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Which Tholins for Simulating Titan's Aerosols?

Jean-Michel Bernard 1 Eric Quirico 1 Gilles Montagnac 2 Bruno Reynard 2 P. Mc Millan 3 Lydie Bonal 1 J.-N. Rouzaud 4 P. Coll 5 Bernard Schmitt 1
1 LPG - Laboratoire de Planétologie de Grenoble
2 LST - Laboratoire de Sciences de la Terre
3 Department of Chemistry [UCL, London]
4 LGENS - Laboratoire de géologie de l'ENS
5 LISA (UMR_7583) - Laboratoire Interuniversitaire des Systèmes Atmosphériques
Abstract : The exploration of Titan by the Cassini-Huygens mission includes different spectrometers covering the visible and infrared ranges which will probe the atmosphere and the surface (DISR/CIRS).
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Conference papers
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https://hal-insu.archives-ouvertes.fr/insu-00355968
Contributor : Béatrice Pibaret-Bourdon Connect in order to contact the contributor
Submitted on : Monday, January 26, 2009 - 12:59:13 PM
Last modification on : Friday, October 15, 2021 - 1:37:54 PM

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  • HAL Id : insu-00355968, version 1

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Citation

Jean-Michel Bernard, Eric Quirico, Gilles Montagnac, Bruno Reynard, P. Mc Millan, et al.. Which Tholins for Simulating Titan's Aerosols?. 36th Lunar and Planetary Science Conference, 2005, Houston, United States. pp. 2. ⟨insu-00355968⟩

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