P32B-02:
Comet 67P/Churyumov-Gerasimenko - First Science Results by Rosetta/OSIRIS

Wednesday, 17 December 2014: 10:40 AM
Holger Sierks1, Cesare Barbieri2, Philippe L Lamy3, Rafael Rodrigo4, Detlef Koschny5, Hans Rickman6, Jessica Agarwal7, Michael F A'Hearn8, Francesco Angrilli9, M. Antonietta Barucci10, Jean-Loup Bertaux11, Ivano Bertini2, Sebastien Besse12, Dennis Bodewits13, Claire Capanna14, Gabriele Cremonese9, Vania Da Deppo15, Björn Davidsson16, Stefano Debei17, Mariolino De Cecco17, Francesca Ferri18, Sonia Fornasier10, Marco Fulle19, Robert W Gaskell20, Olivier Groussin14, Carsten Güttler1, Carsten Güttler1, Pedro Gutiérrez21, Stubbe Faurschou Hviid22, Wing-Huen Ip23, Laurent Jorda24, Horst Uwe Keller25, Knollenberg Joerg26, Rainer Kramm26, Ekkehard Kuhrt27, Michael Küppers12, Fiorangela La Forgia9, Luisa Lara28, Monica Lazzarin9, Cedric Leyrat29, Jose F Moreno30, Steven Lowry31, Sara Magrin2, Simone Marchi32, Francesco Marzari33, Harald Michalik25, Stefano Mottola22, Giampiero Naletto17,33, Nilda Oklay34 and Maurizio Pajola2, (1)Max-Planck Institute for Solar System Research, Goettingen, Germany, (2)CISAS - Center for Studies and Activities for Space, University of Padova, Padova, Italy, (3)Astrophysics Laboratory of Marseilles, Marseilles, France, (4)IAA-CSIC, Granada, Spain, (5)European Space Research and Technology Centre, Noordwijk, Netherlands, (6)PAS Space Research Center, Warsaw, Poland, (7)Max-Planck Institute for Solar System Research, Germany, Goettigen, Germany, (8)University of Maryland, College Park, MD, United States, (9)University of Padova, Department of Physics and Astronomy, Padova, Italy, (10)LESIA Observatoire de Paris, Meudon, France, (11)University of Versailles Saint-Quentin en Yvelines, Versailles, France, (12)European Space Agency, Villanueva De La Can, Spain, (13)University of Maryland College Park, Astronomy, College Park, MD, United States, (14)Aix Marseille University, Marseille Cedex 03, France, (15)CNR-IFN UOS Padova LUXOR, Padova, Italy, (16)Uppsala University, Uppsala, Sweden, (17)University of Padova, Padova, Italy, (18)Univ. Padova, Padova, Italy, (19)Osservatorio Astronomico de Trieste, Trieste, Italy, (20)Planetary Science Institute Tucson, Tucson, AZ, United States, (21)Instituto de Astrofisica de Andalucia, Granada, Spain, (22)German Aerospace Center DLR Berlin, Berlin, Germany, (23)NCU National Central University of Taiwan, Jhongli, Taiwan, (24)Observatoire Astrophysique Marseille, Marseille, France, (25)Technical University of Braunschweig, Braunschweig, Germany, (26)Institut für Planetenforschung, Berlin, Germany, (27)DLR, Berlin, Germany, (28)Instituto de Astrophisica de Andalucia-CSIC, Spain, Dept. of Solar System, Andalucia, Spain, (29)Paris Observatory Meudon, Meudon, France, (30)University of Valencia, Burjassot, Spain, (31)University of Kent, UK, Center for Astrophysics and Planetary Science, Kent, United Kingdom, (32)NASA Lunar Science Institute, Boulder, CO, United States, (33)University of Padua, Padua, Italy, (34)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
Abstract:
Abstract

ESA’s Rosetta mission arrived on August 6, 2014, at target comet 67P/Churyumov-Gerasimenko after 10 years of cruise. OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) is the scientific imaging system onboard Rosetta. It comprises a Narrow Angle Camera (NAC) for nucleus surface and dust studies and a Wide Angle Camera (WAC) for the wide field coma investigations.

We present the first science results achieved by OSIRIS from the arrival at the comet throughout the mapping phase. The overview will cover surface morphology and activity of the nucleus as seen in gas, dust, and local jets.

Acknowledgements

OSIRIS was built by a consortium led by the Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany, in collaboration with CISAS, University of Padova, Italy, the Laboratoire d'Astrophysique de Marseille, France, the Instituto de Astrofísica de Andalucia, CSIC, Granada, Spain, the Scientific Support Office of the European Space Agency, Noordwijk, The Netherlands, the Instituto Nacional de Técnica Aeroespacial, Madrid, Spain, the Universidad Politéchnica de Madrid, Spain, the Department of Physics and Astronomy of Uppsala University, Sweden, and the Institut für Datentechnik und Kommunikationsnetze der Technischen Universität Braunschweig, Germany.

The support of the national funding agencies of Germany (DLR), France (CNES), Italy (ASI), Spain (MEC), Sweden (SNSB), and the ESA Technical Directorate is gratefully acknowledged.

We thank the Rosetta Science Ground Segment at ESAC, the Rosetta Mission Operations Centre at ESOC and the Rosetta Project at ESTEC for their outstanding work enabling the science return of the Rosetta Mission.