1. Laboratory investigations of astrochemically relevant ices
- Author
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Ingman, Emily Rose
- Abstract
The mass of the interstellar medium (ISM) consists of 99% molecular gas and 1% dust grain particles. At the low temperatures and pressures of the ISM, molecules condense onto dust grains to form ice. Interstellar ices are most commonly processed via thermal radiation from nearby stars leading to the desorption of molecules into the gas phase and subsequent rich chemistry of space. This work uses surface science techniques such as temperature programmed desorption (TPD) and reflection absorption infrared spectroscopy (RAIRS) to characterise the adsorption and desorption behaviour of astrophysically relevant organic molecules including acetonitrile, acetaldehyde and acetone. Interstellar ices are multi-component in nature, primarily consisting of water in its amorphous and crystalline phases. Water is known to trap and subsequently affect the desorption of other species; therefore, the interactions between organic molecules and water have been investigated in order to provide a detailed overview of the desorption of astrophysically relevant ices. In addition to water, interstellar ices are comprised of methanol. Previous studies have demonstrated that the desorption kinetics of water are significantly altered due to the presence of methanol. Consequently, an investigation into the modified desorption of water in the presence of methanol was carried out. To provide a detailed insight into the desorption of astrochemically relevant ices, the impact of this modified behaviour on the trapping and subsequent desorption of more complex molecules such as acetone was also investigated. Although thermal processing is most common in interstellar environments, non-thermal desorption of ice has also been observed due to processing via charged particle interactions in the ISM with substantial experimental work also carried out to investigate the photodesorption of molecules due to vacuum ultraviolet (VUV) irradiation. Infrared (IR) light is also present in similar environments; however, it is often omitted from astrochemical models. This work aims to provide a deeper insight into the non-thermally induced diffusion and desorption of small species in order to tackle the current lack of understanding of non-thermal desorption in astrophysical environments. Ices consisting of CO and H2O were irradiated with infrared light using the free electron laser (FEL) at the FELIX Laboratory, Nijmegen. RAIRS and mass spectrometry were used to monitor the infrared-induced photodesorption. The laser-fluence dependence was investigated and desorption cross-sections were obtained in order to propose a detailed mechanism of the photodesorption taking place.
- Published
- 2023