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大西洋东北部珊瑚斑块海山枕状玄武岩中的潜在化石内栖生物。

Potential fossil endoliths in vesicular pillow basalt, Coral Patch Seamount, eastern North Atlantic Ocean.

机构信息

Department of Geology, University of Johannesburg, Johannesburg, South Africa.

出版信息

Astrobiology. 2011 Sep;11(7):619-32. doi: 10.1089/ast.2011.0657. Epub 2011 Aug 29.

DOI:10.1089/ast.2011.0657
PMID:21875356
Abstract

The chilled rinds of pillow basalt from the Ampère-Coral Patch Seamounts in the eastern North Atlantic were studied as a potential habitat of microbial life. A variety of putative biogenic structures, which include filamentous and spherical microfossil-like structures, were detected in K-phillipsite-filled amygdules within the chilled rinds. The filamentous structures (∼2.5 μm in diameter) occur as K-phillipsite tubules surrounded by an Fe-oxyhydroxide (lepidocrocite) rich membranous structure, whereas the spherical structures (from 4 to 2 μm in diameter) are associated with Ti oxide (anatase) and carbonaceous matter. Several lines of evidence indicate that the microfossil-like structures in the pillow basalt are the fossilized remains of microorganisms. Possible biosignatures include the carbonaceous nature of the spherical structures, their size distributions and morphology, the presence and distribution of native fluorescence, mineralogical and chemical composition, and environmental context. When taken together, the suite of possible biosignatures supports the hypothesis that the fossil-like structures are of biological origin. The vesicular microhabitat of the rock matrix is likely to have hosted a cryptoendolithic microbial community. This study documents a variety of evidence for past microbial life in a hitherto poorly investigated and underestimated microenvironment, as represented by the amygdules in the chilled pillow basalt rinds. This kind of endolithic volcanic habitat would have been common on the early rocky planets in our Solar System, such as Earth and Mars. This study provides a framework for evaluating traces of past life in vesicular pillow basalts, regardless of whether they occur on early Earth or Mars.

摘要

对北大西洋东部安普尔珊瑚斑块深海平顶山枕状玄武岩的冷壳进行了研究,将其作为微生物生命的潜在栖息地。在冷壳的填隙磷钙铝石杏仁体中检测到了各种假定的生物成因结构,包括丝状和球形微化石状结构。丝状结构(直径约 2.5 μm)呈磷钙铝石管,周围环绕着富含 Fe-氢氧化物(纤铁矿)的膜状结构,而球形结构(直径 4 至 2 μm)则与 Ti 氧化物(锐钛矿)和含碳物质有关。有几条证据表明,枕状玄武岩中的微化石状结构是微生物的化石遗骸。可能的生物特征包括球形结构的含碳性质、它们的大小分布和形态、天然荧光的存在和分布、矿物学和化学成分以及环境背景。综合来看,这组可能的生物特征支持这样一种假设,即化石状结构具有生物起源。岩石基质的泡状微生境可能曾经是 cryptoendolithic 微生物群落的栖息地。这项研究记录了各种证据,证明在迄今为止研究甚少且被低估的微环境中存在过去的微生物生命,这些证据来自冷枕状玄武岩冷壳中的杏仁体。这种内生火山栖息地在我们太阳系的早期岩石行星上很常见,如地球和火星。这项研究为评估在泡状枕状玄武岩中过去生命的痕迹提供了一个框架,无论它们是在早期的地球还是火星上形成的。

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