The interaction between ore-bearing fluids and the siliciclastic rocks typically hosting orogenic gold deposits in Phanerozoic metamorphic terrains result in the development of a distinctive alteration halo. Along with petrological changes such as the replacement of chlorite by carbonate and the growth of sericite, characteristic geochemical modifications take place within this alteration envelope. These include variations in elemental abundances and more or less pronounced shifts in the H, C, N, O, and S isotopic signature of the ore system. Fingerprinting' these isotopic trends can provide exploration with additional vectors towards the ore zone, and yields valuable information regarding the source of the hydrothermal fluids and the solutes contained therein. Data from radiogenic isotope systems such as Sr-Rb, Ar-Ar, Xe-Ra, Pb-Pb, Re-Os, Sm-Nd, and U-Pb can constrain the kinematic history of ore-hosting structures, provide important clues concerning the absolute timing of gold emplacement, and enable the detailed characterisation of associated intrusives with respect to their magma source(s) and crystallisation age. Although high analytical costs, long turn-around times and the potential for misinterpretation prevent isotope systems from offering a quick & dirty' analytical method that would provide a significant advantage in exploration for orogenic gold mineralisation, the development of integrated four-dimensional ore genesis models depends heavily on constraints obtained from isotope mass spectrometry.