Encapsulation kinetics and dynamics of carbon monoxide in clathrate hydrate.
Nat Commun 2014;
5:4128. [PMID:
24936712 PMCID:
PMC4082632 DOI:
10.1038/ncomms5128]
[Citation(s) in RCA: 54] [Impact Index Per Article: 5.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/19/2013] [Accepted: 05/14/2014] [Indexed: 11/28/2022] Open
Abstract
Carbon monoxide clathrate hydrate is a potentially important constituent in the solar system. In contrast to the well-established relation between the size of gaseous molecule and hydrate structure, previous work showed that carbon monoxide molecules preferentially form structure-I rather than structure-II gas hydrate. Resolving this discrepancy is fundamentally important to understanding clathrate formation, structure stabilization and the role the dipole moment/molecular polarizability plays in these processes. Here we report the synthesis of structure-II carbon monoxide hydrate under moderate high-pressure/low-temperature conditions. We demonstrate that the relative stability between structure-I and structure-II hydrates is primarily determined by kinetically controlled cage filling and associated binding energies. Within hexakaidecahedral cage, molecular dynamic simulations of density distributions reveal eight low-energy wells forming a cubic geometry in favour of the occupancy of carbon monoxide molecules, suggesting that the carbon monoxide–water and carbon monoxide–carbon monoxide interactions with adjacent cages provide a significant source of stability for the structure-II clathrate framework.
Carbon monoxide clathrate hydrate has been widely studied and although the structure-II gas hydrate is predicted to be thermodynamically favourable, it is the structure-I hydrate that has been observed. Here, the authors synthesize the structure-II carbon monoxide hydrate and probe its structure and formation.
Collapse