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火星、早期地球和木卫二的生物潜力。

The biological potential of Mars, the early Earth, and Europa.

作者信息

Jakosky B M, Shock E L

机构信息

Department of Geological Sciences, University of Colorado, Boulder, USA.

出版信息

J Geophys Res. 1998 Aug 25;103(E8):19359-64. doi: 10.1029/98je01892.

Abstract

The potential biomass that could have existed on Mars is constrained by the total amount of energy available to construct it. From an inventory of the available geochemical sources of energy, we estimate that from the time of the onset of the visible geologic record 4 b.y. ago to the present, as much as 20 g cm-2 of biota could have been created. This is the same amount that could have been constructed on the early Earth in only 100 million years. This indicates that there likely was sufficient energy available to support an origin of life on Mars but not sufficient energy to create a ubiquitous and lush biosphere. Similar calculations for Europa suggest that even less would have been available there.

摘要

火星上可能存在的生物量受到构建它所需的总能量的限制。根据可用的地球化学能源清单,我们估计,从40亿年前可见地质记录开始到现在,火星上可能已经产生了多达20克/平方厘米的生物群。这与早期地球上仅在一亿年时间内可能构建的生物量相同。这表明火星上可能有足够的能量支持生命起源,但没有足够的能量创造一个无处不在且繁茂的生物圈。对木卫二进行的类似计算表明,那里可用的能量甚至更少。

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