撞是中国大陆构造应力场强度总体特征的主要来源;(5)与其他研究区相比较,青藏地块地壳在从南向北的挤压作用下呈现出明显的"浅弱深强"特点;(6)最大水平应力方向的总体特征,基本以青藏高原为中心,呈辐射状展布,由西向东,从近N-S方向逐步顺时针旋转至NNE-SSW、NE-SW、NEE-SWW、NW-SE方向,与深部的震源机制解研究结果有一致性.  相似文献