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东乌珠穆沁旗中铁陨石中有二种橄榄石。一种是陨石中基质橄榄石，另一种是镶嵌在陨石表面的角砾状橄榄石。电子探针成分分析结果表明，两种橄榄石中的FeO和MnO比值，包体矿物种类，包体铁纹石和镍纹石中Fe,Ni的含量等，均有较大区别。陨石中基质橄榄石矿物是本陨石中原物质，而角砾状橄榄石是宇宙中物质。他们是两块自由翱于宇宙中的物质碰撞混合而形成的东乌珠穆旗陨石中这种现象。 相似文献
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<正>GRV 020175 is an Antarctic mesosiderite,containing about 43 vol%silicates and 57 vol% metal.Metal occurs in a variety of textures from irregular large masses,to veins penetrating silicates, and to matrix fine grains.The metallic portion contains kamacite,troilite and minor taenite.Terrestrial weathering is evident as partial replacement of the metal and troilite veins by Fe oxides.Silicate phases exhibit a porphyritic texture with pyroxene,plagioclase,minor silica and rare olivine phenocrysts embedded in a fine-grained groundmass.The matrix is ophitic and consists mainly of pyroxene and plagioclase grains.Some orthopyroxene phenocrysts occur as euhedral crystals with chemical zoning from a magnesian core to a ferroan overgrowth;others are characterized by many fine inclusions of plagioclase composition.Pigeonite has almost inverted to its orthopyroxene host with augite lamellae, enclosed by more magnesian rims.Olivine occurs as subhedral crystals,surrounded by a necklace of tiny chromite grains(about 2-3μm).Plagioclase has a heterogeneous composition without zoning. Pyroxene geothermometry of GRV 020175 gives a peak metamorphic temperature(～1000℃) and a closure temperature(～875℃).Molar Fe/Mn ratios(19-32) of pyroxenes are consistent with mesosiderite pyroxenes(16-35) and most plagioclase compositions(An_(87.5_96.6)) are within the range of mesosiderite plagioclase grains(An_(88-95)).Olivine composition(Fo_(53.8)) is only slightly lower than the range of olivine compositions in mesosiderites(Fo_(55-90)).All petrographic characteristics and chemical compositions of GRV 020175 are consistent with those of mesosiderite and based on its matrix texture and relatively abundant plagioclase,it can be further classified as a type 3A mesosiderite.Mineralogical, penological,and geochemical studies of GRV 020175 imply a complex formation history starting as rapid crystallization from a magma in a lava flow on the surface or as a shallow intrusion.Following primary igneous crystallization,the silicate underwent varying degrees of reheating.It was reheated to 1000℃,followed by rapid cooling to 875℃.Subsequently,metal mixed with silicate,during or after which,reduction of silicates occurred;the reducing agent is likely to have been sulfur.After redox reaction,the sample underwent thermal metamorphism,which produced the corona on the olivine, rims on the inverted pigeonite phenocrysts and overgrowths on the orthopyroxene phenocrysts,and homogenized matrix pyroxenes.Nevertheless,metamorphism was not extensive enough to completely reequilibrate the GRV 020175 materials. 相似文献
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铁陨石及中铁陨石的稀有气体同位素丰度和放射性核素活度 总被引：1，自引：0，他引：1
测定了两个铁陨石及两个中铁陨石的稀有气体同位素丰度和＾１０Ｂｅ、＾２６Ａｌ和＾３６Ｃｌ的放射性核素活度。在所研究的４个陨石中,东乌珠穆沁旗（类型Ⅰ）、渭源（类型Ⅲ）中铁陨石及宁波铁陨石（ⅣＡ）是在中国回收的,另一个无结构铁陨石Ｒａｆｒｕｔｉ是于１８８６年在瑞士发现的。根据＾１０Ｂｅ－＾２１Ｎｅ、＾２６Ａｌ－＾２１Ｎｅ和＾３６Ｃｌ－＾３６Ａｒ计算了两个铁陨石的产率及宇宙射线暴露年龄。其中Ｒａｆｒｕｔ 相似文献
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东乌旗中铁陨石为1995年在内蒙发现的、为数不多的降落型中铁陨石,由金属—硫化物和硅酸盐相紧密混合而成。硅酸盐相由角砾部分（主要为角砾状橄榄石和辉长岩岩屑）和非角砾部分组成。岩相学特征、主量元素成分及REE地球化学特征表明角砾状橄榄石、非角砾橄榄石和辉长质硅酸盐（辉长岩岩屑和除橄榄石外的非角砾部分）三者可能分别结晶自不同的岩浆源区。进一步的分析表明Mg含量非常高的角砾状橄榄石可能来自一个分异小行星的橄榄岩质地幔,非角砾橄榄石和辉长质硅酸盐可能和HED陨石具有相同的母体Vesta小行星。冲击碰撞导致两个小行星的物质发生了混合。冲击作用产生的高温（约1200℃—1450℃）使得被撞击小行星表壳玄武质和辉长质岩石发生混合重熔,熔体结晶后形成中铁陨石的辉长质硅酸盐。该温度下非角砾橄榄石和角砾状橄榄石均未发生重熔。该模型较好地解释了角砾状橄榄石、非角砾橄榄石和辉长质硅酸盐三者之间的不平衡现象。 相似文献
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东乌珠穆沁及渭源中铁陨石岩石学特征及其分类 总被引：4，自引：2，他引：2
对我国东乌珠穆沁及渭源２个中铁陨石的岩石学进行了研究,根据其硅酸盐基质的再结晶程度,我们将东乌珠穆沁陨石划分为类型Ｉ的中铁陨石,渭源陨石划分为类型Ⅲ的中铁陨石。东乌珠穆沁中铁陨石主要分布于细粒基质中的富斜方辉石碎屑及金属Ｆｅ－Ｎｉ组成,其硅酸盐质显示轻微的再结晶作用,渭源中铁陨石强烈风化并形成大量褐铁矿,该陨石主要由斜方辉石,斜长石组成,并有少量普通辉石,磷镁钙石,鳞石英及铁的氧化物;硅酸盐矿物广 相似文献
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The Dalgaranga meteorite crater, 100 km northeast of Yalgoo, Western Australia, was one of the first impact structures identified in Australia, the smallest isolated crater found in Australia, and the only confirmed crater in the world associated with a mesosiderite projectile. Seventeen years passed before the Dalgaranga meteorites were described in the scientific literature, and nearly 40 years passed before a survey of the structure was published. The reasons for the time gap were never explained and a number of factual errors about the discovery and early history remain uncorrected in the scientific literature. Using historical and archival documents, and discussions with people involved in Dalgaranga research, the reasons for this time gap are explained by a series of minor misidentifications and coincidences. The age of the crater has yet to be determined, but using published data, we estimate the projectile mass to be 500–1000 kg. 相似文献
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采用剖面中间浓度与镍纹石带宽度关系测定了东乌珠穆沁中铁陨石的金相冷却速率,其冷却速率介于0．05℃／Ma与0.02℃／Ma之间,采用铁纹石颗粒或铁纹石带中心镍含量与到最靠近铁纹石颗粒边界或镍纹石带高镍边的关系所获得的冷却速率介于0．1℃／Ma与0．01℃／Ma之间,并与根据镍纹石层纹的测定结果一致。两种方法的测定结果都表明,东乌珠穆沁中铁陨石比任何其他类型陨石更缓慢冷却（＜05℃／Ma）。根据东乌珠穆沁中铁陨石结构和岩石学特征及宇宙射线暴露年龄,该陨石经受了吸积熔融和分异作用-壳的重熔-局部冲击熔融-破裂和重新组合或重新吸积-开挖和喷射等复杂的演化历史。 相似文献
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