The formation of CO 2 in quiescent regions of molecular clouds is not yet fully understood, despite CO 2 having an abundance of around 10%-34% H 2 O. We present a study of the formation of CO 2 via the nonenergetic route CO + OH on nonporous H 2 O and amorphous silicate surfaces. Our results are in the form of temperature-programmed desorption spectra of CO 2 produced via two experimental routes: O 2 + CO + H and O 3 + CO + H. The maximum yield of CO 2 is around 8% with respect to the starting quantity of CO, suggesting a barrier to CO + OH. The rate of reaction, based on modeling results, is 24 times slower than O 2 + H. Our model suggests that competition between CO 2 formation via CO + OH and other surface reactions of OH is a key factor in the low yields of CO 2 obtained experimentally, with relative reaction rates ofAstrophysically, the presence of CO 2 in low A V regions of molecular clouds could be explained by the reaction CO + OH occurring concurrently with the formation of H 2 O via the route OH + H.