Super star clusters dominate the dynamics and evolution in the central region of the galaxy NGC 1569. Recent studies have determined different ages and complex morphology within the clusters, allowing to create complicated structures of gas related with superbubbles, HII regions and the gas leftover from star formation. Using 3-D hydrodynamic techniques, I have studied the formation of a second star cluster very near to an existing massive star cluster in NGC 1569. The two star clusters are separated by a mere 3 pc in projection and have an age difference of only 3 Myr. This study provides insights into the viability of the second cluster's formation in a challenging environment influenced by the feedback from the first star cluster