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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Olivine-rich rims surrounding chondrules in the Mokoia CV3 carbonaceous chondrite: Further evidence for parent-body processes
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Olivine-rich rims surrounding chondrules in the Mokoia CV3 carbonaceous chondrite: Further evidence for parent-body processes

机译:Mokoia CV3碳质球粒陨石中的软骨圈周围富含橄榄石的轮辋:母体过程的进一步证据

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Fine-grained rims surrounding chondrules and inclusions in the Mokoia CV3 carbonaceous chondrite can be divided into phyllosilicate-rich and olivine-rich types. We present a petrographic and electron microscopic study of the olivine-rich rims and their host objects (referred to as chondrules/olivine-rich rims). The olivine-rich rims consist mainly of Fe-rich olivine and very minor phyllosilicate (saponite). Their host chondrules contain minor saponite and phlogopite, which resulted from aqueous alteration of anhydrous silicates. Mineralogical and compositional characteristics of the chondrules/olivine-rich rims suggest that they experienced mild thermal metamorphic effects. The rims commonly contain veins of coarse-grained Fe-rich olivine, magnetite, and Fe-(Ni) sulfides. The chondrules show abundant evidence of alteration along their peripheries, and the alteration textures suggest a mechanism for rim formation by replacement of the chondrules. Initially, enstatite and opaque nodules preferentially reacted to form coarse, platy, Fe-rich olivine crystals, which were subsequently divided into finer grains. Forsterite was also replaced by Fe-rich olivine. As the alteration advanced, these Fe-rich olivines were disaggregated, mixed with simultaneously produced saponite, and formed rims. In contrast, the surrounding matrix shows no evidence of such alteration and metamorphism. These observations indicate that the chondrules/olivine-rich rims did not experience these secondary processes in their present setting. The results suggest that the chondrules/olivine-rich rims experienced extensive replacement reactions in an environment in which aqueous fluids existed but only in minor amounts. They have probably also undergone simultaneous and/or subsequent mild thermal metamorphism. We suggest that the chondrules/olivine-rich rims are actually clasts transported from a relatively dry region in the parent body that was different from the region where Mokoia was finally lithified.
机译:Mokoia CV3碳质球粒陨石周围的细粒状边缘和夹杂物可以分为富含页硅酸盐和富含橄榄石的类型。我们对富橄榄石的轮辋及其宿主物体(称为软骨/富橄榄石的轮辋)进行岩相和电子显微镜研究。富含橄榄石的轮辋主要由富含铁的橄榄石和极少量的页硅酸盐(皂石)组成。他们的寄主软骨含有少量的皂石和金云母,这是由于无水硅酸盐的水蚀而产生的。软骨/富含橄榄石的轮缘的矿物学和组成特征表明它们经历了温和的热变质作用。轮辋通常包含富含粗铁的橄榄石,磁铁矿和Fe-(Ni)硫化物的粗纹。软骨显示出沿其周边发生改变的大量证据,并且改变纹理暗示了通过替换软骨形成边缘的机制。最初,顽辉石和不透明的结核优先反应形成粗大,板状,富铁的橄榄石晶体,随后将其分成更细的晶粒。镁橄榄石也被富含铁的橄榄石所代替。随着蚀变的进行,这些富铁橄榄石被分解,与同时产生的皂石混合,形成轮辋。相反,周围的矩阵没有证据表明这种改变和变质。这些观察结果表明,软骨/富含橄榄石的轮缘在当前环境下没有经历这些次要过程。结果表明,软骨/富含橄榄石的轮辋在存在水性流体但仅有少量流体的环境中经历了广泛的置换反应。它们也可能同时发生和/或随后发生轻微的热变质作用。我们建议,软骨/富含橄榄石的轮辋实际上是从母体相对干燥的区域运来的碎屑,该区域不同于Mokoia最终被石化的区域。

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