In a rotating celestial system, the distribution of objects of different masses may not align with traditional expectations, as evidenced by the solar system's configuration. High-mass planets are located farther from the center, while lower-mass asteroids are concentrated in the asteroid belt. The discussion highlights that gravitational acceleration affects all objects similarly, complicating mass-based distribution predictions. Dark matter's lack of electromagnetic interaction prevents it from separating from normal matter in the same way collisional species would, leading to distinct distribution patterns. Ultimately, gravitational interactions may influence the separation of matter and dark matter, though the dynamics differ from collisional scenarios.