  A new relative orbit solution with new dynamical masses is determined for the
nearby white dwarf - red dwarf pair 40 Eri BC. The period is 230.09+/-0.68y. It
is predicted to close slowly over the next half-century getting as close as
1.32" in early 2066. We determine masses of 0.575+/-0.018 $m_\odot$ for the
white dwarf and 0.2041+/-0.0064 $m_\odot$ for the red dwarf companion. The
inconsistency of the masses determined by gravitational redshift and dynamical
techniques, due to a premature orbit calculation, no longer exists.
