GIACOMINI, LIVIALIVIAGIACOMINIMassironi, M.M.MassironiThomas, N.N.ThomasPAJOLA, MAURIZIOMAURIZIOPAJOLACREMONESE, GabrieleGabrieleCREMONESELa Forgia, F.F.La ForgiaFerri, F.F.FerriLazzarin, M.M.LazzarinBarbieri, C.C.BarbieriBettini, I.I.BettiniMagrin, S.S.MagrinMarzari, F.F.MarzariNaletto, G.G.NalettoSierks, H.H.SierksRosetta OSIRIS Team2020-06-172020-06-1720160037-8720http://hdl.handle.net/20.500.12386/26115OSIRIS, the Scientific Imaging System for Rosetta mission \citep{keller07} has been acquiring images of the nucleus of the comet 67P/Churyumov-Gerasimenko since Aug 2014 with a resolution that allows a detailed analysis of its surface. Indeed, data reveal a complex surface morphology that is likely the expression of different processes affecting the cometary nucleus \citep{thomas15}. In order to characterize these different morphologies and better understand their distribution we performed a geomorphological mapping of the illuminated surface of 67P. For this purpose we used NAC images acquired on August 5-8 with a spatial resolution ranging from 1.5 and 2.4 m/pixel.ELETTRONICOenArticlehttp://sait.oat.ts.astro.it/MSAIt870116/index.html2016MmSAI..87..159GFIS/05 - ASTRONOMIA E ASTROFISICA