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彗星和彗尘中的有机物。

Organic matter in comets and cometary dust.

作者信息

Llorca Jordi

机构信息

Department of Inorganic Chemistry, University of Barcelona, Spain.

出版信息

Int Microbiol. 2005 Mar;8(1):5-12.

Abstract

Comets are primitive conglomerates of the solar system containing a mixture of frozen gases, refractory grains, and carbonaceous particles rich in biogenic elements. The dramatic display of comets is mostly caused by a cloud of micrometer-sized dust particles that leave the comet nucleus when frozen gases sublimate as they approach the Sun. Analyses of cometary dust captured in the stratosphere together with data obtained from space missions to comets have revealed the presence of a great variety of organic molecules. Since substantial amounts of cometary dust were gently deposited on Earth, their organic content could have played a major role in prebiotic processes prior to the appearance of microorganisms. This review discusses the description and implications for life of the organic content of comets and cometary dust.

摘要

彗星是太阳系的原始聚集体,包含冷冻气体、难熔颗粒和富含生物成因元素的碳质颗粒的混合物。彗星的壮观景象主要是由微米级尘埃颗粒云造成的,当冷冻气体在接近太阳时升华,这些尘埃颗粒就会离开彗核。对平流层中捕获的彗星尘埃的分析以及从彗星太空任务获得的数据表明,存在着各种各样的有机分子。由于大量彗星尘埃被轻柔地沉积在地球上,它们的有机成分可能在微生物出现之前的益生元过程中发挥了重要作用。这篇综述讨论了彗星和彗星尘埃有机成分的描述及其对生命的意义。

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