As the main destination of carbon in the destruction of methane in the atmosphere of Titan, ethane provides information about the carbon isotopic composition of the reservoir from which methane is replenished. If the amount of methane entering the atmosphere is presently equal to the amount converted to ethane, the 12C/13C ratio in ethane should be close to the ratio in the reservoir. We have measured the 12C/13C ratio in ethane both with Cassini CIRS1 and from the ground2 and find that it is very close to the telluric standard and outer planet values (89), consistent with a primordial origin for the methane reservoir. The lower 12C/13C ratio measured for methane by Huygens GCMS (82.3) can be explained if the conversion of CH4 to CH3 (and C2H6) favors 12C over 13C with a carbon kinetic isotope effect of 1.08. The time required for the atmospheric methane to reach equilibrium, i.e., for replenishment to equal destruction, is approximately 5 methane atmospheric lifetimes. 1Nixon et al., Icarus 195, 778 (2008). 2Jennings et al., Journal of Physical Chemistry A, in press (2009).
|Publicación||American Astronomical Society, DPS meeting #50|
|Estado||Published - 1 sep 2009|
|Publicado de forma externa||Sí|
Jennings, D. E., Nixon, C. A., Romani, P. N., Bjoraker, G. L., Sada, P. V., Lunsford, A. W., Boyle, R. J., Hesman, B. E., & McCabe, G. H. (2009). Ethane's 12C/13C Ratio in Titan: Implications for Methane Replenishment. American Astronomical Society, DPS meeting #50, 41. http://adsabs.harvard.edu/abs/2009DPS....41.3308J