The discussion explores the potential density of Earth's atmosphere, considering its current state and the possibility of increased thickness without changing Earth's mass or solar position. It references Venus as a comparison, noting that Earth could hold a significantly thicker atmosphere due to its gravity and insolation. The conversation highlights that there is enough CO2 in Earth's crust to support a 45 bar atmosphere, although this is less than Venus. Additionally, if oceans were to boil, a theoretical atmosphere of about 300 bar could exist, but this scenario is deemed unlikely under current conditions. The topic emphasizes the complexities of atmospheric retention and the potential for a denser atmosphere based on geological factors.