云南西双版纳曼桂陨石雨调查     

李世杰  罗维均  李博方  李阳 《矿物学报》2020,40(2):176-182

北京时间2018年6月1日21:43左右,在云南西双版纳景洪市的西南有火流星滑过夜空,通过目击者拍摄的视频初步判断又是一次陨石降落,这是继2017年10月4日(农历中秋节)后又一次目击到流星光顾云南省上空。6月2日有消息称在西双版纳勐海县勐遮镇的曼伦村发现了降落的陨石。随后的几天,陆续有很多媒体记者、陨石爱好者和陨石猎人赶往陨石降落地,随即,一场陨石雨呈现出来。截止目前,已经收集到的数据表明这次陨石雨的已知范围约3km×12km,从南东向北西方向以55.3°±2.5°的入射角度降落至地面,先后在曼南、曼光、曼央囡、曼潘、曼么代、曼楷龙、曼庄、曼垒、曼伦、曼迈回、曼朗、曼赛、蔓燕和曼桂村等10余个自然村发现陨石,据不完全统计,陨石数量超过1000个,质量由0.04 g至1280 g,总质量超过50 kg。该陨石雨陨石类型为L6,冲击程度为S4。  相似文献   

火星陨石和火星表面泥岩中蚀变过程对比研究     

付晓辉  凌宗成  周琴  Bradley L.JOLLIFF  尹庆柱  王阿莲  李勃  武中臣  张江 《地学前缘》2020,27(4):340-354

火星次生含水蚀变矿物是火星地质历史时期水环境和气候演变历史的真实记录,一直以来都是火星探测、火星陨石研究的重点,是认识火星环境特征和气候演化的重要研究对象。文中对比研究了表土角砾岩NWA7034、火成堆晶岩MIL03346等两块最富蚀变矿物火星陨石,以及Gale撞击坑出露的Sheepbed泥岩3种岩石类型的蚀变程度及其蚀变矿物类型和组合,分析了层状硅酸盐、铁氧化物/氢氧化物、钙硫酸盐等蚀变矿物的成因及环境指示意义。发现这3类岩石的蚀变作用各不相同。火星陨石NWA7034的蚀变作用以氧化和加热作用为主,无蒸发盐类矿物。火星陨石MIL03346的蚀变程度最低,为后期水溶液进入缝隙而引发的,蚀变作用以橄榄石的伊利石化、裂隙和缝隙中填充次生矿物细脉为主。而火星Sheepbed泥岩经历了后期的等化学风化过程(isochemical weathering),次生过程包括成岩蚀变和成岩后蚀变两个阶段。其中,成岩过程中的蚀变以橄榄石蚀变为铁氧化物和蒙皂石矿物为主,成岩后以形成蒸发盐类矿物硫酸钙为主。以上3种岩石蚀变矿物组成差异反映了火星上不同地质背景中、不同气候条件下蚀变过程的复杂性。文中对火星含水矿物及部分典型矿物的形成条件和过程进行系统总结,这对于理解未来火星探测任务、识别含水矿物的形成、揭示火星水环境和地质历史具有重要指导意义。  相似文献   

Geochemistry of the Martian Meteorite GRV 99027     

王鹤年  谢志东  梁英 《极地研究(英文版)》2009,20(2):110-134

GRV 90027 is a Martian lherzolitic shergottites (L-S) containing poikilitic, non-poikilitic, and melted pocket components. GRV 99027 is mainly composed of olive (55 vol%) and pyroxene (37.5 vol%), with minor maskelynite (6 vol%) and chromite (1.5 vol%), and trace whitelockite and troilite, ect. In this paper, the mineralogy and petrology of GRV 99027 are reported; in addition, the geochemical characteristics of the REEs and H isotopes in the GRV 99027 are also further investigated. The ΣREE in GRV 99027 is relatively low; HREEs are enriched in olivine and pyroxene grains; LREEs are enriched in plagioclase with a high positive Eu anomaly. High ΣREE value is found in rare mineral whitlockite (less than 0.2 vol%), LREE≈HREE, and whitlockite has a negative Eu anomaly. The REE distribution patterns of the whole -rock of GRV 99027 is similar to but different from that of other L-S Martian meteorites, indicating that they came from different location of Mars. GRV 99027 has a high δD value. Different water-bearing minerals give different contribution for δD value. The δD of phosphates generally does not correlate with water content, and δD has a weak negative correlation with water content. GRV 99027 can be classified as an L-S Martian meteorite based on mineralogical assemblage patterns, REE distribution patterns, and hydrogen isotope. The isotope data of Sr, Nd, Pb, Os and REE from other L-S Martian meteorites were collected to discuss the formation history of the GRV 99027. Similar to other L-S Martian meteorites, GRV 99027 originated from part of Mar's mantle; during one strong impact event about 4M years ago, the meteorites were ejected from deep mantle into space, and traveled for a different duration in space (indicated by different cosmic exposure time), and captured by the Earth later in different time, ultimately falling on the Antarctica as L-S Martian meteorites.  相似文献   

GRV 051523： A new eucrite     

刘焘  林杨挺  胡森  冯璐 《极地研究(英文版)》2009,20(2):200-208

Grove Mountains (GRV) 051523 is a newly identified eucrite, consisting mainly of coarse-grained pyroxene (62.9 vol%) and plagioclase (34.2 vol%), with less abundant opaque minerals (2.7 vol%), minor silica and tiny FeO-rich olivine (Fa75). Coarse-grained pyroxenes show exsolution of augite lamellae in pigeonite or vice versa. Width of most exsolution lamellae in pyroxenes is 1-3 μm. Opaque minerals are mainly chromite, ilmenite and sulfides. The meteorite was heavily shocked, as indicated by breccias and melt veins. Coarse-grained pyroxenes commonly contain abundant tiny or needle-like chromite inclusions with orientation, probably due to heavy shock events. Pyroxenes in various petrographic occurrences exhibit highly homogeneous compositions, indicating that GRV 051523 experienced intense thermal metamorphism in the parent asteroid 4 Vesta. GRV 051523 is classified as Type 5-6. This new eucrite will have additional constraints on chemical composition, magmatic differentiation, multi-stage shock and thermal history of Vesta.  相似文献   

Bulk Chemical Composition of the Ningqiang Carbonaceous Chondrite： An Issue of Classification   总被引：1，自引：0，他引：1  

WANG Guiqin LIN Yangting 《《地质学报》英文版》2007,81(1):141-147

The Ningqiang meteorite is a fall carbonaceous chondrite, containing various Ca-, Al-rich inclusions that usually escaped from secondary events such as high-temperature heating and low- temperature alteration. However, it has not yet been classified into any known chemical group. In order to address this issue, 41 elements of the bulk Ningqiang meteorite were analyzed using inductively coupled plasma mass spectrometry （ICP-MS） and inductively coupled plasma atom emission spectrometry （ICP-AES） in this study. The Allende （CV3） carbonaceous chondrite and the Jilin （H5） ordinary chondrite were also measured as references, and our analyses are consistent with the previous results. Rare earth and other refractory lithophile elements are depleted in Ningqiang relative to both Allende and mean CK chondrites. In addition, the REE pattern of Ningqiang is nearly flat, while that of Allende shows slight enrichment of LREE relative to HREE. Siderophile elements of Ningqiang are close to those of mean CK chondrites, but lower than those of Allende. Our new analyses indicate that Ningqiang cannot be classified into any known group of carbonaceous chondrites, consistent with previous reports.  相似文献   

青藏高原东北部黄土沉积化学风化程度及古环境   总被引：14，自引：1，他引：14  

张西营  马海州  谭红兵 《海洋地质与第四纪地质》2004,24(2):43-47

通过对青藏高原东北部西宁盆地大墩岭剖面24种常微量元素的测定及数据的处理分析，研究了该地区黄土沉积的化学风化程度及某些地球化学特征。相对上部陆壳(UCC)元素平均值，大墩岭剖面显著富集Ca、Mg、Ti、V、Cr、Ni、Y、Zr等，而亏损Si、Al、K、Na、Sr、Nb等；相对于中国黄土(CL)元素平均值，大墩岭剖面明显富含Fe、Ca、Mg、K、Ti、Cr、Mn、Cu、Rb、Sr、Nb、Ba和P，而Si、Na、Co、Ni、Pb则表现为亏损；在UCC标准化图与CL标准化图中，大墩岭黄土与古土壤变化趋势基本一致。大墩岭剖面尚处于脱Ca、Na的大陆风化初期阶段。与其他地区的风尘沉积相似，大墩岭黄土沉积很可能也起源于上部陆壳，但不排除物源存在一定差别。风尘堆积时该区的气候环境比黄土高原要干冷，这与青藏高原第四纪以来的强烈隆升有直接关系。  相似文献   

Possible impact event in the Late Cambrian   总被引：1，自引：0，他引：1  

References： 《东北亚地学研究》2007,10(1):78-82

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Cosmic-ray exposure age of Martian meteorite GRV 99027     

Kong Ping  D. Fabel  R. Brown  S. Freeman 《中国科学D辑(英文版)》2007,50(10):1521-1524

We have determined the concentrations of 10Be and 26Al in GRV 99027 recovered by the 16th Chinese Antarctic expedition team, which are 14.1 ± 0.6 dpm/kg and 67.5 ± 3.4 dpm/kg, respectively. From the concentration of 10Be, we calculate a cosmic-ray exposure age of 4.4 ± 0.6 Ma for GRV 99027. The concentration of 26Al is too high compared to the 10Be exposure age, indicating extra production from solar ray. The exposure ages, petrologic and geochemical characteristics of mantle-derived Martian meteorites GRV 99027, LEW 88516, Y-793605, NWA 1950 and ALHA77005 are very similar, suggesting that these meteorites most probably were ejected from Mars in the same impact event.  相似文献   

青海省西宁地热田成因分析及资源评价   总被引：10，自引：3，他引：7       下载免费PDF全文

赵振  于漂罗陈惠娟  罗银飞  赵东阳  边疆 《中国地质》2015,42(3):803-810

笔者通过对西宁地热田已有钻探资料和区域地热地质资料,结合近几年的勘查项目研究成果,分析了西宁地热田的埋藏条件、补径排条件、地温场及水文地球化学的特征,阐述了西宁地热田主要以大地热流为热源—低热导率岩层聚热—深循环逐渐加热受迫对流机制—构成控水控热,具有以盆地传导型面状热储为主,兼有断裂对流型带状热储特征.同时,采用热储法对西宁地热田地热资源量进行了评价,该地热田内热储中储存的热量9.343×1014kJ,利用平均布井法计算出该地热田每年开采热量为1.12×1012kJ,折合标准煤3.78×104t,按地热田规模分级为中型低温地热田.初步摸清了西宁地热田分布规律以及资源量,为西宁地热田地热资源合理开发利用提供了重要依据.  相似文献   

青海西宁盆地三趾马、副板齿犀化石的发现及意义     

韩建恩  邵兆刚  陈麒光  孟宪刚  朱大岗  张倩倩  权凯  王津  胥彪 《地球学报》2015,36(1):115-120

首次在青海西宁盆地新近纪河湖相沉积地层中发现了三趾马、副板齿犀牙齿化石,对化石的基本特征和埋藏情况进行了描述,三趾马化石经鉴定为东乡三趾马。结合区域和前人资料认为,本次发现化石的岩石地层应该属于咸水河组或以上层位,时代为晚中新世早期。分析前人孢粉资料认为化石形成时的古植被为森林-草原,古气候环境为亚热带干旱气候环境。这一发现为西宁盆地晚新生代河湖相地层格架的建立,提供了古生物学依据,对西宁盆地中新世地层确立起到时序标尺的作用。为青藏高原东北缘盆地的环境演化、地层划分、时代厘定提供了新的资料,对深入研究青藏高原隆升环境效具有重要意义。同时,也为青藏高原东北缘、华北地区、青藏高原三趾马动物群进行对比研究,提供了基础材料。  相似文献