期刊
ICARUS
卷 181, 期 1, 页码 320-322出版社
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2005.11.023
关键词
Mars; Mars; atmosphere; photochemistry; abundances; atmospheres
We suggest that the methane observed on Mars can be formed by photolysis of water vapor in the presence of CO, in addition to possible geological sources, rather than biologically. (c) 2005 Elsevier Inc. All rights reserved.
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