The discussion centers on calculating the power per square meter received from a star at a distance of 1.5 x 10^11 m. Initially, there was confusion regarding the area to use, with some participants suggesting the total surface area of a sphere rather than the effective area of a disc facing the star. The correct approach involves dividing the total power output of the star by the area over which it spreads, leading to the conclusion that the power per unit area is based on the irradiance received by a square meter directly facing the star. Participants noted the ambiguity in the original question, which led to varied interpretations about whether to consider total power or average power across a planet's surface. Ultimately, clarity on the question's intent is crucial for accurate calculations.