Possible contribution of different energy sources to the production of organics in Titan's atmosphere

被引：29
|
作者：
Ramírez, SI
Navarro-González, R
Coll, P
Raulin, F
机构：
[1] Natl Autonomous Univ Mexico, Inst Ciencias Nucl, Lab Quim Plasmas & Estudios Planetarios, Mexico City 04510, DF, Mexico
[2] Univ Paris 12, Lab Interuniv Syst Atmospher, F-94010 Creteil, France
来源：
SPACE LIFE SCIENCES: LIFE IN THE SOLAR SYSTEM: PREBIOTIC CHEMISTRY, CHIRALITY AND SPACE BIOLOGY | 2001年 / 27卷 / 02期
关键词：
D O I：
10.1016/S0273-1177(01)00056-4
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
A quantitative comparison of the products arising from the irradiation of a Titan's simulated atmosphere is presented. The energy sources used represent some of the main events that occur in the satellite's atmosphere. All of the compounds identified are classified in the hydrocarbon and nitrile chemical families. Almost all of the detected compounds in Titan's atmosphere are produced by one or more energy sources. The compounds with the highest energy yields include the C-2 hydrocarbons, methanonitrile and ethanonitrile. The possibility of using some of the produced organics as tracer compounds during the Huygens descend to identify the leading energy form in the different atmospheric levels remains open. (C) 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：261 / 270
页数：10
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