G Filacchione, M C De Sanctis, F Capaccioni, A Raponi, F Tosi, M Ciarniello, P Cerroni, G Piccioni, M T Capria, E Palomba, G Bellucci, S Erard, D Bockelee-Morvan, C Leyrat, G Arnold, M A Barucci, M Fulchignoni, B Schmitt, E Quirico, R Jaumann, K Stephan, A Longobardo, V Mennella, A Migliorini, E Ammannito, J Benkhoff, J P Bibring, A Blanco, M I Blecka, R Carlson, U Carsenty, L Colangeli, M Combes, M Combi, J Crovisier, P Drossart, T Encrenaz, C Federico, U Fink, S Fonti, W H Ip, P Irwin, E Kuehrt, Y Langevin, G Magni, T McCord, L Moroz, S Mottola, V Orofino, U Schade, F Taylor, D Tiphene, G P Tozzi, P Beck, N Biver, L Bonal, J-Ph Combe, D Despan, E Flamini, M Formisano, S Fornasier, A Frigeri, D Grassi, M S Gudipati, D Kappel, F Mancarella, K Markus, F Merlin, R Orosei, G Rinaldi, M Cartacci, A Cicchetti, S Giuppi, Y Hello, F Henry, S Jacquinod, J M Reess, R Noschese, R Politi, G Peter
Although water vapour is the main species observed in the coma of comet 67P/Churyumov-Gerasimenko and water is the major constituent of cometary nuclei, limited evidence for exposed water-ice regions on the surface of the nucleus has been found so far. The absence of large regions of exposed water ice seems a common finding on the surfaces of many of the comets observed so far. The nucleus of 67P/Churyumov-Gerasimenko appears to be fairly uniformly coated with dark, dehydrated, refractory and organic-rich material...
January 21, 2016: Nature