Identification of nitrogenous organic species in Titan aerosols analogs: Nitrogen fixation routes in early atmospheres

被引:23
作者
He, Chao [1 ,2 ]
Smith, Mark A. [1 ,2 ,3 ,4 ]
机构
[1] Univ Arizona, Dept Chem & Biochem, Tucson, AZ 85721 USA
[2] Univ Houston, Dept Chem, Houston, TX 77204 USA
[3] Univ Arizona, Dept Planetary Sci, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[4] Univ Houston, Dept Earth & Atmospher Sci, Houston, TX 77204 USA
关键词
Titan; Atmosphere; Organic chemistry; Prebiotic chemistry; AMINO-ACIDS; COUPLING PHOTOCHEMISTRY; HAZE FORMATION; N-15; NMR; THOLINS; CHEMISTRY; C-13; HCN; SIMULATION; PYROLYSIS;
D O I
10.1016/j.icarus.2013.05.013
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Titan, an icy world surrounded by auburn organic haze, is considered as one of the best targets for studying abiotic planetary organic chemistry. In spite of a great many efforts being made, the chemistry in Titan's atmosphere and its resulting chemical structures are still not fully understood. In our previous work, we have investigated the structure of Titan aerosols analogs (tholin) by NMR and identified hexamethylenetetramine as a dominant small molecule in Titan tholin. Here we report a more complete and definitive structural investigation of the small molecule inventory in Titan tholin. We identified several nitrogenous organic molecules including cyanamide, guanidine, 2-cyanoguanidine, melamine, N'-cyanoformamidine and 1,2,4-triazole in Titan tholin by using NMR and GC-MS and standard sample comparison. The structural characteristics of these molecules suggest a possible formation pathway from the reaction of HCN and NH3, both of which are known to exist in appreciable density in the atmosphere and were tentatively detected by the Huygens probe. (C) 2013 Elsevier Inc. All rights reserved.
引用
收藏
页码:33 / 40
页数:8
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