The paper addresses attitude stabilization of the rotational axis of an asymmetric carrying body by pendulum dampers. Steady motions in which the kinetic energy of the system takes stationary values are identified. Whether these motions are stable is established Keywords: stabilization, rotational axis, asymmetric carrying body, pendulum dampers, kinetic energy Introduction. Attitude stabilization of the rotational axis of a carrying perfectly rigid body (PRB) is an important problem of mechanics. Such bodies can be artificial satellites or spacecraft with spin stabilization [1][2][3][4][5][6][7][8][9][10][11][12][13][14]. Spin stabilization is disadvantageous in that, for example, inaccurate initial rotation imparted to a symmetric satellite causes its rotational axis to long precess about a fixed axis (axis of precession). To suppress the nutation, various dampers are applied. It was shown in [1, 3, 6, 7, 12] that pendulums and viscous dampers effectively decrease rather large initial nutation angles of the PRB rotation axis. However, the reasons for the residual nutation of this axis have not yet been established. The fundamental possibility to completely damp nutation with pendulum dampers was pointed out in [13,14]. This possibility has not been examined so far. In this connection, the present paper looks into the attitude stabilization of the rotational axis of a PRB with pendulum dampers. Namely, steady motions of the system will be identified, it will be established whether these motions are stable, and the possibility of complete dampening of nutation with dampers will be examined.Closely related issues are considered in [15][16][17][18]. We will consider a damper consisting of two pairs of pendulums set onto an axis rigidly fixed to the PRB. The theory of passive automatic balancers [9] suggests that such a device can completely counterbalance a nonsymmetric PRB and, thereby, completely damp nutation.1. Model Description. Consider a PRB of mass Ì. The mass and inertia characteristics of the PRB and the whole system will be described using the principal axes of inertia OXYZ, with the origin O at the centroid of the PRB (Fig. 1a). The axial moments of inertia about the X-, Y-, and Z-axes are denoted by A, B, and C, respectively. In the general case, we have À Â Ñ ¹ ¹ .