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地球与木卫二上的生物发生及早期生命:碱性海洋是其有利条件吗?

Biogenesis and early life on Earth and Europa: favored by an alkaline ocean?

作者信息

Kempe Stephan, Kazmierczak Jozef

机构信息

Institute of Applied Geosciences, University of Technology Darmstadt, Darmstadt, Germany.

出版信息

Astrobiology. 2002 Spring;2(1):123-30. doi: 10.1089/153110702753621394.

Abstract

Recent discoveries about Europa--the probable existence of a sizeable ocean below its ice crust; the detection of hydrated sodium carbonates, among other salts; and the calculation of a net loss of sodium from the subsurface--suggest the existence of an alkaline ocean. Alkaline oceans (nicknamed "soda oceans" in analogy to terrestrial soda lakes) have been hypothesized also for early Earth and Mars on the basis of mass balance considerations involving total amounts of acids available for weathering and the composition of the early crust. Such an environment could be favorable to biogenesis since it may have provided for very low Ca2+ concentrations mandatory for the biochemical function of proteins. A rapid loss of CO2 from Europa's atmosphere may have led to freezing oceans. Alkaline brine bubbles embedded in ice in freezing and impact-thawing oceans could have provided a suitable environment for protocell formation and the large number of trials needed for biogenesis. Understanding these processes could be central to assessing the probability of life on Europa.

摘要

近期对木卫二的发现——其冰壳下可能存在一个相当大的海洋;检测到水合碳酸钠及其他盐类;以及对地下钠净损失的计算——表明存在一个碱性海洋。基于涉及可用于风化的酸总量和早期地壳成分的质量平衡考虑,早期地球和火星也被假设存在碱性海洋(类比地球上的苏打湖,昵称为“苏打海洋”)。这样的环境可能有利于生物起源,因为它可能提供了蛋白质生化功能所必需的极低钙离子浓度。木卫二大气中二氧化碳的快速流失可能导致海洋冻结。在冻结和解冻的海洋中,嵌入冰中的碱性盐水泡可能为原细胞形成和生物起源所需的大量试验提供了适宜环境。了解这些过程可能是评估木卫二上存在生命可能性的核心。

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