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以无光合作用的高温生存作为火星模型。

High-temperature life without photosynthesis as a model for Mars.

作者信息

Shock E L

机构信息

Department of Earth and Planetary Sciences, McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri, USA.

出版信息

J Geophys Res. 1997 Oct 25;102(E10):23687-94. doi: 10.1029/97je01087.

Abstract

Discoveries in biology and developments in geochemistry over the past two decades have lead to a radical revision of concepts relating to the upper temperature at which life thrives, the genetic relationships among all life on Earth, links between organic and inorganic compounds in geologic processes, and the geochemical supply of metabolic energy. It is now apparent that given a source of geochemical energy, in the form of a mixture of compounds that is far from thermodynamic equilibrium, microorganisms can take advantage of the energy and thrive without the need for photosynthesis as a means of primary productivity. This means that life can exist in the subsurface of a planet such as Mars without necessarily exhibiting a surface expression. Theoretical calculations quantify the geochemically provided metabolic energy available to hyperthermophilic organisms in submarine hydrothermal systems on the Earth, and help to explain the enormous biological productivity of these systems. Efforts to place these models in the context of the early Earth reveal that substantial geochemical energy would have been available and that organic synthesis would have been thermodynamically favored as hydrothermal fluids mix with seawater.

摘要

在过去二十年里,生物学领域的发现以及地球化学的发展,促使人们对以下相关概念进行了彻底修正:生命能够繁盛的最高温度、地球上所有生命之间的遗传关系、地质过程中有机化合物与无机化合物之间的联系以及代谢能量的地球化学供应。现在很明显,只要有以远离热力学平衡的化合物混合物形式存在的地球化学能量来源,微生物就可以利用这种能量并蓬勃发展,而无需光合作用作为主要生产力手段。这意味着生命可以存在于火星等行星的地下,而不一定在表面表现出来。理论计算量化了地球上海底热液系统中嗜热生物可利用的地球化学提供的代谢能量,并有助于解释这些系统巨大的生物生产力。将这些模型置于早期地球背景下的研究表明,当时会有大量的地球化学能量可用,并且随着热液与海水混合,有机合成在热力学上会受到青睐。

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