When verifying a sophisticated numerical code, it is usual practice to
compare the results with reliable solutions obtained by other means.
This work provides such solutions for the wavelength-dependent dust ra
diative transfer problem. We define a set of benchmark problems in sph
erical geometry and solve them by three radiative transfer codes which
implement different numerical schemes. Results for the dust temperatu
re and emerging spectra agree to better than 0.1 per cent, and can be
used as benchmark solutions for the verification of the dust radiative
transfer codes.