Preliminary Results from a New Titan Atmospheric Model

Details Preliminary Results from a New Titan Atmospheric Model Preliminary Results from a New Titan Atmospheric Model

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dps....42.5803a&link_type=abstract

American Astronomical Society, DPS meeting #42, #58.03; Bulletin of the American Astronomical Society, Vol. 42, p.1082

Biology

Scientific paper

A new comprehensive Titan atmospheric model has been developed as part of the NASA Astrobiology Institute JPL-Titan team effort to understand the complexity of organic chemistry in the combined Titan atmosphere/surface system. Details of this model are available in Willacy et al. (poster this conference). In this talk, preliminary results will be presented from the atmospheric simulation. We will discuss the flux of molecular hydrogen in the lower atmosphere, the partitioning of carbon in material settling on the surface, and the relative upper atmosphere/lower atmosphere source for this material.

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