Reference : Herschel PACS and SPIRE Observations of comet 103P/Hartley 2
Scientific congresses and symposiums : Paper published in a journal
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/107052
Herschel PACS and SPIRE Observations of comet 103P/Hartley 2
English
Bockelee-Morvan, D. [Observatoire de Paris, LESIA, Meudon, France (dominique.bockelee@obspm.fr)]
Swinyard, B. [Rutherford Appleton Laboratory, Oxfordshire, UK]
Vandenbussche, B. [Institute for Astronomy, KU, Leuven, Belgium]
Hartogh, P. [Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany]
Jehin, Emmanuel mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image]
Hutsemekers, Damien mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)]
Manfroid, Jean mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)]
Biver, N. [Observatoire de Paris, LESIA, Meudon, France (dominique.bockelee@obspm.fr)]
de Val-Borro, M. [Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany]
Crovisier, J. [ > > ]
Küppers, M. [ > > ]
Lis, D. C. [ > > ]
Rengel, M. [ > > ]
Szutowicz, S. [ > > ]
2011
EPSC Abstracts 2011
231, pp. 1-2
No
International
EPSC-DPS Joint Meeting
October 2011
[en] The ESA Herschel Space Observatory [8] used its full complement of state-of-the-art instruments to observe the far-infrared and submillimetre spectrum and to image the thermal dust radiation of the Jupiter family comet 103P/Hartley 2 in the 70-672 μm spectral range. The observations were carried out in the period 24 October to 17 November 2010, as part of the Herschel Guaranteed Time Key program "Water and related chemistry in the Solar System" (HssO) [6]. We present here observations of H2O lines and of the dust coma made with the Photodetector Array and Camera (PACS) [9] and the Spectral and Photometric Imaging Receiver (SPIRE) [5].
Researchers
http://hdl.handle.net/2268/107052
http://adsabs.harvard.edu/abs/2011epsc.conf..231B

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