Laboratory studies of catalysis of CO to organics on grain analogs

被引:29
作者
Ferrante, RF [1 ]
Moore, MH
Nuth, JA
Smith, T
机构
[1] USN Acad, Dept Chem, Annapolis, MD 21402 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
基金
美国国家航空航天局;
关键词
atmospheric composition; atmospheric evolution; organic chemistry; prebiotic chemistry; solar nebula;
D O I
10.1006/icar.2000.6350
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Experiments simulating heterogeneous conversion of H-2 and CO into simple hydrocarbons in astrophysical environments have been performed, utilizing realistic cosmic grain analogs of Fe-doped silicates as Fischer-Tropsch-Type catalysts. Catalysis was studied for temperatures from 470-670 K and reactant gas mixtures of H-2/CO with a ratio of 2-100. The total gas pressure was near 0.5 bar. Maximum conversion rates of a few percentage points were achieved over a 3-h time period. Major products were methane, ethane, ethylene, carbon dioxide, and water. Products were identified by IR. spectroscopy. (C) 2000 Academic Press.
引用
收藏
页码:297 / 300
页数:4
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