Hydrogen consumptions by methanogens on the early earth

被引:81
作者
Kral, TA [1 ]
Brink, KM
Miller, SL
McKay, CP
机构
[1] Univ Arkansas, Dept Biol Sci, Fayetteville, AR 72701 USA
[2] University California San Diego, Dept Chem & Biochem, La Jolla, CA 92093 USA
[3] NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
来源
ORIGINS OF LIFE AND EVOLUTION OF THE BIOSPHERE | 1998年 / 28卷 / 03期
基金
美国国家航空航天局;
关键词
D O I
10.1023/A:1006552412928
中图分类号
Q [生物科学];
学科分类号
07 ; 0710 ; 09 ;
摘要
It is possible that the first autotroph used chemical energy rather than light. This could have been the main source of primary production after the initial inventory of abiotic organic material had been depleted. The electron acceptor most readily available for use by this first chemoautotroph would have been CO2. The most abundant electron donor may have been H-2 that would have been outgassing from volcanoes at a rate estimated to be as large as 10(12) moles yr(-1), as well as from photo-oxidation of Fe+2. We report here that certain methanogens will consume H-2 down to partial pressures as low as 4 Pa (4 X 10(-5) atm) with CO2 as the sole carbon source at a rate of 0.7 ng H-2 min(-1) mu g(-1) cell protein. The lower limit of pH(2) for growth of methanogens can be understood on the basis that the pH(2) needs to be high enough for one ATP to be synthesized per CO2 reduced. The pH(2) values needed for growth measured here are consistent with those measured by Stevens and McKinley for growth of methanogens in deep basalt aquifers. H-2-consuming autotrophs are likely to have had a profound effect on the chemistry of the early atmosphere and to have been a dominant sink for H-2 on the early Earth after life began rather than escape from the Earth's atmosphere to space.
引用
收藏
页码:311 / 319
页数:9
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