Methane on Mars:: A product of H2O photolysis in the presence of CO

被引:23
作者
Bar-Nun, A [1 ]
Dimitrov, V [1 ]
机构
[1] Tel Aviv Univ, Dept Geophys & Planetary Sci, IL-69978 Tel Aviv, Israel
基金
以色列科学基金会;
关键词
Mars; atmosphere; photochemistry; abundances; atmospheres;
D O I
10.1016/j.icarus.2005.11.023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:320 / 322
页数:3
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