Escape velocity at 1 Planck length from an event horizon can be approximated using the equation for gamma, γ, which relates velocity to mass and distance. The discussion suggests that escape velocity varies with mass, and a simplified equation can be derived by letting R equal the Schwarzschild radius plus a small distance, d. The derived formula indicates that escape velocity approaches (1 - d/2R_s)c, where R_s is the Schwarzschild radius. The conversation emphasizes the use of Planck units for simplification, asserting G and c equal to 1. This analysis provides a theoretical framework for understanding escape velocity near black holes without considering rotating scenarios.