  The faint young Sun paradox remains an open question. Presented here is one
possible solution to this apparent inconsistency, a more massive early Sun.
Based on conditions on early Earth and Mars, a luminosity constraint is set as
a function of mass. We examine helioseismic constraints of these alternative
mass-losing models. Additionally, we explore a dynamic electron screening
correction in an effort to improve helioseismic agreement in the core of the an
early mass-losing model.
