We investigated the broadening of spectral lines in a high-pressure zinc discharge. The contributions of resonance, van der Waals and Stark broadening are calculated and compared with broadening constants derived from side-on measurements. The energy balance is solved for a lamp containing about 1 bar metallic zinc and 2.25 bar Ar as a starting rare gas. The axis temperature of the discharge derived from the contours of the spectral lines is 5400 K as compared to model calculations yielding 5370 K. It is shown, that the contribution of radiation diffusion to the thermal conductivity is dominating at plasma temperatures above 5000 K, i.e. at temperatures, where the discharge is assumed to be in local thermal equilibrium. In a similar way as for mercury discharges, broadening of the resonance line at λ = 213.8 nm (Hg: λ = 253.6 nm) is dominant with respect to radiation diffusion, but also transitions to the triplet S4P3P and to the singlet S4P1P must be taken into account. The energy balance is solved using the measured line broadening data, resulting in a good agreement of the temperature profile with that derived from side-on measurements.