Intergalactic stars, often referred to as "rogue" stars, do exist and are typically ejected from galaxies due to gravitational interactions, such as collisions or close encounters with supermassive black holes. While there is substantial evidence for the existence of these stars, the discussion around intergalactic planets remains more contentious, with some suggesting that if rogue stars exist, then rogue planets likely do as well. Statistical evidence indicates that a small percentage of stellar mass in clusters like Virgo may be composed of intergalactic stars, supporting the possibility of planets orbiting them. However, the mechanisms for planets being ejected from galaxies are debated, particularly regarding the tidal forces that could disrupt their integrity during such events. Overall, while intergalactic stars are recognized, the existence of intergalactic planets is still under scrutiny and requires further evidence.