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Published on: August 18, 2022
Acetone-Water Interactions in Crystalline and Amorphous Ice Environments
Michelle R Brann1, Stephen P Hansknecht1, Mark Muir1
1The James Franck Institute and Department of Chemistry, The University of Chicago, 929 East 57th Street, Chicago, Illinois 60637, United States.
Acetone forms stronger hydrogen bonds with porous D2O ice than nonporous ice. This interaction is limited in porous ice due to pore blockage and low-temperature diffusion, impacting astrophysical models.
Area of Science:
- Astrochemistry
- Surface Science
- Spectroscopy
Background:
- Acetone is a common organic molecule found in astrophysical environments.
- Water ice, particularly D2O ice, serves as a crucial substrate for molecule interactions in space.
- Understanding these interactions is key to modeling chemical processes on icy dust grains.
Purpose of the Study:
- To systematically investigate the interaction between acetone and various D2O ice structures.
- To quantify the extent of hydrogen bonding between acetone and different ice morphologies.
- To elucidate the influence of ice porosity on acetone-ice interactions.
Main Methods:
- Time-resolved, in situ reflection absorption infrared spectroscopy (RAIRS) was employed.
- Acetone was deposited onto different D2O ice films: nonporous amorphous (np-ASW), crystalline (CI), and porous amorphous (p-ASW).
- RAIR spectra were analyzed to track changes in chemical bonds and hydrogen bonding.
Main Results:
- Acetone exhibited stronger hydrogen bonding with porous D2O ices compared to nonporous or crystalline ices.
- Hydrogen bonding was quantified by spectral shifts in the C=O region and reduction in dangling bond area.
- Increased porosity (70° vs 30° deposition) led to reduced hydrogen bonding, suggesting pore blockage and limited diffusion.
Conclusions:
- The porosity of D2O ice significantly influences acetone's hydrogen bonding behavior.
- Pore accessibility and diffusion limitations at low temperatures restrict acetone-ice interactions in porous structures.
- These findings provide quantitative insights crucial for accurate modeling of organic molecule interactions on astrophysical icy surfaces.
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