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Complex organic matter in Titan's atmospheric aerosols from in situ pyrolysis and analysis.
Israël, G; Szopa, C; Raulin, F; Cabane, M; Niemann, H B; Atreya, S K; Bauer, S J; Brun, J-F; Chassefière, E; Coll, P; Condé, E; Coscia, D; Hauchecorne, A; Millian, P; Nguyen, M-J; Owen, T; Riedler, W; Samuelson, R E; Siguier, J-M; Steller, M; Sternberg, R; Vidal-Madjar, C.
Afiliación
  • Israël G; Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin, Verrières-le-Buisson, F 91371, France. Guy.israel@aerov.jussieu.fr
Nature ; 438(7069): 796-9, 2005 Dec 08.
Article en En | MEDLINE | ID: mdl-16319825
Aerosols in Titan's atmosphere play an important role in determining its thermal structure. They also serve as sinks for organic vapours and can act as condensation nuclei for the formation of clouds, where the condensation efficiency will depend on the chemical composition of the aerosols. So far, however, no direct information has been available on the chemical composition of these particles. Here we report an in situ chemical analysis of Titan's aerosols by pyrolysis at 600 degrees C. Ammonia (NH3) and hydrogen cyanide (HCN) have been identified as the main pyrolysis products. This clearly shows that the aerosol particles include a solid organic refractory core. NH3 and HCN are gaseous chemical fingerprints of the complex organics that constitute this core, and their presence demonstrates that carbon and nitrogen are in the aerosols.
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Colección: 01-internacional Base de datos: MEDLINE Asunto principal: Compuestos Orgánicos / Saturno / Medio Ambiente Extraterrestre Idioma: En Revista: Nature Año: 2005 Tipo del documento: Article País de afiliación: Francia Pais de publicación: Reino Unido
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Colección: 01-internacional Base de datos: MEDLINE Asunto principal: Compuestos Orgánicos / Saturno / Medio Ambiente Extraterrestre Idioma: En Revista: Nature Año: 2005 Tipo del documento: Article País de afiliación: Francia Pais de publicación: Reino Unido