There is no fixed limit to the number of planets that can orbit a star like the Sun, as the definition of a planet is not universally agreed upon. The current understanding suggests that our solar system is "dynamically full," meaning additional planets would struggle to maintain stable orbits within it, primarily outside Neptune. The formation of new planets beyond Neptune ceased due to insufficient material and slow orbital velocities in that region. In binary star systems, the presence of a partner star can restrict stable zones for planets, while close encounters in star clusters can strip outer planets away. Ultimately, the classification of celestial bodies as planets is arbitrary and varies based on definitions, with the IAU's recent decisions highlighting the complexity of this categorization.