Hydrocarbons formation following UV photo-induced dissociation of CD 3 Cl trapped and caged inside thin amorphous solid water ͑ASW͒ layers on Ru͑001͒ has been measured for the first time under well-defined UHV conditions. Stable products such as C 2 D 6 , CHD 3 , CD 3 CD 2 Cl, CD 3 OH were detected via post-irradiation temperature programmed desorption. Specific reactivity pathways for the various photo-products were identified based on excitation wavelengths, ASW layer thickness, and parent molecules initial coverage dependence. Cross sections of (1-6) ϫ10 Ϫ19 cm 2 and (1-3)ϫ10 Ϫ20 cm 2 at 193 nm and 248, respectively, were measured. These photo-induced phenomena of caged molecules are discussed as a possible mechanism for the formation of hydrocarbons in interstellar space.