In the recent years, driven by the increasingly stringent stability requirements imposed by some satellites' payloads (e.g. the new generation of optical instruments), the issue of accurate on-board spacecraft microvibration modelling has attracted signicant interest from engineers and scientists. This paper investigates the microvibrationinduced phenomenon on a cantilever congured reaction wheel assembly including sub and higher harmonic amplications due to modal resonances and broadband noise. A mathematical model of the reaction wheel assembly is developed and validated against experimental test results. The model is capable to represent each conguration in which the reaction wheel assembly will operate whether it is hard-mounted on a dynamometric platform or suspended free-free. The outcomes of this analysis are used to establish a novel methodology to retrieve the dynamic mass of the reaction wheel assembly in its operative range of speeds. An alternative measurement procedure has been developed for this purpose, showing to produce good estimates over a wide range of frequency using a less complex test campaign compared to typical dynamic mass setups. Furthermore, the gyroscopic eect inuence in the reaction wheel assembly response is thoroughly examined both analytically and experimentally. Finally, to what extent the noise aects the convergence of the novel approach is investigated.