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Naked singularities form during the gravitational collapse of inhomogeneousmatter clouds. The final nature of the singularity depends on the initialconditions of the matter properties and types of matter profiles. These nakedsingularities can also be divided into two types: null-like and timelikesingularities. The spacelike singularity of the Schwarzschild black hole can bedistinguished from the null and timelike naked singularity spacetimes. In lightof this, we investigate the precession of timelike bound orbits in the nullnaked singularity spacetime, as well as tidal force effects and geodesicdeviation features. As a result, we find that the orbital precession of thetimelike bound orbits in null naked singularity spacetime could bedistinguished from the Schwarzschild precession case. The radial component ofthe tidal force has an intriguing profile, whereas the angular component has aprofile which is comparable to that of a Schwarzschild black hole scenario. Thegeodesic deviation equation is then solved numerically, yielding results thatresemble a Schwarzschild black hole. These characteristic features can then beused to discern amongst these singularities.

Tidal force effects and periodic orbits in null naked singularity spacetime