  A strongly naked singularity (SNS) was modelled at the center of the Galaxy.
This specific type of naked singularity was characterized in 2008 by Virbhadra
and Keeton. The lens is described using the Janis-Newman-Winicour metric, which
has an ordinary mass and massless scalar charge parameters. Gravitational
lensing by the SNS gives rise to 4 images: 2 images on the same side as the
source and 2 images on the opposite side of the source from the optic axis. We
compute magnification centroid, magnification centroid shift, and total
absolute magnification for many values of the angular source position. The
nature of the curve for all three results are qualitatively similar to
Schwarzschild black hole lenses, but quantitatively different. Magnification
centroid increases as angular source position increases. As angular source
position increases, magnification centroid shift increases to a maximum value,
and then begins to decrease. As angular source position becomes large,
magnification centroid shift will approach zero. Total magnification is large
for small values of angular source position, and decreases to a limiting value
of one. The results expand upon previous work on an SNS of {\nu}=0.01. If such
observations were viewed experimentally, they would show support for an SNS at
the galactic center. Interpretation of an SNS would disprove the cosmic
censorship hypothesis by Penrose, as well as the weaker cosmic censorship
hypothesis by Virbhadra, which allows the existence of weakly naked
singularities.
