Chemical Structure and Optical Properties of Titan’s Tholins and “hcn Polymer”. Implications for the Analysis of Cassini-huygens Observations and Refractory Organics in Cometary
نویسندگان
چکیده
POLYMER”. IMPLICATIONS FOR THE ANALYSIS OF CASSINI-HUYGENS OBSERVATIONS AND REFRACTORY ORGANICS IN COMETARY GRAINS. E. Quirico, J-M Bernard, G. Montagnac, J-N Rouzaud, C. Szopa, G. Cernogora, B. Reynard, P. Mc Millan, N. Fray, B. Schmitt, P. Coll and F. Raulin. Laboratoire de Planétologie 38041 Grenoble Cedex France ([email protected]), Laboratoire de Sciences de la Terre ENS-Lyon 69364 Lyon Cedex 7 France, Laboratoire de Géologie ENS-Paris 75 Paris France, Service d’Aéronomie 91371 Verrières le Buisson Cedex France, University College of London UK, Laboratoire Interdisciplinaire des Systèmes Atmosphériques 94010 Créteil France.
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Introduction: The chemical compositions and structures of Titan’s aerosols are still unknown, so that the use of analogs formed in laboratory experiments is still necessary for atmospheric modeling and analysis of data from the space-based missions. Various different types of experiment have been carried out worldwide during the past 30 years to produce and evaluate such analogs, termed tholins...
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تاریخ انتشار 2006