General relativity (GR) accounts for orbital precession, such as that observed in Mercury, due to its fundamentally different treatment of gravity compared to Newtonian mechanics. In GR, gravity is not simply an inverse square force; it involves additional velocity-dependent interactions, often referred to as "gravitomagnetic" effects. This complexity leads to orbits that deviate from perfect ellipses, as the curvature of spacetime affects the motion of orbiting bodies. The precession is influenced by factors like angular velocity and proximity to massive objects, which alter the gravitational field experienced by the orbiting body. Ultimately, the combination of these factors results in the observed precession that cannot be explained by Newtonian physics alone.