The hard-sphere potential has been the most intensively studied interaction model in many areas of statistical mechanics for at least two reasons. The first reason is that hard-spheres exhibit many phenomena observed in real systems, such as the existence of liquid, solid, and metastable phases, and indeed provide a good first approximation for real systems of such properties as liquid structure, transport properties, and both liquid- and solid-phase thermodynamic properties. The second reason is that the hard-sphere interaction is the only one for which a tractable kinetic equation applicable at moderate densities, the Enskog equation [1‐ 3], exists. The Enskog equation was originally proposed on physical grounds as a finite-density generalization of the Boltzmann equation which, although applicable to arbitrary two-body interaction models, is restricted to low densities. The generalization of the Enskog equation by van Beijeren and Ernst [4] is capable of giving a unified description of liquid, solid, and metastable states [5]. However, because of the complexity of the Enskog equation, the only analytic solutions available are perturbative and recently developed numerical techniques [6] have yet to be widely applied so that little is known about its description of systems far from equilibrium. The standard method of analyzing either the Boltzmann or the Enskog equation is the Chapman-Enskog expansion [2,3] which is a perturbative expansion of the one-body distribution function, and the kinetic equation describing it, in terms of the uniformity of the system. For example, in a fluid undergoing uniform shear flow (USF), in which the local macroscopic flow velocity along the x axis varies linearly with position along the y axis, $ us$ rd › ay ˆ x, this amounts to an expansion in powers of the shear rate, a. This expansion has only been performed in the general case to third order in the uniformity parameter and the range of validity of such results is presumably limited to near-equilibrium states; the analytic complexity of the Chapman-Enskog procedure has proven prohibitive of the study of higher-order effects. An alternative method of analysis of the Boltzmann equation is the moment method of Grad [2,7,8] according to which the distribution is expressed as an expansion in terms of velocity about local equilibrium. Keeping all terms in the expansion gives an infinite set of coupled equations for the generally spaceand time-dependent coefficients which, assuming the validity of the expansion, is equivalent to the Boltzmann equation. Approximations are then introduced to truncate or decouple the equations allowing for an approximate solution. The method has found particular use in the study of small-wavelength hydrodynamics near equilibrium [9] where the close connection between the moment method and kinetic models has been exploited. The purpose of this Letter is to show that the method may be used to obtain good approximate solutions to the Enskog equation for systems far from equilibrium. In the following, attention is focused on USF since sheared fluids may be reliably simulated and the connection between theory and simulation is well understood. Indeed, for these reasons, USF has been the subject of numerous investigations over the last 20 years (see, e.g., Ref. [10]), and is often viewed as a prototypical nonequilibrium state free from complicating features such as boundary effects. In addition, it has been known for some time that the hard-sphere system is unstable at high shear rates [11] and theories of the instability depend on knowledge of the one-body distribution [12,13]. Since only perturbative results, which lack important physical effects such as shear thinning, have been available, these theories remain tentative. One of the motivations for the present work has been to allow for a more detailed study of this problem. Both the Boltzmann and Enskog equations may be written in the form