Mean distance between sun or star and earth or planet evaluator uses Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5 to evaluate the Mean Distance between Sun and Planet, Mean distance between sun or star and earth or planet formula is defined as the average distance between the center of the sun or star and the center of the earth or planet, which is a critical parameter in understanding the radiation and energy exchange between the two celestial bodies. Mean Distance between Sun and Planet is denoted by L symbol.
How to evaluate Mean distance between sun or star and earth or planet using this online evaluator? To use this online evaluator for Mean distance between sun or star and earth or planet, enter Radius of the Sun (r), Effective Surface Temperature (Ts) & Total Solar Irradiance (Gs) and hit the calculate button.