Restricted migration of reactive species limits chemical transformations within interstellar and cometary ices. We report the migration of CO from clathrate hydrate (CH) cages to amorphous solid water (ASW) in the presence of tetrahydrofuran (THF) under ultrahigh vacuum (UHV) and cryogenic conditions. Thermal annealing of sequentially deposited CO and HO ice, CO@HO, to 90 K resulted in the partitioning of CO in 5 and 56 CH cages (CO@5, CO@56). However, upon preparing a composite ice film composed of CO@5, CO@56 and THF distributed in the water matrix at 90 K, and annealing the mixture for 6 h at 130 K produced mixed CO-THF CH, where THF occupied the 56 cages (THF@56) exclusively while CO in 56 cages (CO@56) got transferred to the ASW matrix and CO in the 5 cages (CO@5) remained as is. This cage-matrix exchange may create a more conducive environment for chemical transformations in interstellar environments.
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http://dx.doi.org/10.1021/acs.jpclett.3c00373 | DOI Listing |
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