  The purpose of this paper is to explore a resolution for the Faint Young Sun
Paradox that has been mostly rejected by the community, namely the possibility
of a somewhat more massive young Sun with a large mass loss rate sustained for
two to three billion years. This would make the young Sun bright enough to keep
both the terrestrial and Martian oceans from freezing, and thus resolve the
paradox. It is found that a large and sustained mass loss is consistent with
the well observed spin-down rate of Sun-like stars, and indeed may be required
for it. It is concluded that a more massive young Sun must be considered a
plausible hypothesis.
