Precession of timelike bound orbits in Kerr spacetime

Abstract Astrometric observations of S-stars provide a unique opportunity to probe the nature Sagittarius-A* (Sgr-A*). In view this, it has become important understand and behavior timelike bound trajectories particles around massive central object. It is known now that whereas Schwarzschild black hole does not allow negative precession for S-stars, naked singularity spacetimes can admit positive as well orbits. this context, we study perihelion test particle in Kerr spacetime geometry. Considering some approximations, investigate whether orbits have precession. paper, only consider low eccentric equatorial With these considerations, find spacetimes, allowed.