Biology
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufm.p31c1550b&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #P31C-1550
Biology
[5200] Planetary Sciences: Astrobiology, [5215] Planetary Sciences: Astrobiology / Origin Of Life, [6281] Planetary Sciences: Solar System Objects / Titan
Scientific paper
Titan’s N2-CH4 atmosphere provides the starting material for a wide array of organic compounds to be formed via photochemistry, and the presence of unsaturated hydrocarbon, amine, and polycyclic aromatic species has been supported by data from the Cassini-Huygens mission [1,2]. Production of tholins by UV irradiation of a simulated N2-CH4 environment has yielded products that match the observed optical properties of Titan haze, suggesting that these compounds provide suitable analogs to Titan aerosol compounds [3, 4, 5]. Organics produced in Titan’s atmosphere eventually settle to the surface and very likely contribute to the particulate matter comprising the expansive longitudinal dune features observed at mid-latitudes [6]. Once on the surface, conditions that lead to incorporation of oxygen via contact with water ice or liquid water in Titan’s low temperature environment are of particular interest and have important implications for astrobiology [7; 8]. In this work, we postulate that the mechanical energy from wind-driven grains in the dunes of Titan can ultimately drive chemical processes and lead to the incorporation of oxygen into organic compounds via tribochemical reactions [9] and describe experiments designed to test this hypothesis. While the exact composition of the dunes of Titan is unknown, it is likely that they mainly comprise organic and water ice particles approximately 0.2 mm in diameter, the ideal size for saltation by the winds of Titan [6]. During the saltation process, organic particles undergo charging due to friction between particles, leading in turn to formation of ions and free radicals in localized electrical discharges at particle interfaces [10]. These reactive intermediates can initiate processes such as free radical and ionic polymerization that further transform organics. Of particular interest is the incorporation of oxygen into organic molecules, providing a pathway to the synthesis of biologically relevant compounds. Experiments modeling such systems are being conducted with laboratory-produced tholins and model unsaturated hydrocarbons, nitriles, imines, and aromatic compounds, and the results and implications of these studies will be presented. 1. Coates, A. J., A. Wellbrock, G. R. Lewis, G. H. Jones, D. T. Young, F. J. Crary, and J. H. Waite Jr (2009), Planet. Space Sci., 57(14-15), 1866-1871. 2. Crary, F. J., B. A. Magee, K. Mandt, J. H. Waite Jr, J. Westlake, and D. T. Young (2009), Planet. Space Sci., 57(14-15), 1847-1856. 3. Khare, B. N., C. Sagan, E. T. Arakawa, F. Suits, T. A. Callcott, and M. W. Williams (1984), Icarus, 60(1), 127-137. 4. Ramirez, S. I., P. Coll, A. da Silva, R. Navarro-González, J. Lafait, and F. Raulin (2002), Icarus, 156(2), 515-529. 5. Imanaka, H., and M. A. Smith (2010), Proc. Natl. Acad. Sci. U.S.A., 107(28), 12423-12428. 6. Lorenz, R. D., et al. (2006), Science, 312(5774), 724-727. 7. O'Brien, D. P., R. D. Lorenz, and J. I. Lunine (2005), Icarus, 173(1), 243-253. 8. Neish, C. D., A. Somogyi, and M. A. Smith (2010), Astrobiology, 10(3), 337-347. 9. Beyer, M. K., and H. Clausen-Schaumann (2005), Chem. Rev., 105(8), 2921-2948. 10. Kajdas, C., and K. Hiratsuka (2009), Proc. Inst. Mech. Eng., Part J, 223(6), 827-848.
Beauchamp J. L.
Thomas David A.
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