A rotational light curve for the Kuiper belt object 1997 CV29

We present R- and V-band rotational light curves for classical Kuiper belt object 1997 CV₂₉. The imaging data was obtained from the Canada-France-Hawaii Telescope (CFHT) archive located at the Canadian Astronomical Data Center (CADC). The data consist of one nights observations of a series of 42, 8 minute exposures in R band followed by 33, 8 minute exposures in V band acquired on the following night. Using relative photometry we determined a highly significant variation in the brightness of 1997 CV₂₉. Using phase-dispersion-minimization we find 8.0, 11.2, and 15.8 hrs to be the most likely, periods of rotation and we argue that the ∼16 hr period is the most likely based on our limited observing window. The phased light curve has a peak-to-peak range of Δm?0.4±0.1 mag suggesting an axial ratio of a/b?1.45.     

Diverse albedos of small trans-neptunian objects

Discovery of trans-neptunian object (TNO) satellites and determination of their orbits has recently enabled estimation of the size and albedo of several small TNOs, extending the size range of objects having known size and albedo down into the sub-100 km range. In this paper we compute albedo and size estimates or limits for 20 TNOs, using a consistent method for all binary objects and a consistent method for all objects having reported thermal fluxes. As is true for larger TNOs, the small objects show a remarkable diversity of albedos. Although the sample is limited, there do not yet appear to be any trends relating albedo to other observable properties or to dynamical class, with the possible exception of inclination. The observed albedo diversity of TNOs has important implications for computing the size-frequency distribution, the mass, and other global properties of the Kuiper belt derived from observations of objects' apparent magnitudes and may also point the way toward an improved compositional taxonomy based on albedo in addition to color.     

胶南-威海造山带与罗迪尼亚(Rodinia)超大陆相关问题的初步探讨

胶南-威海造山带中的榴辉岩为晋宁早期板块俯冲作用的产物;沿造山带广泛分布的花岗质片麻岩,则为晋宁晚期板块由俯冲转为碰撞过程中同造山岩浆事件的产物.它们与全球性的格林威尔造山运动属同一事件范畴,但具有明显的穿时性.侵入于同造山花岗质片麻岩的片麻状花岗岩及震旦纪朋河石组,为后造山伸展机制下发生的岩浆及沉积事件的产物,与700～650Ma期间Rodinia超大陆的裂解作用密切相关.     

Lamproitic Rocks from a Continental Collision Zone: Evidence for Recycling of Subducted Tethyan Oceanic Sediments in the Mantle Beneath Southern Tibet

Major and trace element, Sr–Nd–Pb isotope and mineralchemical data are presented for newly discovered ultrapotassiclavas in the Tangra Yumco–Xuruco graben in southern Tibet.The ultrapotassic lavas are characterized by high MgO, K₂O andTiO₂, low Al₂O₃ and Na₂O contents, and also have high molarK₂O/Al₂O₃, molar (K₂O + Na₂O)/Al₂O₃ and K₂O/Na₂O ratios. Theirhigh abundances of incompatible trace elements such as largeion lithophile elements (LILE) and light rare earth elements(LREE) reach the extreme levels typical of lamproites. The lamproitesshow highly radiogenic ⁸⁷Sr/⁸⁶Sr (0· 7166–0·7363) and unradiogenic ¹⁴³Nd/¹⁴⁴Nd (0· 511796–0·511962), low ²⁰⁶Pb/²⁰⁴Pb (18· 459–18· 931),and elevated radiogenic ²⁰⁷Pb/²⁰⁴Pb (15· 6732–15·841) and ²⁰⁸Pb/²⁰⁴Pb (39· 557–40· 058) ratios.On the basis of their geochemical and isotopic systematics,the lamproites in south Tibet have a distinct magma source thatcan be differentiated from the sources of potassic lavas inthe east Lhasa and Qiangtang blocks. Their high Nb/Ta ratios(17· 10–19· 84), extremely high Th/U ratios(5· 70–13· 74) and distinctive isotope compositionsare compatible with a veined mantle source consisting of partialmelts of subducted Tethyan oceanic sediments and sub-continentallithospheric depleted mantle. Identification of the lamproitesand the delineation of their mantle source provide new evidencerelevant for models of the uplift and extension of the Tibetanplateau following the Indo-Asia collision. Metasomatism by partialmelts from isotopically evolved, old sediment subducted on theyoung Tethyan slab is an alternative explanation for PrecambrianNd and Pb model ages. In this model, differences in isotopiccomposition along-strike are attributed to differences in thetype of sediment being subducted, thus obviating the need formultiple metasomatic events over hundreds of million years.The distribution of lamproites, restricted within a north–south-trendinggraben, indicates that the initiation of east–west extensionin south Tibet started at 25 Ma. KEY WORDS: lamproites; subducted oceanic sediment; Tibetan active continental collision belt     

赣西石竹山硅灰石矿床石榴子石特征及其地质意义

江西省石竹山硅灰石矿床位于钦杭成矿带东段的萍乐坳陷带内,是世界资源储量规模最大的硅灰石矿床。为了厘清区内成矿流体性质及进一步找矿潜力,本文根据矿物间的穿插关系和光学特征,将该矿床的石榴子石分为早(GrtⅠ)、晚(GrtⅡ)两个世代,在详细的野外工作基础上,利用电子探针(EMPA)和LA-ICP-MS原位微区分析技术,对石竹山矿床中的石榴子石开展了系统研究。结果表明,石竹山硅灰石矿床石榴子石属于钙铝榴石-钙铁榴石固溶体系列,早期形成的石榴子石(GrtⅠ)Fe含量更高,且震荡环带发育,而晚期形成的石榴子石(GrtⅡ)则发育复杂环带。石榴子石GrtⅠ和GrtⅡ都亏损大离子亲石元素K、Rb、Ba、Sr等,而Nb、Ta、Zr等高场强元素相对含量较高,U含量与∑REE成正比。GrtⅡ的∑REE较低(12.92×10^-6~21.12×10^-6),具有较平坦的稀土元素配分模式,轻微富集轻稀土元素(Ce、Pr、Nd、Sm),微弱负铕异常;GrtⅠ的∑REE相对较高(13.78×10^-6~73.52×10^-6),更富集轻稀土元素(Ce、Pr、Nd、Sm),呈右倾的稀土元素配分模式,负铕异常明显。推测石榴子石GrtⅠ形成于相对开放、水岩比值较高、高氧逸度的酸性体系中,GrtⅡ则形成于相对封闭、水岩比值较低、高氧逸度的中酸性体系中。此外,将石榴子石的端员组分和微量元素特征与国内外不同矿种的接触交代型金属矿床进行对比,结果显示该矿床存在成Cu、Fe、Mo矿体的潜力。     

内蒙古沙麦钨矿花岗岩岩石地球化学、锆石U-Pb年代学及其地质意义

沙麦钨矿床位于内蒙古东乌旗地区,是该区目前已探明的中型岩浆热液型钨矿床。矿体主要赋存在黑云母二长花岗岩和黑云母二长花岗斑岩中,对这两种花岗质岩石的岩相学、岩石地球化学和LA-ICP-MS锆石U-Pb年代学进行了研究。结果表明,黑云母二长花岗岩锆石U-Pb年龄为135.6±1.6 Ma和136.3±1.8 Ma,黑云母二长花岗斑岩锆石U-Pb年龄为138.6±1.1 Ma,二者侵位时间均为早白垩世。两种花岗质岩体具有富SiO₂(73.73%～78.23%)、高钾钠(Na₂O+K₂O)(7.56%～8.89%)、贫MgO(0.09%～0.20%)、贫CaO(0.51%～0.89%)、贫TiO₂(0.03%～0.12%)的特征,属于过铝质-高钾钙碱性系列;微量元素富集Rb、K、Th和U,相对亏损Sr、Ba、Nb、P和Ti元素,具有强烈的Eu负异常,具有较高的FeO^T含量,较高的FeO^T/MgO和FeO^T/(FeO^T+M...     

河西走廊成矿带区域成矿规律及找矿方向

河西走廊成矿带是分布于祁连地区最北部的Ⅲ级成矿单元(全国统一编号为Ⅲ-20), 目前共有235处矿产地, 形成了石油、煤、凹凸棒石黏土、萤石、石膏、芒硝、石灰岩、天然石英砂、铁、铜、金、钨等40余种矿产。该成矿带以沉积成矿作用为主, 其次为流体、岩浆、变质和表生成矿作用, 可分为11种矿床类型, 主要成矿期为华力西期、加里东期、燕山期和喜马拉雅期。河西走廊成矿带可进一步划分为2个成矿亚带, 分别为玉门—民乐成矿亚带和山丹—中卫—泾源成矿亚带。根据构造空间、成矿时间、成矿作用和矿种等四要素的耦合关系, 河西走廊成矿带厘定了10个矿床成矿系列, 包括4个沉积作用有关矿床成矿系列、3个流体作用有关矿床成矿系列、1个岩浆作用有关矿床成矿系列、1个变质作用有关矿床成矿系列和1个表生作用有关矿床成矿系列。通过细分成矿时段和细化成矿地质作用, 进一步解析出16个矿床成矿亚系列, 并建立了47个矿床式。根据区内地质、矿产、物探、化探和遥感信息, 河西走廊成矿带共圈出5个综合预测区, 为下一步找矿工作指出了方向。     

江西钨锡多金属矿床成矿系列与找矿

本文在江西省地质勘查基金项目十余年找矿成果的基础上, 进一步阐述了江西钨锡成矿区(带)时空演化规律, 建立了江南和南岭2条钨锡多金属成矿带, 进而划分9条成矿亚带和15个矿集区; 厘定了包括江南地块与燕山期Ⅰ型中酸-弱酸性斑岩有关的铜钨金钼矿床成矿系列等共3个成矿系列、与燕山晚期S1型酸性花岗岩有关的钨锡钼银矿床成矿亚系列等6个成矿亚系列和朱溪式等15个矿床式; 总结了3个钨锡多金属矿床成矿系列特征及成矿规律, 剖析了朱溪、大湖塘、东坪、松树岗等找矿重大突破典型案例; 提出了“异常指方向、标志定靶区、主攻新类型”的“面上选点”找矿预测及勘查思路, 研发了“脉面层体”就矿找矿法的“点上突破”朱溪式“关键控矿要素识别勘查模型+地球化学元素示踪+地球物理三维反演+钻探”等快速、精准、高效探测技术组合的找矿方法, 对江西钨锡矿找矿潜力进行评价分析, 并提出下一步找矿建议。     

以门源M6.9地震为契机的祁连带中东段地震热红外异常区域特征研究

以中国静止气象卫星亮温资料为数据基础,使用小波变换和功率谱估计法研究2022年1月8日门源M6.9地震前的热辐射异常,并对祁连带中东段以往震例的热辐射异常作回溯性研究。门源6.9级地震的热辐射异常发展过程可分为3个阶段：初始演化阶段、增强持续阶段、减弱消失阶段。面积最大时强辐射区的面积约为8万km~2,地震发生在其西北部。相对功率谱峰值为平均值的17倍,地震发生在峰值后82天。大面积、高强度的热辐射状态持续时间长是此次异常的显著特点。祁连带中东段的几次地震前均出现过热辐射异常,其特征可为该区震情判定不断积累经验,以期形成可作为判定指标的区域震例库。     

张家口—渤海地震带岩石圈磁场时空变化特征

利用2016—2018年3期华北地区流动地磁矢量原始测量资料, 经数据计算获得2期华北地区和张家口—渤海地震活动带及邻区岩石圈磁场时空变化模型。 研究结果显示: 张家口—渤海地震带岩石圈磁场变化空间分布不均匀, 具有明显的分区特征, 在张家口段(西段)与北京段(中西段)分界处和北京段(中西段)与唐山段(中东段)分界处岩石圈磁场各要素具有明显的异常变化, 如水平矢量存在转向和幅值变化, 磁偏角与磁倾角具有正负异常高梯度带的特征, 这与张家口—渤海地震带构造分段性特征密切相关。 张家口—渤海地震带位于燕山块体与华北平原块体之间, 两者运动的平动速率之差是张家口—渤海地震带左旋走滑的直接动力来源, 而各断裂带左旋走滑速率之差很可能是岩石圈磁场空间变化分段性分布的主要原因。