  The current status of neutrino physics is reviewed with some near future
perspective. After recollecting the birth of modern neutrino physics with
nonzero masses and flavor mixing, I summarize the present status of measurement
of the mixing parameters in 2-3, 1-2, and 1-3 sectors of the MNS matrix. Then,
I describe the attempts to uncover the regularities, if any, in the measured
values of the mixing angles; mostly reviewing. Yet, a possible large deviation
of \theta_{23} to the second octant may trigger interests in the triangle
relation of the lepton mixing angles. In the latter part of my lecture some
perspective of determination of the mass hierarchy and measurement of lepton
Kobayashi-Maskawa phase $\delta$ are described. Finally, I discuss the
prospects of the new, fast developing field of high-energy neutrino
astrophysics, and the emerging new precision era of cosmology and particle
physics. I conclude with optimistic speculations.
