Greenhouse warming by CH4 in the atmosphere of early Earth

被引:357
|
作者
Pavlov, AA
Kasting, JF
Brown, LL
Rages, KA
Freedman, R
机构
[1] Penn State Univ, Dept Geosci, University Pk, PA 16802 USA
[2] NASA, Ames Res Ctr, Space Phys Res Inst, Moffett Field, CA 94035 USA
关键词
D O I
10.1029/1999JE001134
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Earth appears to have been warm during its early history despite the faintness of the young Sun. Greenhouse warming by gaseous CO2 and H2O by itself is in conflict with constraints on atmospheric CO2 levels derived from paleosols for early Earth. Here we explore whether greenhouse warning by methane could have been important. We find that a CH4 mixing ratio of 10(-4)(100 ppmv) or more in Earth's early atmosphere would provide agreement with the paleosol data from 2.8 Ga. Such a CH4 concentration could have been readily maintained by methanogenic bacteria, which are thought to have been an important component of the biota at that time. Elimination of the methane component of the greenhouse by oxidation of the atmosphere at about 2.3 - 2.4 Ca could have triggered the Earth's first widespread glaciation.
引用
收藏
页码:11981 / 11990
页数:10
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