The discussion revolves around the relationship between temperature and mass in stars, questioning whether a hotter star is more massive than a cooler one due to increased atomic kinetic energy. Participants clarify that two identical stars, if one heats up without external influences, would not change in mass simply due to temperature differences, as mass is not directly affected by temperature in this context. The concept of black holes is also addressed, with clarification that they do not possess infinite mass but rather infinite density. The conversation highlights the importance of distinguishing between rest mass and total mass, emphasizing that energy contributes to total mass according to the equation E=mc². Ultimately, the thread underscores the complexity of stellar evolution and the nuances of mass-energy relationships in physics.