We present a study investigating the impact of strong interactions on the bar structures of galaxies. Using Hubble SpaceTelescope (HST) deep field observations, we visually inspected a sample of 140 galaxies that show bridge features indicativeof interaction and 57 M51-type galaxies. Our analysis revealed a consistent bar fraction of of 16% across both samples,significantly lower than the bar fractions observed in isolated galaxies. Additionally, we found that bars are more likely to formand persist in nearby galaxies, with a clear decline at higher redshifts, and in larger, brighter galaxies with weaker interactions.In contrast, smaller and fainter galaxies are less likely to support bar structures due to the destabilizing effects of stronggravitational interactions. This result contributes to our understanding of the dynamics and structural evolution of galaxiesunder the influence of gravitational interactions.