When a star collapses into a black hole, its gravitational force appears to increase due to the significant reduction in its radius, allowing objects to get much closer to its center. This phenomenon is explained by the curvature of space-time in general relativity, rather than just Newtonian gravity, which considers mass alone. While the gravitational force does not increase at a fixed distance, the distortion of space-time around the black hole becomes more pronounced. If a star could collapse quietly into a black hole, the orbits of its surrounding planets would remain unchanged, as they would be outside the event horizon. However, objects that venture too close may experience gravitational radiation, which could lead to their spiraling into the black hole.