Distribution of water around the nucleus of comet 67P/Churyumov-Gerasimenko at 3.4 AU from the Sun as seen by the MIRO instrument on Rosetta

N. Biver (1) , M. Hofstadter (2) , S. Gulkis (2) , D. Bockelée-Morvan (1) , M. Choukroun (3) , E. Lellouch (1) , F. Schloerb , L. Rezac (4) , W. Ip (5) , C. Jarchow (4) , P. Hartogh (4) , S. Yip Lee (6) , P. von Allmen , J. Crovisier (1) , C. Leyrat (7, 1) , P. Encrenaz (8)

1 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
2 JPL - Jet Propulsion Laboratory
3 LPG - Laboratoire de Planétologie et Géodynamique [UMR 6112]
4 MPS - Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research
5 Institute of Space Science [Taiwan]
6 Northern Research Station
7 HCTLab - Human Computer Technology Laboratory
8 LERMA - Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique

Domaines: Physique [physics]; Astrophysique [astro-ph]; Planète et Univers [physics]

N. Biver, M. Hofstadter, S. Gulkis, D. Bockelée-Morvan, M. Choukroun, et al.. Distribution of water around the nucleus of comet 67P/Churyumov-Gerasimenko at 3.4 AU from the Sun as seen by the MIRO instrument on Rosetta. Astronomy and Astrophysics - A&A, 2015, 583, pp.A3. ⟨10.1051/0004-6361/201526094⟩. ⟨hal-02484170⟩