Constant acceleration in rotating objects results from a combination of centrifugal force and gravity, with constant thrust required for sustained acceleration. The density of celestial bodies near the sun is not coincidental; as the solar nebula collapsed, heavier elements were drawn toward the center due to gravitational forces. This process led to the formation of denser planets closer to the sun, particularly within the frost line. However, some exoplanetary systems challenge this theory, showcasing gas giants in unexpected orbits, suggesting they may have migrated from their original positions beyond the snow line. Overall, the dynamics of gravity and rotation play crucial roles in the structure of solar systems.