Research indicates that planets can form in systems without stars, such as in dark systems or around massive bodies like brown dwarfs. While traditional planet formation typically involves a star, oversized gas giants could theoretically exist in such environments. Rogue planets, which are not gravitationally bound to any star, also exemplify this phenomenon. Sub-brown dwarfs represent a category of planetary-mass objects formed from gas cloud collapse, lacking the mass to initiate nuclear fusion. Overall, while less common, the formation of planets without stars is a plausible scenario in astrophysics.