The discussion clarifies that the mass of ionized hydrogen is considered to be 0.5 AMU because it averages the mass of protons and free electrons, with the electron mass being negligible compared to protons. This average is used in pressure calculations within stars, particularly in the context of the Sun's composition, which includes hydrogen and helium. The pressure formula P=((density)/(avg mass of a particle))*kT relies on this average mass, leading to a value of 0.61 AMU when accounting for heavier elements. Additionally, in certain stars, the electron gas may become degenerate, necessitating the use of Fermi gas pressure for accurate calculations. Understanding these factors is crucial for comprehending stellar pressure dynamics.