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         Title:  The atmosphere and surface of Titan
        investigated from the ground and from space 
        Author(s):   A. Coustenis (Poster)
         ABSTRACT 
          Titan,
        Saturn’s largest satellite is currently the only confirmed exobiotical
        environment known to us. It is also perhaps the most intriguing object
        in our Solar System. Its uncanny resemblance to our own planet has
        motivated generations of scientists into studying it from both the space
        and from the ground, and has initiated the Saturn-bound Cassini/Huygens
        ESA/NASA mission (arrival at Titan is scheduled for end of 2004). 
          In the meantime, Titan is observed from the ground (using large
        telescopes, such as those in Hawaii and Chile), but also from space
        (initially with Voyager 1 and 2, with the HST, and recently with ISO). 
        
         
          Thus, we know today that the thick atmosphere layer covering the
        yet-to-be-determined satellite’s surface, is essentially made of
        nitrogen, with small amounts of methane and hydrogen. The combination
        among these mother molecules yields an exciting organic chemistry in
        Titan’s atmosphere, with hydrocarbons and nitriles (one of the latter,
        HCN, is a prebiotic molecule). As a difference with our own planet one
        should mention the absence of significant amounts of oxygen (only traces
        of CO, CO2 and more recently, H2O have been
        discovered), as well as the low temperatures prevailing (180 K in the
        atmosphere and 94 K on the surface) that delay chemical reactions. 
          Titan’s surface is hidden under a veil of a thick aerosol
        cloud, but recently, spectroscopy and imaging of the satellite in the
        near-IR have shown that this surface is inhomogeneous, bright on the
        leading side and darker on the trailing one. A large, bright, equatorial
        region - possibly connected with relief - is found on the leading
        hemisphere, while bright areas are also observed near the poles. The
        exact nature of this ground remains to be discovered, but is probably a
        mixture of ices (H2O, CH4, CO2...),
        hydrocarbon liquid and rocks.  
          We
        will discuss the implications of recent observations on the nature and
        the origins of Titan and its connection with our own planet.
        
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