  In this paper, we propose novel methods to increase total luminosity and
decrease error propagation during subluminal or luminal interstellar transits
by navigation with star maps. We demonstrate with theoretical and simulation
models in first order approximation results that are correlated to eccentric
and concentric of light bands, ebbing and ascending of light streaks, and
centric of celestial distance. Finally our models show that both near-field and
far-field celestial objects enhance error correction and navigation vectors
even when the traveling speed is approaching the speed-of-light. We demonstrate
that our method of varying a spaceship's primary axis rotational rate and angle
of approach are superior than traveling at a straight line, especially when the
traveling speed is approaching or exceeding the speed of light.
