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The Visible InfraRed (VIR) mapping spectrometer onboard Dawn mission hasobtained the spatial distribution of the spectral reflectance of Vesta in thewavelength ranges between 0.25-1.07 micrometers and 0.95-5.1 micrometers. Aphotometric correction allows to characterize the intrinsic variability of thesurface albedo by removing the dependance of the reflectance from the observinggeometry. In this work, we present the photometric correction obtained forobservations from the Survey, HAMO and HAMO 2 mission phases at Vesta in thewhole spectral range investigated by VIR, as well as the surface albedo maps.

Spectrophotometric correction of Vesta observations performed by the VIR Imaging spectrometer onboard Dawn mission