  An important aspect of General Relativity is to study properties of
geodesics. A useful tool for describing geodesic behavior is the geodesic
deviation equation. It allows to describe the tidal properties of gravitating
objects through the curvature of spacetime. This article focuses on the study
of the axially symmetric Taub-NUT metric. We study tidal effects in this metric
using the geodesic deviation equation. Radial geodesics along the symmetry axis
of spacetime are considered. We show that all spatial components of tidal
forces always change sign under the event horizon. We find a solution of the
geodesic deviation equation for all geodesic deviation vector components. It
allows us to quantify the effect of the NUT-charge on the tidal properties of
Taub-NUT metric. And another important feature that we found is the regular
behavior of all tidal force components at all points of spacetime.
