The Geomorphology of Comet Churymov-Gerasimenko As Revealed By Rosetta/Osiris: Implicationsfor Past Collisional Evolution
Simone Marchi1, Michael F A'Hearn2, Cesare Barbieri3, M. Antonietta Barucci4, Sebastien Besse5, Gabriele Cremonese6, Wing-Huen Ip7, Horst Uwe Keller8, Detlef Koschny9, Ekkehard Kuhrt10, Philippe L Lamy11, Francesco Marzari3, Matteo Massironi12, Maurizio Pajola13, Hans Rickman14, Rafael Rodrigo15, Holger Sierks16, Colin Snodgrass17, Nicolas Thomas18 and Jean-Baptiste Vincent17, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)University of Maryland College Park, College Park, MD, United States, (3)University of Padua, Padua, Italy, (4)Observatoire Paris, Paris, France, (5)European Space Agency, Villanueva De La Can, Spain, (6)INAF - Astronomical Observatory of Padova, Padova, Italy, (7)NCU National Central University of Taiwan, Jhongli, Taiwan, (8)Institute for Geophysics and Extraterrestrial Physics, Braunschweig, Germany, (9)European Space Research and Technology Centre, Noordwijk, Netherlands, (10)German Aerospace Center DLR Berlin, Berlin, Germany, (11)Astrophysics Laboratory of Marseilles, Marseilles, France, (12)Univ Padova, Padova, Italy, (13)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (14)Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden, (15)IAA-CSIC, Granada, Spain, (16)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (17)Max-Planck Institute for Solar System Research, Goettingen, Germany, (18)University of Bern, Bern, Switzerland