The exploration of terrestrial planets in the Solar System was and still is performed mainly on data that cover almost all the electromagnetic spectrum, acquired over the last century by several types of orbiters, rovers, and landers. Planetary data volumes are constantly increasing both in quality and quantity, with the contribution of both public and private entities.Imagery has always been the primary resource for researchers in planetary sciences, especially for geologists and geomorphologists. In the last two decades, the progress in the development of very high-resolution image sensors gave the community access to images with a spatial resolution on the order of centimeters. Data collected by High Resolution Imaging Science Experiment (HiRISE) instrument, on board of the Mars Reconnaissance Orbiter (MRO) (McEwen et al., 2007) or by the Narrow Angle Camera experiment, on board of Lunar Reconnaissance Orbiter (Robinson et al., 2010), have been used in several works to constrain the surface properties of respectively, Mars and the Moon.