The translation of the relativistic motion into the language of forces
, proposed by the author (1995, Nuovo Cimento B 110 973), is employed
to interpret the gyroscope precession in general relativity. The prece
ssion is referred to the comoving Frenet triad built up along the proj
ection of the gyroscope's trajectory onto the 3-space of the local hyp
ersurface-orthogonal observer. The contributions of the centrifugal, t
he gravitational and the dragging + Coriolis forces are identified res
pectively with the Thomas, the geodetic, and the gravitomagnetic compo
nents of precession. Explicit expressions are given for several simple
types of motion in the Kerr (or simpler) field in order to show that
the general formulae obtained are not only very simple, but also yield
clear results in accord with intuition in concrete situations.