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Planetary and Space Science 66, 1 (2012) 173-178
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
(2012)

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.
1:  Physikalisches Institut, Universität Bern
Universität Bern
2:  Institut Pierre-Simon-Laplace (IPSL)
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
3:  Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
CNRS : UMR8190 – Université Pierre et Marie Curie [UPMC] - Paris VI – Université de Versailles Saint-Quentin-en-Yvelines – INSU
4:  Université Pierre et Marie Curie - Paris 6 (UPMC)
Université Pierre et Marie Curie [UPMC] - Paris VI
5:  Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB)
Belgian Institute for Space Aeronomy
6:  Institute of Computer and Network Engineering (IDA)
Technische Universität Braunschweig
7:  Lockheed Martin Advanced Technology Center, Space Physics Dept
Advanced Technology Center
8:  Max-Planck-Institut für Sonnensystemforschung
Max-Planck-Institut für sonnensystemforschung
9:  Centre d'étude spatiale des rayonnements (CESR)
CNRS : UMR5187 – Observatoire Midi-Pyrénées – INSU – Université Paul Sabatier [UPS] - Toulouse III
10:  Institut de recherche en astrophysique et planétologie (IRAP)
CNRS : UMR5277 – Université Paul Sabatier [UPS] - Toulouse III – Observatoire Midi-Pyrénées
11:  University of Michigan
University of Michigan
heppi
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
Rosetta – ROSINA – Lutetia – in situ mass spectrometry – Spacecraft outgassing – Exosphere