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

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).

Domaines: Planète et Univers [physics]

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⟩