This paper presents a novel resolution to the gravity freefall paradox, where General Relativity (GR) appears to introduce prematurespatial contraction effects that contradict Newtonian expectations. The paradox arises from the fact that GR predicts the same exter-nal gravitational field for both a physical mass and a black hole, yet point mass freefall marker behavior differs in both cases. We introduce the sine-alpha function, a dynamic formulation that naturally regulates spatial curvature according to the evolving ratio of marker separations. This model predicts Newtonian behavior outside the event horizon while dynamically allowing self-regulated curvature inside it. Our model preserves logical consistency between classical and relativistic physics. We provide evidence from numerical simulation, comparing our function’s predictions to GR, demonstrating its stability within and beyond the event horizon. We restrict ourselves to theoretical considerations only.