Gas trapping by clathrate-hydrate formation in low temperature "cometary" water ice has been quoted repeatedly, especially regarding CO. However, of the plethora of gases detected in Comets Halley, Hyakutake, and Hale-Bopp, only methanol (CH 3 OH) and hydrogen sulfide (H 2 S) were shown experimental
The mechanism of methanol formation and other reactions following formaldehyde adsorption on Ni(110)
✍ Scribed by J. Thomas Dickinson; Robert J. Madix
- Publisher
- John Wiley and Sons
- Year
- 1978
- Tongue
- English
- Weight
- 611 KB
- Volume
- 10
- Category
- Article
- ISSN
- 0538-8066
No coin nor oath required. For personal study only.
✦ Synopsis
Abstract
The adsorption/desorption and reactive behavior of formaldehyde was studied on clean single‐crystal Ni(110) at adsorption temperatures down to 200 °K. For low exposures of the surface to formaldehyde, hydrogen and CO binding states were populated due to decomposition of the molecule upon adsorption. Higher exposures gave rise to a decomposition‐limited hydrogen peak exhibiting an activation energy of 20 kcal/gmol and an apparent frequency factor of 10^14^ sec^−1^. At initial coverages of H~2~CO exceeding about 0.5, monolayer methanol was observed to form. The formation of methanol involved a hydrogen atom transfer between two adsorbed H~2~CO molecules and did not occur totally via surface hydrogen. Self‐oxidation to form CO~2~ was also observed. The surface exhibited reaction heterogeneity, and the surface reactivity was observed to depend on the temperature of adsorption of reactants, suggesting strong adsorbate‐induced surface “reconstruction.”
📜 SIMILAR VOLUMES