In a two-body system governed by Newton's Law of gravitation, there should theoretically be no orbital precession, as the orbits would consistently map out the same ellipse due to the system's dynamical symmetry. However, numerical simulations can introduce errors that may result in apparent precession over time, leading to misconceptions about the system's behavior. It's essential to monitor the total energy of the system in simulations to ensure stability and accuracy. Perturbations that deviate from a 1/r potential can indeed cause precession. The discussion highlights the importance of understanding the limitations of numerical simulations in accurately predicting orbital dynamics.