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Adsorption and Desorption of Mixed Ices
Cosmic Dust Adsorption and Desorption of Mixed Ices
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Experimental Aims Investigate the formation of methanol on dust grain surfaces Study the desorption characteristics of mixed ices using TPD Initially study methanol on a pre-dose of water ice Vary the pre-dose of water to study: Methanol on a thin layer of Water Ice Methanol on a thick layer of Water Ice
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Experimental Set-up UHV chamber with facilities to cool the sample to 10 – 20 K, coupled to an atom source Mimic conditions in ISM Reflection Absorption Infrared Spectroscopy (RAIRS) and Temperature Programmed Desorption (TPD) studies
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Temperature Programmed Desorption
Heat sample in a linear manner Monitor desorbing species with a QMS Adsorption kinetics can be determined by analysing the spectra.
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Methanol on Single Layer Ice
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Water Spectra: Single Layer
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Methanol on Single Layer: Summary
Layer of low density amorphous ice forms Monolayer of methanol on the water layer Multilayer methanol formation
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Methanol on Thick Layer Ice
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Water Spectra: Thick Layer
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Methanol on Thick Layer Summary
Thick layer of low density amorphous ice Methanol binds to pores in ice surface – dependent on ice thickness Monolayer of methanol on the water layer Multilayer methanol formation
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Summary of Mixed Ice Features
Methanol shows complex desorption features highlighting need for mixed ice studies Co-desorption feature possibly indicating trapping. Intensity dependent on thickness of water layer Monolayer on ice Multilayer Heavily influenced by H-bonding Methanol to H2O interaction > methanol to methanol
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Future work Analyse results
Repeat TPD with methanol and water co-adsorbed Vary proportions of the mixture RAIRS
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Acknowledgements Deep Bolina, Sabine Barjansky, Carolina Carlstedt
Wendy Brown UCL Centre for Cosmic Chemistry and Physics EPSRC Royal Society
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