  I discuss how the ideas associated with Seesaws, first introduced in the
context of neutrino masses, are generally useful for understanding the very
disparate scales one encounters in particle physics. From this point of view,
the energy scale characterizing the Universe's dark energy presents a real
challenge. A natural Seesaw explanation for this scale ensues if one imagines
tying the dark energy sector to the neutrino sector, but this idea requires
bold new dynamics.
