Diffusion and Clustering of Carbon Dioxide on non-porous Amorphous Solid Water
arXiv:1611.02182 · doi:10.3847/1538-4357/aa5f52
Abstract
Observations by ISO and Spitzer towards young stellar objects (YSOs) showed that CO segregates in the icy mantles covering dust grains. Thermal processing of ice mixture was proposed as responsible for the segregation. Although several laboratory studied thermally induced segregation, a satisfying quantification is still missing. We propose that the diffusion of CO along pores inside water ice is the key to quantify segregation. We combined Temperature Programmed Desorption (TPD) and Reflection Absorption InfraRed Spectroscopy (RAIRS) to study how CO molecules interact on a non-porous amorphous solid water (np-ASW) surface. We found that CO diffuses significantly on a np-ASW surface above 65~K and clusters are formed at well below one monolayer. A simple rate equation simulation finds that the diffusion energy barrier of CO on np-ASW is 215050 K, assuming a diffusion pre-exponential factor of 10 s. This energy should also apply to the diffusion of CO on wall of pores. The binding energy of CO from CO clusters and CO from HO ice have been found to be and ~K, respectively, assuming the same prefactor for desorption. CO-CO interaction is stronger than CO-HO interaction, in agreement with the experimental finding that CO does not wet np-ASW surface. For comparison, we carried out similar experiments with CO on np-ASW, and found that the CO-CO interaction is always weaker than CO-HO. As a result, CO wets np-ASW surface. This study should be of help to uncover the thermal history of CO on the icy mantles of dust grains.
arXiv comment8 pages, 11 figures, submitted to ApJ
References in corpus (10)
- Observations of the Icy Universe
- The c2d Spitzer spectroscopic survey of ices around low-mass young stellar objects II: CO2
- A 3-5 micron VLT spectroscopic survey of embedded young low mass stars I: Structure of the CO ice
- Thermal desorption characteristics of CO, O2 and CO2 on non-porous water, crystalline water and silicate surfaces at sub-monolayer and multilayer coverages
- Quantification of segregation dynamics in ice mixtures
- Binding Energy of Molecules on Water Ice: Laboratory Measurements and Modeling
- CO diffusion into amorphous H2O ices
- Sticking of molecules on non-porous amorphous water ice
- The Nature of Carbon Dioxide Bearing Ices in Quiescent Molecular Clouds
- Interactions of adsorbed CO on water ice at low temperatures
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- Mid-IR and VUV Spectroscopic Characterisation of Thermally Processed and Electron Irradiated CO2 Astrophysical Ice Analogues
- Characterization of thin film CO ice through the infrared combination mode
- Spectroscopic measurements of CHOH in layered and mixed interstellar ice analogues
- The formation of CO through consumption of gas-phase CO on vacuum-UV irradiated water ice
- Molecular Mobility of Extraterrestrial Ices: Surface Diffusion in Astrochemistry and Planetary Science
- Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content
- Ammonia, carbon dioxide and the non-detection of the 2152 cm CO band
- New measurement of the diffusion of carbon dioxide on non-porous amorphous solid water
- Theoretical computations on the efficiency of acetaldehyde formation on interstellar icy grains