The general relationship between mass and distance from the Sun is that larger celestial bodies, such as planets and moons, tend to be found at varying distances from the Sun, with their masses influencing their gravitational interactions and orbits. For example, the gas giants, which are more massive, are located farther from the Sun compared to the smaller, rocky inner planets. However, mass does not directly determine distance; rather, it is the gravitational dynamics and formation history of the solar system that dictate the positions of these bodies. Thus, while there is some correlation, it is not a strict rule.
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