Ab initio calculations are used to investigate the energetics of the r
eaction of C-2(X (1) Sigma(g)(+)) with CH4. The heat of reaction is pr
edicted to be exothermic by 5.4 kcal mol(-1) and the barrier height is
0.2 kcal mol(-1) at the QCISD(T)/6-311++G(2df,2p)//UMP2/6-311G(2df,2p
) level of theory. The implications of the results are discussed in te
rms of their importance to the atmospheric evolution of ethane oceans
on Titan.