Neutrinos represent a new "window" to the Universe, spanning a large range
of energy. We discuss the science of neutrino astrophysics and focus on two
energy regimes. At "lower" energies (approximate to 1 MeV). studies of neu
trinos born inside the sun, or produced in interactions of cosmic rays with
the atmosphere, have allowed the first incontrovertible evidence that neut
rinos have mass. At energies typically one thousand to one million times hi
gher, sources further than the sun (both within the Milky Way and beyond) a
re expected to produce a flux of particles that can be detected only throug
h neutrinos.