The origin of methane and biomolecules from a CO2 cycle on terrestrial planets

被引:26
作者
Civis, Svatopluk [1 ]
Knizek, Antonin [1 ,2 ]
Ivanek, Ondrej [1 ]
Kubelik, Petr [1 ,3 ]
Zukalova, Marketa [1 ]
Kavan, Ladislav [1 ]
Ferus, Martin [1 ]
机构
[1] Czech Acad Sci, J Heyrovsky Inst Phys Chem, Dolejskova 3, CZ-18223 Prague 8, Czech Republic
[2] Charles Univ Prague, Fac Sci, Dept Phys & Macromol Chem, Albertov 2030, CZ-12840 Prague 2, Czech Republic
[3] Czech Acad Sci, Dept Radiat & Chem Phys, Inst Phys, Slovance 1999-2, CZ-18221 Prague 8, Czech Republic
关键词
HIGH-ENERGY CHEMISTRY; CARBON-DIOXIDE; MARTIAN SOIL; MARS; FORMAMIDE; EXCHANGE; TIO2; NUCLEOBASES; ATMOSPHERE; MOLECULES;
D O I
10.1038/s41550-017-0260-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Understanding the chemical evolution of newly formed terrestrial planets involves uncertainties in atmospheric chemical composition and assessing the plausibility of biomolecule synthesis. In this study, an original scenario for the origin of methane on Mars and terrestrial planets is suggested. Carbon dioxide in Martian and other planetary atmospheres can be abiotically converted into a mixture of methane and carbon monoxide by 'methanogenesis' on porous mineral photoactive surfaces under soft ultraviolet irradiation. On young planets exposed to heavy bombardment by interplanetary matter, this process can be followed by biomolecule synthesis through the reprocessing of reactive reducing atmospheres by impact-induced shock waves. The proposed mechanism of methanogenesis may help to answer the question concerning the formation of methane and carbon monoxide by photochemical processes, the formation of biomolecules on early Earth and other terrestrial planets, and the source and seasonal variation of methane concentrations on Mars.
引用
收藏
页码:721 / 726
页数:6
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