2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/8073In this paper we report the multi-band BVRI photometry of HD 52452. The comparison of our data with previous observations reported by Messina et al. (2001) shows that there is a variation in amplitude, but the phases of the two minima, thus the positions of the spot, are quite stable during our observations.4 pages, 2 figures, IBVS No. 5553, 1Astrophysicstext