奥吉尔陨石中原核微生物化石

R. Hoover
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引用次数: 19

摘要

奥盖尔CI1陨石于1864年5月14日晚落在法国南部,是所有已知的碳质陨石中研究最广泛的陨石之一。环境和场发射扫描电子显微镜(ESEM和FESEM)对Orgueil陨石新断裂的内表面进行了研究,结果发现了大量不同种群的丝状原核微生物的化石遗骸。这些遗迹的分类和保存方式是多种多样的。一些遗骸表现出空心鞘的碳化,在其他情况下,遗骸与水溶性蒸发岩矿物(如硫酸镁或铵盐)一起过矿化。提供的图像和能谱数据记录了各种Orgueil微观结构:非生物蒸发岩矿物;pre-solar谷物;生物原性不确定的树状、卵状和富氟细丝。这些结果提供了在美国华盛顿毒药湖和西班牙萨拉戈萨Catalayud地区发现的原生隐盐岩、结晶性和纤维性泻湖中发现的非生物微观结构的大小、大小范围、形态和化学组成的信息。高分辨率ESEM和FESEM二次和背散射电子图像和能量色散x射线能谱(EDS)数据也将提供可识别的丝状蓝藻和其他原核微化石。在陨石岩石基质中发现的许多微化石在大小和微观结构上与已知的丝状蓝藻属和种一致。许多这些形式可以被认为是蓝藻属于秩序振荡科的形态型。这些大而复杂的微观结构与所检测的非生物矿物(隐石和纤维状体)明显不同。Orgueil陨石中许多保存完好的丝状形式嵌入岩石基质中,并表现出可识别的生物特征和EDS元素组成,这清楚地将它们与非生物微观结构区分开来。它们表现出分枝和不分枝的细丝;单株和多株被鞘的毛状体,具有专门的细胞和结构,用于生殖(如激虫和动虫)和固氮(异囊)。陨石形态也显示出运动性的证据(涌现的潮藻和中空的,卷曲的空鞘),它们经常在席子,联合体和微生物组合中被发现,这些组合与已知的现代蓝藻属和物种的关联和生态一致。在Orgueil陨石中也发现了与现代蓝藻席相关的缺氧层中典型存在的光养丝状原核生物相一致的更小的细丝。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fossils of Prokaryotic microorganisms in the Orgueil meteorite
The Orgueil CI1 meteorite, which fell in southern France on the evening of May 14, 1864, has been one of the most extensively studied of all known carbonaceous meteorites. Environmental and Field Emission Scanning Electron Microscopy (ESEM and FESEM) studies of freshly fractured interior surfaces of the Orgueil meteorite have resulted in the detection of the fossilized remains of a large and diverse population of filamentous prokaryotic microorganisms. The taphonomy and the modes of the preservation of these remains are diverse. Some of the remains exhibit carbonization of a hollow sheath and in other cases the remains are permineralized with watersoluble evaporite minerals, such as magnesium sulfate or ammonium salts. Images and EDS spectral data are provided documenting a variety of Orgueil microstructures: abiotic evaporite minerals; pre-solar grains; framboids, ovoids and fluorine-rich filaments of indeterminate biogenicity. These results provide information regarding the size, size range, morphologies and chemical compositions of abiotic microstructures found in native cryptohalite and crystalline and fibrous epsomites from Poison Lake, Washington, USA and Catalayud, Zaragoza, Aragon, Spain. High resolution ESEM and FESEM secondary and backscattered electron Images and Energy Dispersive X-ray Spectroscopy (EDS) data will also be presented of recognizable filamentous cyanobacteria and other prokaryotic microfossils. Many of the microfossils found embedded in the meteorite rock matrix are consistent in size and microstructure with known genera and species of filamentous cyanobacteria. Many of these forms can be recognized as morphotypes of cyanobacteria belonging to the Order Oscillatoriaceae. These large, complex microstructures are clearly distinguishable from the abiotic minerals examined - cryptohalite and fibrous epsomites. Many of the well-preserved filamentous forms in the Orgueil meteorite are embedded in the rock matrix and exhibit identifiable biological characteristics and EDS elemental compositions that clearly differentiate them from abiotic microstructures. They exhibit branched and unbranched filaments; uniseriate and multiseriate ensheathed trichomes with specialized cells and structures for reproduction (e.g. hormogonia and akinetes) and nitrogen fixation (heterocysts). The meteorite forms also show evidence of motility (emergent hormogonia and hollow, coiled empty sheaths) and they are often found in mats, consortia and microbial assemblages that are consistent with the known associations and ecologies of modern genera and species of cyanobacteria. Smaller filaments, consistent with the phototrophic filamentous prokaryotes typically present in anoxic layers associated with modern cyanobacterial mats, have also been found in the Orgueil meteorite.
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