LABORATORY SIMULATIONS OF TITANS ATMOSPHERE - ORGANIC GASES AND AEROSOLS

Titan, the main satellite of Saturn, has been observed by remote sensi ng for many years, both from interplanetary probes (Pioneer and Voyage r's flybys) and from the Earth. Its N-2 atmosphere, containing a small fraction of CH4 (approximate to 2%), with T approximate to 90 K and P approximate to 1.5 bar at the ground level, is irradiated by solar UV photons and deeply bombarded by energetic particles, i.e. Saturn magn etospheric electrons and protons, interplanetary electrons and cosmic rays. The resulting energy deposition, which takes place mainly below 1000 km, initiates chemical reactions which yield gaseous hydrocarbons and nitriles and, through polymerisation processes, solid aerosol par ticles which grow by coagulation and settle down to the ground. At the present time, photochemical models strongly require the results of sp ecific laboratory studies. Chemical rate constants are not well known at low temperatures, charged-particle-induced reactions are difficult to model and laboratory simulations of atmospheric processes are there fore of great interest. Moreover, the synthesis of organic compounds w hich have not been detected to date provides valuable information for future observations. The origin and chemical composition of aerosols d epend on the nature of chemical and energy sources. Their production f rom gaseous species may be monitored in laboratory chambers and their optical or microphysical properties compared to those deduced from the observations of Titan's atmosphere. The development of simulation cha mbers of Titan's extreme conditions is necessary for a better understa nding of past and future observations. Space probes will sound Titan's atmosphere by remote sensing and in situ analysis in the near future (Cassini-Huygens mission). It appears necessary, as a preliminary step , to test on-board experiments in such chambers, and as a final step, when new space data have been acquired, to use them for more general s cientific purposes.