In this paper, we apply the recently found breakthrough topological method of Robson, Villari and Biancalana (RVB) [1,2] to the various black holes to derive their Hawking temperature. We show that the RVB method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the RVB method provides a consistent formula to achieve the Hawking temperature using the topology.