Tidal forces from a binary companion can significantly stretch a star, impacting its magnetic field and the dynamics of its collapse during a supernova. The deformation caused by these forces may lead to changes in the star's magnetic field strength and configuration, potentially influencing the supernova explosion mechanism. Additionally, the interaction between the star's magnetic field and its material can affect the energy distribution during collapse. Understanding these effects is crucial for predicting supernova behavior and the resulting phenomena. The relationship between tidal forces and stellar evolution remains a key area of astrophysical research.