I review the current status of the solar neutrino problem, including the exciting possibility of matter enhanced neutrino oscillations. Neutrino flux measurements, independent of questions of solar dynamics, appear to leave only one competing candidate astrophysical solution, at least in the case of steady-state solar models. That possibility — mixing of the solar core on time scales of 3He equilibration — appears to have some attractive features. A “score card” is presented in which the two alternatives — mixed neutrinos or a mixed sun — are handicapped.