This dissertation is an experimental study of the factors responsible for the state of water ice in extraterrestrial environments, and the changes induced in these ices due to pervasive space phenomena such as thermal processing and UV and energetic particle irradiation. The properties of frozen water are strongly dependent on the astronomical environment that harbors the ice. Ice morphology, phase, and chemical composition continually evolve due to processes such as thermal cycling, exposure to exospheric gases, and interaction with cosmic rays and stellar UV and particle fluxes. In this project, analytical techniques such as quartz crystal microgravimetry, infrared spectroscopy, ultraviolet-visible spectroscopy, and mass spectrometry were used in tandem to probe physical and chemical changes induced in laboratory-scale analogs of astronomical ices First, we characterized the transformation of amorphous ice to the cubic crystalline phase, CHAPTER 3