Within the approximation of dominant charging collisions the explicit microscopic calculations of the FokkerPlanck kinetic coefficients for highly-charged grains moving in plasma are performed. It is shown that due to ion absorption by grain the collecting friction coefficient can be negative and the appropriate threshold value of the grain charge is found. The stationary solutions of the Fokker-Planck equation with the velocity dependent kinetic coefficient are obtained and the considerable deviation of such solutions from the Maxwellian distribution is established.In the systems close to equilibrium Brownian particles keep stationary random motion under the action of stochastic forces which are compensated by the particle friction and thus, the work produced by the Langevin sources is equal to the energy dissipated in course of the Brownian particle motion. This [5,6]. The possibility of negative friction (negative values of friction coefficient) of the Brownian particles was regarded, as a result of energy pumping. For some phenomenological dependences of the friction coefficient as a function of the grain's velocity the one-particle stationary non-Maxwellian distribution function was found.The traditional formulations of the non-equilibrium Brownian motion are based on some phenomenological expressions for the friction and diffusion coefficients. In particular, it means that deviations from the Einstein relation, as well as the velocity dependence of these coefficients are postulated and high level of uncertainty for the application of such models to the real systems takes place. Here we will consider another situation, when the kinetic coefficients can be calculated exactly on the basis of the microscopically derived Fokker-Planck equation for dusty plasmas [7,8]. It will be shown that in the case of strong interaction parameter Γ ≡ e 2 Z g Z i /aT i 1 (here Z g , Z i are the charge numbers for the grains and ions respectively, a is the grain radius, T i is the ion temperature) the negative collecting friction coefficient appears for some velocity domain. The physical reason for manifestation of negative friction is clear: the cross-section for ion absorption by grain increases with the relative velocity between the ion and grain decrease due to the charge-dependent part of the cross-section. Therefore, for a moving highly-charged grain (Γ 1) the momentum transfer from ions to the grain in the direction of grain velocity is higher than in the opposite direction.We start from the Fokker-Planck equation for the spherical grains in dusty plasma with typical narrow charge distribution around a negative value q = e e Z g , that permits to put all grain charges to be equal. We also ignore