科研之友
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摘要
Detection of life on other planets requires identification of biosignatures, i.e., observable planetary properties that robustly indicate the presence of a biosphere. One of the most widely accepted biosignatures for an Earth-like planet is an atmosphere where oxygen is a major constituent. Here we show that lifeless habitable zone terrestrial planets around any star type may develop oxygen-dominated atmospheres as a result of water photolysis, because the cold trap mechanism that protects H2O on Earth is ineffective when the atmospheric inventory of non-condensing gases ( e. g., N-2, Ar) is low. Hence the spectral features of O-2 and O-3 alone cannot be regarded as robust signs of extraterrestrial life.
- 出版日期2014-4-20
