Dark matter influences the orbital velocities of stars in galaxies but has a negligible effect on the solar system due to its low density within that scale. While dark matter interacts gravitationally, it does not clump together like regular matter, making direct impacts with black holes rare. Most dark matter exists in a halo around galaxies, spending more time in outer regions rather than near supermassive black holes. When dark matter approaches a black hole, it typically swings around rather than falling in, similar to comets orbiting the Sun. The dynamics of dark matter and its collisionless nature explain why it behaves differently than regular matter in the vicinity of black holes.