This works presents a perturbative analysis of the supersymmetric Chern-Simons model in three spacetime dimensions coupled to a Higgs field, using the superfield formalism. We study the spontaneous symmetry breaking of the U (1) gauge symmetry and evaluate the first quantum corrections to the effective action in the broken phase. We show that the infinite renormalization of the gap equation is enough to ensure the renormalizability of the model at the first loop level.PACS numbers: 1.15. Ex, 11.10.Gh,11.30.Pb,12.60.Jv Field theories in three-dimensional spacetime are often simpler than their similar four dimensional counterparts and, as such, can be regarded as useful laboratories for several field theoretical properties. In particular, induced by the Chern-Simons term [1, 2], three dimensional theories exhibit massive gauge fields, exotic statistics and fractional spin, relevant qualities for the study of the quantized Hall effect [3]. In the non-Abelian case, the invariance of the action under large gauge transformations requires the Chern-Simons coefficient to be quantized [1], an aspect that can be explicitly verified in perturbation theory [4,5].One interesting possibility that has been considered in the literature is the coupling of the ChernSimons term to a Higgs field (CSH), thus allowing for spontaneous gauge symmetry breaking to occur, and a nontrivial dynamics for the Chern-Simons gauge field to be settled (giving rise to a self-dual model, which happens to be equivalent to a Maxwell-Chern-Simons theory [6]). The quantization of the Chern-Simons coefficient for non-Abelian theories in the broken phase holds if the remaining gauge symmetry is non-Abelian [7,8], whereas such quantization does not happen in the case of an Abelian theory, or a completely broken non-Abelian gauge symmetry [9,10,11]. Also, for a specific form of the Higgs potential, the CSH model has solutions which satisfy a Bogomol'nyi equation [12,13]. The exact form of this potential can be obtained either by imposing a self-dual condition on the matter field [14] or by enlarging the model to obtain an N = 2 supersymmetric theory [15]. It is interesting to note that a tridimensional analog of the Coleman-Weinberg model in * Electronic address: lehum, alysson, mgomes, ajsilva@fma.if.usp.br