Planetary systems without a central star are considered unlikely to form, as traditional models of planetary formation rely on the gravitational collapse of gas clouds that create a star at the center. Stars, including low-mass ones like brown dwarfs, are essential for providing the gravitational force needed to hold planets in orbit. Without a star, there is insufficient mass to facilitate the accretion of material necessary for planet formation. The existence of isolated planetary bodies is acknowledged, but they do not constitute a true planetary system. Overall, the consensus is that starless planetary systems are improbable compared to those with stars.