  The geodesics of bound spherical orbits i.e. of orbits performing
Lense-Thirring precession, are obtained in the case of the $\Lambda$-term
within gravito-electromagnetic formalism. It is shown that the presence of the
$\Lambda$-term in the equations of gravity leads to both relativistic and
non-relativistic corrections in the equations of motion. The contribution of
the $\Lambda$-term in the Lense-Thirring precession is interpreted as an
additional relativistic correction and the gravito-gyromagnetic ratio is
defined.
