This paper discusses the results of an experiment on board the Mir space st
ation, using the Pegas UV camera. Spectrozonal photography of the surface o
f the hull of the Progress cargo space ship, illuminated by the sun at a ce
rtain zenith angle at a wavelength of 0.28 mum and a spectral width of 0.02
5 mum, made it possible to measure the spectral radiance densities of indiv
idual elements (sections) of the hull surface, to determine their statistic
al weights, and to compute the spectral radiance density (averaged over the
part of the hull surface turned toward the observer) and the mean spectral
geometrical albedo. (C) 2001 The Optical Society of America.