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Discowry of Cosmic Dust in Gold Deposits in Northwestern Sichuan and Its Significance
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作者 Zheng M inghua, Zhou Yufeng, Fu Reaping Department of Mineral Resources, Chengdu University of Technology, Chengdu, Sichuan Fei Zhenbi 《Acta Geologica Sinica(English Edition)》 SCIE CAS CSCD 1995年第4期396-405,448,共11页
In recent years, a considerable amount of microscopic spherules have been found in concentrates recovered from some stratabound gold deposits occurring in Middle-Upper Triassic turbidite series in northwestern Sichuan... In recent years, a considerable amount of microscopic spherules have been found in concentrates recovered from some stratabound gold deposits occurring in Middle-Upper Triassic turbidite series in northwestern Sichuan. Study indicates that these spherules are cosmic dust. It is the first time that cosmic dust of extraterrestrial origin has been found in hydrothermal gold deposits in China.The spherules are steel-grey in colour and show metallic luster. Their grain size is commonly less than 100 μm. According to their composition, they belong to chromium-rich iron cosmic dust. The spherules have complex and diverse microscopic structures and textures, i.e. they show a very distinct Widmanstaten structure.The variation of cosmic dust content in gold deposits exhibits a positive correlation with the mineralization intensities and hydrothermal alteration. Such a relation indicates that the ore sub- stances may transport not only mechanically but also may chemically in hydrothermal solutions. 展开更多
关键词 gold deposit cosmic dust northwestern Sichuah Middle-Upper Triassic
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DISCOVERY OF ORGANIC MOLECULES IN DEEP-SEA IRON COSMIC DUST
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作者 彭汉昌 徐培苍 《Chinese Journal of Oceanology and Limnology》 SCIE CAS CSCD 1995年第1期9-12,共4页
A great quartity of cosmic dust(spherules) was found in deep-sea sediments during May to July,1983manganese nodule investigations by the R/V“XIANGYANGHONG 16”in the area 7°-11°N,167°-178°Win th... A great quartity of cosmic dust(spherules) was found in deep-sea sediments during May to July,1983manganese nodule investigations by the R/V“XIANGYANGHONG 16”in the area 7°-11°N,167°-178°Win the Pacific.Comprehensive study of the cosmic dust and determination with Laser Raman MolecularMicroprobe(LRMM) of the molecules in it showed that besides Fe-Fe,Fe<sup>3+</sup>-O,Fe-Ni,Al-O,Fe-Obr-Si and Si-Onb,it also contained the organic molecules C-H-O and C-H-S-O,various no fixed form molecules of C,CH<sub>2</sub>,CH<sub>3</sub> and volatile molecules CO<sub>2</sub>,H<sub>2</sub>O,OH<sup>-</sup> and H<sub>2</sub>S,etc…The study result has very important applications for exploring the origin of interplanetary dust parti-cles and life material. 展开更多
关键词 IRON cosmic dust organic MOLECULE Laser Raman molecular MICROPROBE life material
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Cosmic Dust as an Indicator for the Genetic Classification of Granites
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作者 付成义 付国飞 《Chinese Journal Of Geochemistry》 EI CAS 1993年第4期361-364,共4页
In the strdy of the source material of granites ,it is found that cosmic dust can be used as one of the indicators for identifying the genetic types of granites.It is suggested that granites can be grouped into two ge... In the strdy of the source material of granites ,it is found that cosmic dust can be used as one of the indicators for identifying the genetic types of granites.It is suggested that granites can be grouped into two genetic types, dust-barren granite and dust-containing granite, corresponding to I-type and S-type respectively as defined by Chappell et al. 展开更多
关键词 宇宙尘埃 花岗岩 分类 矿物 化学组成
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A study on cosmic dust particles in Antarctic ice,snow and non-Antarctic region and their origins
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作者 王道德 戴诚达 《Chinese Journal of Polar Science》 1995年第2期1-17,共17页
A large number of cosmic dust particles, micrometeorites and volcanic dust bands have been found and collected in Antarctic ice, snow and glacial sediments, especially in meteorite concentrated regions. Extraterrestri... A large number of cosmic dust particles, micrometeorites and volcanic dust bands have been found and collected in Antarctic ice, snow and glacial sediments, especially in meteorite concentrated regions. Extraterrestrial spherules also have been discovered from the stratosphere and deep-sea sediments. On the basis of their distributive characteristics the cosmic dust particles are classified into interplanetary dust particles and interstellar dust particles. According to their origins cosmic dust particles can be divided into cometary origin particles, asteroidal origin particles, ablation particles from meteorites and interstellar origin particles. The criteria for identifying cosmic dust particles have been established and the origins of cosmic dust particles are also discussed in aegis paper. 展开更多
关键词 ANTARCTICA cosmic dust particles interplanetary dust particles interstellar dust particles.
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COSMIC DUSTS FROM WENDUERMIAO GROUP AND BAINAIMIAO GROUP IN NEI MONGOL OF CHINA
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作者 李增慧 《Chinese Science Bulletin》 SCIE EI CAS 1986年第16期1129-1133,共5页
When we investigated the occurring conditions of the iron-riih deposits in Jining-Erlian area, Nei Mongol, in 1977, many opaque and shiny steel balls about 200μ in diameter have been found in the strong magnetic frac... When we investigated the occurring conditions of the iron-riih deposits in Jining-Erlian area, Nei Mongol, in 1977, many opaque and shiny steel balls about 200μ in diameter have been found in the strong magnetic fraction of both natural and artifact heavy minerals from the Wenduermiao Group and Bainaimao Group. Examinations of different approaches led to the conclusion that they are the cosmic dusts. 展开更多
关键词 cosmic dustS FROM WENDUERMIAO GROUP AND BAINAIMIAO GROUP IN NEI MONGOL OF CHINA
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MEASUREMENTS OF ANNUAL DEPOSIT MASS OF COSMIC DUST BY DEEP-SEA SEDIMENTATION
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作者 彭汉昌 陆康 柴之芳 《Chinese Science Bulletin》 SCIE EI CAS 1989年第1期57-60,共4页
We measured the annual deposit mass of cosmic dust on the Earth based on average sedimentation rate and content of cosmic dust at 20 surface stations on the Pacific investigation area (6°—13°N, 166°—1... We measured the annual deposit mass of cosmic dust on the Earth based on average sedimentation rate and content of cosmic dust at 20 surface stations on the Pacific investigation area (6°—13°N, 166°—178°W). The results indicate that measured results of each station are more identical and in accord with most measured results in the past, too. 展开更多
关键词 cosmic dust ANNUAL DEPOSIT MASS SEDIMENTATION rate surface area of the Earth sampler.
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A STUDY ON THE GENESES OF SURFACIAL TEXTURES OF COSMIC DUST
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作者 傅国飞 傅成义 徐洪武 《Chinese Science Bulletin》 SCIE EI CAS 1991年第3期214-216,共3页
Most cosmic dusts possess distinctive surfacial textures. The investigation on these textures greatly contributes to the research of ablation for meteorite and the geneses of cosmic dusts.
关键词 cosmic dust surfacial TEXTURE genesis.
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The Cosmic Dusts in the Malan Loess Near Xi' an
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作者 赵济湘 肖永林 祝一志 《Chinese Science Bulletin》 SCIE EI CAS 1994年第24期2063-2067,共5页
The Quaternary loess deposits in the arid-semiarid area in northwestern China are composed of eolian sedimemts which are continuous in terms of sedimentation and have undergone little alternation after deposition.They... The Quaternary loess deposits in the arid-semiarid area in northwestern China are composed of eolian sedimemts which are continuous in terms of sedimentation and have undergone little alternation after deposition.They provide an ideal place for the preservation of the extraterrestrial falls on the earth.The Late Pleistocene Malan loess is chosedn for our study of the preserved cosmic dusts. 展开更多
关键词 Malan LOESS cosmic dust Xi’an.
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Discovery and implication of cosmic dust from Ⅰ-type granite of western Suzhou
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作者 王尔康 林承毅 +3 位作者 胡中为 万玉秋 张文兰 宋永勤 《Chinese Science Bulletin》 SCIE EI CAS 1995年第21期1818-1823,共6页
Since the discovery of cosmic dust from Suzhou A-type granite, a following new problem is whether cosmic dust is preserved in only one type granite or in different types. In order to make the problem clear, the author... Since the discovery of cosmic dust from Suzhou A-type granite, a following new problem is whether cosmic dust is preserved in only one type granite or in different types. In order to make the problem clear, the authors carried out many field and room investigations on I-type granite of western Suzhou, and found out that Suzhou I-type granite also could retain microspherules. Studies about these microspherules indicate that they are of ablated cosmic dust. 展开更多
关键词 cosmic dust MICROSPHERULE GRANITE Suzhou.
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DISCOVERY OF COSMIC DUST IN GRANITE AND ITS SIGNIFICANCE
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作者 傅成义 刘孝善 《Chinese Science Bulletin》 SCIE EI CAS 1988年第23期1974-1978,共5页
The systematic study in this article has proved that the magnetic ferro-spherules in granite of various ages are cosmic dust which was discovered in the Yangjiazhangzi Molybdenum (Mo) field in the west of Liaoning Pro... The systematic study in this article has proved that the magnetic ferro-spherules in granite of various ages are cosmic dust which was discovered in the Yangjiazhangzi Molybdenum (Mo) field in the west of Liaoning Province (see the newspaper of 'Chinese Geology' for detailed information). 展开更多
关键词 cosmic dust GRANITE LIAONING
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Cosmic Dust in Suzhou A-Type Granite
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作者 王尔康 万玉秋 +4 位作者 朱政 胡中为 林承毅 周剑雄 倪邦发 《Science China Chemistry》 SCIE EI CAS 1994年第9期1119-1129,共11页
A large number of microspherules have been extracted from Suzhou A-type granite bymeans of heavy placer.Both natural surfaces and part sections of 539 microspherules have been observed bySEM.457 microspherules have be... A large number of microspherules have been extracted from Suzhou A-type granite bymeans of heavy placer.Both natural surfaces and part sections of 539 microspherules have been observed bySEM.457 microspherules have been determined by EDX,with some of them by EPMA,XRD and INAA.The results suggest these spherules are of ablated cosmic dust.Among them silicate glassy microspheruleshave been highly enriched in REE and other lithophile refractory trace elements,and REE abundance patternfavors a meteoritic origin as a roughly flat distribution.Ringwoodite has been first found in these glassy mi-crospherules.The composition of these iron spherules is similar to those of the ablated cosmic dust from deepsea and polar ice.Some Fe-Ni spherules and spherules composed of troilite have also been found.This isprobably the first report on various types of cosmic dust extracted from granite. 展开更多
关键词 cosmic dust MICROSPHERULE GRANITE SUZHOU
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COSMIC DUST FROM CHANGZHOUGOU FORMATION IN JIXIAN AREA AND ITS FALLING AGE
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作者 李增慧 马来斌 《Chinese Science Bulletin》 SCIE EI CAS 1991年第21期1816-1819,共4页
Ⅰ. GEOLOGICAL SETTINGS OF SAMPLING LOCALITY The sampling locality is in Changzhougou Village on the northern North China Platform. In the late Precambrian, this area seriously sank. Changzhougou Formation overlies un... Ⅰ. GEOLOGICAL SETTINGS OF SAMPLING LOCALITY The sampling locality is in Changzhougou Village on the northern North China Platform. In the late Precambrian, this area seriously sank. Changzhougou Formation overlies unconformably the Archaean gneiss. 展开更多
关键词 cosmic dust fusion-type from METEORITE FALLING age ~40Ar/~39Ar age SPECTRUM
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Cosmic Contributions to the Deposition of Petroleum Source Rocks: Review and Analysis 被引量:1
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作者 Heinz-Jürgen Brink 《International Journal of Geosciences》 2023年第11期1123-1145,共23页
The development of globally distributed Phanerozoic petroleum source rocks is concentrated on time intervals, which correlate convincingly with climatic driven glaciation epochs of Earth’s history, repeated every 150... The development of globally distributed Phanerozoic petroleum source rocks is concentrated on time intervals, which correlate convincingly with climatic driven glaciation epochs of Earth’s history, repeated every 150 million years, and during sea level high stands and maxima of global magmatism with a period of 300 million years. The 150 million year periodicity appears to be related to the path of the solar system through the spiral arms of the Milky Way and the 300 million year periodicity to changes of the spiral system. The spiral arms are preferred birth places of new stars, of which the larger ones have only smaller lifespans. Their preliminary deaths ended with explosions and selectively with the development of so-called white dwarfs, neutron stars or black holes. The times of the explosions of intermediate (sun-like) stars can be determined by measuring the present brightness of the dwarfs. Not surprisingly the last two maxima of recordable near solar system star explosions took place during the presumably spiral arms driven glacial epochs in Eocene to present and Upper Jurassic times. Such near solar system star explosions may have been the source of intense neutrino showers, cosmic rays and star dust. This dust contained all kinds of chemical elements, including phosphorus and uranium. Such cosmic phosphorus may have supported, through fertilizing, the distribution of life on Earth additionally to local phosphorus resources via bloom of biota in lakes and oceans and the enhanced growth of plants on land across all climatic zones. Subsequently it maintained the development of petroleum source rocks of all organic matter types within black shales and coals. Via the distribution of remnants of exploding stars—mainly white dwarfs, but neutron stars and black holes have to be counted as well—a cosmic contribution can therefore casually linked to the deposition of petroleum source rocks on Earth, not only purely correlatively by their contemporaneous appearances. 展开更多
关键词 cosmic Rays cosmic dust Milky Way Spiral Arms Stars PHOSPHORUS URANIUM Petroleum Source Rock
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Organic Molecules in the Interstellar Dust
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作者 Ali Abdul Sattar Jaber Al-Edhari 《材料科学与工程(中英文版)》 2010年第1期16-21,共6页
关键词 星际尘埃 有机分子 生物材料 二氧化硅 银河系中心 有机物质 大肠杆菌 识别模型
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空间碎片与空间环境 被引量:51
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作者 李春来 欧阳自远 都亨 《第四纪研究》 CAS CSCD 北大核心 2002年第6期540-551,共12页
空间碎片起源于人类的航天活动 ,目前空间碎片的空间密度已经对航天器的安全造成威胁 ,且其数量仍在高速增长 ,已成为一个引人瞩目的环境问题 ,航天器受空间碎片撞击的事件时有发生。大空间碎片的撞击会使航天器姿态和轨道发生改变 ,更... 空间碎片起源于人类的航天活动 ,目前空间碎片的空间密度已经对航天器的安全造成威胁 ,且其数量仍在高速增长 ,已成为一个引人瞩目的环境问题 ,航天器受空间碎片撞击的事件时有发生。大空间碎片的撞击会使航天器姿态和轨道发生改变 ,更严重的是会导致航天器破损甚至完全解体 ;小空间碎片的撞击会使航天器表面性能改变 ,部分器件损伤或失效 ,使航天器丧失功能。目前地基设备只能对厘米级及更大的碎片进行观测、跟踪和编目 ,航天器可以根据空间碎片的轨道参数进行规避和机动飞行 ,以避免撞毁 ;小空间碎片 (<1cm)数量众多 ,但无法进行轨道测量 ,只能通过天基直接探测和样品回收获得数据 ,数值建模和超高速撞击模拟实验是进行小空间碎片风险评估和撞击效应研究的有效方法。对小空间碎片只能采取被动防护的方法 ,在航天器总体设计、防护结构和材料方面着手 ,降低空间碎片的威胁。改善空间环境 ,减少空间碎片的最根本方法是对航天器采取钝化措施 ,减少空间碎片的产生 ,理论上还可以采取措施 ,清扫、清除或回收空间碎片。 展开更多
关键词 空间碎片 宇宙尘 空间环境 撞击 航天器 航天活动
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我国若干地区宇宙尘的初步研究 被引量:7
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作者 李增慧 陈克樵 +3 位作者 马淑兰 魏家秀 郭文歧 王凤桐 《地球科学(中国地质大学学报)》 EI CAS CSCD 北大核心 1990年第2期172-182,T003,共12页
本文论述了我国若干地区不同时代地层中宇宙尘的物理特性、化学成分和微结构特征,并同深海沉积的铁质尘粒进行了对比。笔者以为,这些宇宙尘是球外物质,可能是铁陨石在大气中的消熔物或是在太空中的碎裂物。
关键词 宇宙尘 铁纹石 陨石 消溶型
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用扫描隧道显微镜研究铁陨石和铁质宇宙尘球粒的亚微米和纳米结构 被引量:2
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作者 周瑶琪 柴之芳 +2 位作者 徐英庭 王大文 白春礼 《岩矿测试》 CAS CSCD 北大核心 1996年第1期1-12,共12页
运用扫描隧道显微镜(STM)观测了一颗深海铁质宇宙尘球粒的亚微米和纳米结构,并与一块宁波(ⅣA)铁陨石的线切割碎片的表面结构进行了对比。通过分形几何学的定量研究,发现在亚微米尺度铁陨石碎片和铁质宇宙尘的表面结构存在自... 运用扫描隧道显微镜(STM)观测了一颗深海铁质宇宙尘球粒的亚微米和纳米结构,并与一块宁波(ⅣA)铁陨石的线切割碎片的表面结构进行了对比。通过分形几何学的定量研究,发现在亚微米尺度铁陨石碎片和铁质宇宙尘的表面结构存在自相似性,但铁质宇宙尘与铁陨石线切割碎片的表面分数维特征却明显不同,前者分数维D值约为2.3,后者D值为2.6~2.7。这与它们的热动力学过程的差异有关。 展开更多
关键词 铁质宇宙尘 扫描隧道显微镜 纳米结构 铁损石
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一九九九年狮子座强流星雨的无线电观测 被引量:2
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作者 何友文 马月华 +2 位作者 徐品新 李广宇 赵海斌 《电波科学学报》 EI CSCD 北大核心 2005年第4期467-471,共5页
1999年我国首次在白天开展了狮子座强流星雨及其电离效应的无线电观测,结合国际流星组织收集的30余个国家光学(目视)流星观测资料,初步证实:1999年狮子座强流星雨发生了比1998年更强的爆发;fbEs异常峰被丢失。同时,不仅对fbEs异常峰的... 1999年我国首次在白天开展了狮子座强流星雨及其电离效应的无线电观测,结合国际流星组织收集的30余个国家光学(目视)流星观测资料,初步证实:1999年狮子座强流星雨发生了比1998年更强的爆发;fbEs异常峰被丢失。同时,不仅对fbEs异常峰的丢失作了进一步的确认,并且还对人们关心的宇宙尘演化过程作了粗浅的讨论。 展开更多
关键词 狮子座流星雨 强流星雨 fbEs异常峰 宇宙尘 无线电流星
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利用高空科学气球收集宇宙尘粒 被引量:3
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作者 欧阳自远 万固存 +2 位作者 黄伯钩 徐以文 吴锡光 《空间科学学报》 CAS CSCD 北大核心 1993年第1期73-79,共7页
本文叙述了高空科学气球上一种自行研制的宇宙尘收集器以及气球吊篮系统。利用该系统进行了五次高空字宙尘粒的收集飞行,简述了对所收集的尘粒进行系统研究的结果。
关键词 高空气球 宇宙尘 收集器
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中纬区长寿命Es层的维持机制 被引量:2
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作者 何友文 马月华 +1 位作者 徐品新 赵海斌 《电波科学学报》 EI CSCD 北大核心 2007年第6期1047-1051,共5页
首届狮子座强流星雨国际联测期间,我们开展了多学科、多手段的狮子座和天龙座强流星雨及其电离效应的综合观测,并结合近半个世纪的(1957~2003年)狮子座、英仙座和天龙座强流星雨及其电离效应等相关资料的综合分析,证实夜间(18:0... 首届狮子座强流星雨国际联测期间,我们开展了多学科、多手段的狮子座和天龙座强流星雨及其电离效应的综合观测,并结合近半个世纪的(1957~2003年)狮子座、英仙座和天龙座强流星雨及其电离效应等相关资料的综合分析,证实夜间(18:00~06:00)爆发的强流星雨在其爆发的-92h到102h时段内,在大范围同时观测到fbEs异常峰的存在。下述结论亦得到初步证明:fbEs异常峰出现规律,强流星雨和宇宙尘暴的形成机制。文内还对宇宙尘的演化过程,中纬区Es层金属离子的来源和中纬区长寿命Es层的维持机制作了粗浅的讨论。 展开更多
关键词 强流星雨 fbEs 异常峰 宇宙尘暴
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