“…Saryshev and Mirer (2001) found a new analytical solution of all equilibria for the case where the internal angular momentum of the gyrostat satellite is collinear to its principal axis of inertia. Following the 2001 study, Sarychev et al (2005) determined the bifurcation values and showed the evolution of the regions of validity, for the same particular case, while Sarychev et al (2008) studied the special case where the gyrostatic moment vector lies in one of the satellite's principal central planes of inertia. Molina and Monde ´jar (2004) focused on the motion of a satellite that had, in the first case, spherical symmetry, and in the second case, axial symmetry.…”