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We present a progress report of a project to study the quantitative starformation history (SFH) in different parts of the Small Magellanic Cloud (SMC).We use the information in [(B-R), R] color-magnitude diagrams (CMDs), whichreach down to the oldest main-sequence turnoffs and allow us to retrieve theSFH in detail. We show the first results of the SFH in a SMC field located inthe Southern direction (at $\thicksim$1 kpc from the SMC center). This field isparticularly interesting because in spite of being located in a place in whichthe HI column density is very low, it still presents a recent enhancement ofstar formation.Comment: Poster presented at: Stellar Populations as Building Blocks of  Galaxies, Proceedings IAU Symposium No. 241, 200

The Star Formation History in a SMC field: IAC-star/IAC-pop at work