Organic Chemistry and Exobiology on Titan |
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Authors: | Raulin François Owen Tobias |
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Institution: | (1) LISA, CNRS & Universités Paris 12 et Paris 7, Avenue du général de Gaulle, 94010 Créteil Cedex, France;(2) Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA |
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Abstract: | Exobiology is not only the study of the origin, distribution and evolution of life in the universe, but also of structures
— including at the molecular level, and processes — including organic chemical transformations — related to life. In that
respect, with its dense nitrogen atmosphere, which includes a noticeable fraction of methane, and the many organic compounds
which are present in the gas and aerosols phases, Titan appears to be a planetary object of prime interest for exobiology
in the Solar system, allowing the study of chemical organic evolution in a planetary environment over a long time scale. We
describe here some aspects of this extraterrestrial organic chemistry which involves many physical and chemical couplings
in the different parts of what can be called ‘Titan's geofluid’ (gas phase, aerosol phases and surface solid and maybe liquid
phases). The three complementary approaches which can be followed to study such chemistry of exobiological interest are considered.
Those are experimental simulations in the laboratory, chemical and photochemical modeling and of course observation, using
both remote sensing and in situ measurements, which is an essential approach. The Cassini-Huygens mission, that offers a unique
opportunity to study in detail the many aspects of Titan's organic chemistry, is discussed and the many expected exobiological
returns from the different instruments of the Cassini orbiter and the Huygens probe are considered.
This revised version was published online in August 2006 with corrections to the Cover Date. |
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