The discussion centers on the radiation pressure exerted by a black hole, specifically one with a mass equivalent to the Sun. It is established that the radiation pressure from such a black hole, due to its extremely low temperature and Hawking radiation, is negligible—approximately 10^44 times weaker than that from the Sun. Participants explore the theoretical balance between radiation pressure and gravitational force, noting that this balance occurs at very small black hole masses, but such scenarios are fleeting and not practically significant. The conversation also touches on the limitations of current physics in measuring phenomena at the Planck scale, suggesting that while theoretical limits exist, empirical evidence is lacking. Overall, the implications of black hole radiation pressure remain largely theoretical and not applicable in practical scenarios.