Pavlov A A, Kasting J F, Brown L L, Rages K A, Freedman R
Department of Geosciences, Pennsylvania State University, University Park, USA.
J Geophys Res. 2000 May 25;105(E5):11981-90. doi: 10.1029/1999je001134.
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 warming 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 Ga could have triggered the Earth's first widespread glaciation.
尽管早期太阳较为昏暗,但地球在其早期历史中似乎一直处于温暖状态。由气态二氧化碳和水导致的温室效应本身与从早期地球古土壤得出的大气二氧化碳水平限制相冲突。在此,我们探讨甲烷引起的温室效应是否重要。我们发现,地球早期大气中甲烷混合比达到10⁻⁴(100 ppmv)或更高,将与28亿年前的古土壤数据相符。这样的甲烷浓度本可由产甲烷细菌轻松维持,而产甲烷细菌被认为是当时生物群的重要组成部分。在大约23亿至24亿年前,大气氧化导致温室气体中的甲烷成分被消除,这可能引发了地球的首次广泛冰川作用。