Numerical results obtained with direct simulation Monte Carlo and Navier-Stokes methods are presented for a Mach-20 nitrogen flow about a 70-deg blunted cone. The flow conditions simulated are those that can be obtained in existing low-density hypersonic wind tunnels. Three sets of flow conditions are considered with freestream Knudsen numbers ranging from 0.03 to 0.001. The focus is on the wake structure: how the wake structure changes as a function of rarefaction, what the afterbody levels of heating are, and to what limits the continuum models are realistic as rarefaction in the wake is progressively increased. Calculations are made with and without an afterbody sting. Results for the afterbody sting are emphasized in anticipation of an experimental study for the current flow conditions and model configuration. The Navier-Stokes calculations were made with and without slip boundary conditions. Comparisons of the results obtained with the two simulation methodologies are made for both flowfield structure and surface quantities. Nomenclature A = base area of cone, ird 2 /4 C D = drag coefficient, ID/p^V^A C H = heat transfer coefficient, 2q/p 00 Vl> D = drag d = base diameter Kn = Knudsen number, \/d M -Mach number M = molecular weight of N 2 , 28.02 g/mole R = gas constant for N 2 , 296.7 J/kg-K R b = cone base radius R c = corner radius Re = Reynolds number, pVd/p Re 2 = total Reynolds number, Re^ (MOO/MO) R n -nose radius S = speed ratio, V\/M/2RT s = distance along the body surface measured from the stagnation point s = temperature exponent of the coefficient of viscosity T = thermodynamic temperature 7} = internal kinetic temperature r ov = overall kinetic temperature T w = surface temperature u = axial velocity V = velocity v = radial velocity