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木卫二作为生命的栖息地。

Europa as an abode of life.

作者信息

Chyba Christopher F, Phillips Cynthia B

机构信息

Center for the Study of Life in the Universe, SETI Institute, Mountain View, CA, USA.

出版信息

Orig Life Evol Biosph. 2002 Feb;32(1):47-68. doi: 10.1023/a:1013958519734.

Abstract

Life as we know it on Earth depends on liquid water, a suite of 'biogenic' elements (most famously carbon) and a useful source of free energy. Here we review Europa's suitability for life from the perspective of these three requirements. It is likely, though not yet certain, that Europa harbors a subsurface ocean of liquid water whose volume is about twice that of Earth's oceans. Little is known about Europa's inventory of carbon, nitrogen, and other biogenic elements, but lower bounds on these can be placed by considering the role of commentary delivery over Europa's history. Sources of free energy are challenging for a world covered with an ice layer kilometers thick, but it is possible that hydrothermal activity and/or organics and oxidants provided by the action of radiation chemistry at Europa's surface and subsequent mixing into Europa's ocean could provide the electron donors and acceptors needed to power a Europan ecosystem. It is not premature to draw lessons from the search for life on Mars with the Viking spacecraft for planning exobiological missions to Europa.

摘要

我们所知的地球上的生命依赖于液态水、一系列“生物成因”元素(最著名的是碳)以及有用的自由能源。在此,我们从这三个要求的角度来审视木卫二是否适合生命存在。木卫二很可能(尽管尚未确定)拥有一个地下液态水海洋,其体积约为地球海洋的两倍。关于木卫二的碳、氮和其他生物成因元素的存量,我们所知甚少,但通过考虑在木卫二历史过程中物质输送的作用,可以确定这些元素的下限。对于一个覆盖着数公里厚冰层的世界来说,自由能源的来源颇具挑战性,但木卫二表面辐射化学作用产生的热液活动和/或有机物及氧化剂,以及随后混入木卫二海洋的情况,有可能提供为木卫二生态系统提供能量所需的电子供体和受体。借鉴“维京号”航天器在火星上寻找生命的经验来规划前往木卫二的外星生物学任务,并非为时过早。

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