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In this paper, we investigate the properties of the Lense-Thirring precessionfrequency and periastron precession of the relativistic bound orbits in slowlyrotating naked singularity spacetimes. We show that the precession frequenciesof a stationary test gyroscope are quite unique in slowly rotating nakedsingularity spacetimes, and therefore, one can easily distinguish them from theslowly rotating Kerr black hole spacetime. On the other hand, we also show thatin slowly rotating Joshi-Malafarina-Narayan (JMN1) naked singularity spacetime,negative precession of the timelike bound orbits is allowed which is notpossible in Kerr and slowly rotating null naked singularity spacetimes.

Lense-Thirring effect and precession of timelike geodesics in slowly rotating black hole and naked singularity spacetimes