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In situ mass spectrometry during the Lutetia flyby
Altwegg K., Balsiger H., Calmonte U., Hässig M., Hofer L., Jäckel A., Schläppi B., Wurz P., Berthelier J.-J., De Keyser J. et al
Planetary and Space Science 66, 1 (2012) 173-178 - http://hal.archives-ouvertes.fr/hal-00623340
Article in peer-reviewed journal
Sciences of the Universe/Astrophysics/Instrumentation and Methods for Astrophysic
Physics/Astrophysics/Instrumentation and Methods for Astrophysic
Sciences of the Universe/Astrophysics/Earth and Planetary Astrophysics
Physics/Astrophysics/Earth and Planetary Astrophysics
In situ mass spectrometry during the Lutetia flyby
K. Altwegg 1, H. Balsiger 1, U. Calmonte 1, M. Hässig 1, L. Hofer 1, A. Jäckel 1, B. Schläppi 1, P. Wurz 1, Jean-Jacques Berthelier 2, 3, 4, J. De Keyser 5, B. Fiethe 6, S. Fuselier 7, U. Mall 8, H. Rème 9, 10, M. Rubin 11
1:  Physikalisches Institut, Universität Bern
http://www.phinst.unibe.ch/content/index_ger.html
Universität Bern
Sidlerstrasse 5 CH-3012 Bern
Switzerland
2:  Institut Pierre-Simon-Laplace (IPSL)
http://www.ipsl.jussieu.fr/
CNRS : FR636 – Institut de recherche pour le développement [IRD] – CEA – CNES – INSU – Université Pierre et Marie Curie [UPMC] - Paris VI – Université de Versailles Saint-Quentin-en-Yvelines – Ecole normale supérieure de Paris - ENS Paris
4 Place Jussieu 75252 PARIS CEDEX 05
France
3:  Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
http://www.latmos.ipsl.fr
CNRS : UMR8190 – Université Pierre et Marie Curie [UPMC] - Paris VI – Université de Versailles Saint-Quentin-en-Yvelines – INSU
France
4:  Université Pierre et Marie Curie - Paris 6 (UPMC)
http://www.upmc.fr/
Université Pierre et Marie Curie [UPMC] - Paris VI
4 place Jussieu - 75005 Paris
France
5:  Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB)
http://www.aeronomie.be/en/
Belgian Institute for Space Aeronomy
Institute for Space Aeronomy Ringlaan-3-Avenue Circulaire B-1180 Brussels
Belgium
6:  Institute of Computer and Network Engineering (IDA)
Technische Universität Braunschweig
Braunschweig
Germany
7:  Lockheed Martin Advanced Technology Center, Space Physics Dept
Advanced Technology Center
Palo Alto
United States
8:  Max-Planck-Institut für Sonnensystemforschung
Max-Planck-Institut für sonnensystemforschung
Germany
9:  Centre d'étude spatiale des rayonnements (CESR)
http://www.cesr.fr
CNRS : UMR5187 – Observatoire Midi-Pyrénées – INSU – Université Paul Sabatier [UPS] - Toulouse III
9 Av du colonel Roche - BP 4346 31028 TOULOUSE CEDEX 4
France
10:  Institut de recherche en astrophysique et planétologie (IRAP)
CNRS : UMR5277 – Université Paul Sabatier [UPS] - Toulouse III – Observatoire Midi-Pyrénées
France
11:  University of Michigan
http://www.umich.edu/
University of Michigan
500 Church Street Ann Arbor, MI 48109-1090
United States
heppi
During the Rosetta flyby at asteroid Lutetia the ROSINA instrument tried to detect a thin exosphere of the asteroid. Although the instrument is sensitive enough to detect even very tenuous gases at a density level of 1 cm−3 the Lutetia exosphere could not be unambiguously detected due to spacecraft outgassing, which was not constant because of the changing solar aspect angle. An upper limit for a water exosphere density at the flyby distance of 3160 km of (3.5±1.0)*103 cm−3 was deduced from the measurements.
English

Planetary and Space Science
Publisher Elsevier
ISSN 0032-0633 
international
2012
66
1
173-178

Rosetta – ROSINA – Lutetia – in situ mass spectrometry – Spacecraft outgassing – Exosphere