The heat shield of the Mars Science Laboratory was equipped with thermocouple stacks to measure in-depth heating of the thermal protection system during atmospheric entry. The heat load derived from the thermocouples in the stagnation region was found to be 33% lower than corresponding postflight predictions of convective heating alone. It was hypothesized that this difference could be attributed to radiation from the shock-heated gas, a mechanism not considered in preflight analyses of flowfields. To test the hypothesis and quantify the contribution of shock-layer radiation to total surface heating, ground tests and simulations (both flow and radiation) were performed at several points along the best-estimated entry trajectory of the Mars Science Laboratory. The present paper provides an assessment of the quality of the radiation model and its impact to stagnation point heating. The impact of radiative heating is shown to account for 43% of the heat load discrepancy. Additional possible factors behind the remaining discrepancy are discussed. Nomenclature B λ T = Planck (blackbody) function at temperature, T, W∕cm 2 · sr · μm D = shock-tube diameter, m d = shock standoff distance, m e λ x = emission coefficient at position x, W∕cm 2 · sr · μm L λ x = spectral radiance at position x, W∕cm 2 · sr · μm L λ x; θ = spectral radiance at position x at off-normal angle θ, W∕cm 2 · sr · μm _ m = mass blowing rate, kg∕m 2 · s q = heat flux or irradiance Tx = temperature at position x, K v = velocity, m∕s x = position along stagnation line or perpendicular to heat shield, cm or m y = position along heat shield surface, m δ = boundary-layer thickness, m θ = off-normal angle, rad λ = wavelength, nm p c = ablation product density, kg∕m 3