During this project, we developed new methods for mixing ‘water-hating’ carbon materials and ice - effectively making a comet in the lab. Using highly specialised neutron techniques, we studies the structure of water surrounding the carbon molecules. A plethora of diverse structures was discovered and we observed the onset of the often-discussed cross-over from small molecules towards water-repelling surfaces. Furthermore, we studied the effects of the carbon species on the phase transitions of the ice and the thermal desorption properties as it would be observed on comets. As part of our efforts to mix carbon species and ice, we found that ball-milling at low temperatures produces a new form of ice, medium-density amorphous ice, that may enable us to understand the many anomalies of liquid water in the future. Furthermore, we showed that ice can be a high-energy geophysical material under certain conditions. In addition to the work on carbon species, we showed that ammonium fluoride has an enormous impact on the phase transitions of ice and we also conducted detailed studies into the effects of acid and base dopants. In summary, this project has given new insights into the properties of the all-important H2O molecule in its condensed states and the effects other chemical species can have on ice. The results are important with respect to space research, the hydration of biomolecules and the formation of ice in clouds.