  In this article, we investigate the gravitational field of a charged,
non-vacuum, non-rotating, spherically symmetric body of mass $M$ assuming a
static solution to the Einstein-Maxwell field equations. We demonstrate that
the characteristics of perihelion precession of orbits in Schwarzschild and
Null singularity spacetimes are similar, whereas, in the case of charged naked
singularity (CNS) spacetime, the characteristics are the opposite of those in
Schwarzschild and Null singularity spacetime. Here we discuss some novel
features of the timelike and lightlike geodesics in this spacetime. We also
discuss the comparative study of tidal force in the null singularity spacetime
and charged naked singularity spacetime.
