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SARIM PLUS--sample return of comet 67P/CG and of interstellar matter
Srama R., Krüger H., Yamaguchi T., Stephan T., Burchell M. et al
Experimental Astronomy 33 (2012) 723-751 - http://hal.in2p3.fr/in2p3-00673501
Physique/Astrophysique/Planétologie et astrophysique de la terre
Planète et Univers/Astrophysique/Planétologie et astrophysique de la terre
SARIM PLUS--sample return of comet 67P/CG and of interstellar matter
R. Srama ()1, 2, H. Krüger3, T. Yamaguchi, T. Stephan, M. Burchell, A. T. Kearsley, V. Sterken1, 4, F. Postberg1, S. Kempf4, 5, E. Grün2, 5, N. Altobelli, P. Ehrenfreund, V. Dikarev, M. Horanyi5, Z. Sternovsky5, J. D. Carpenter, A. Westphal, Z. Gainsforth, A. Krabbe1, J. Agarwal, H. Yano, J. Blum4, H. Henkel, J. Hillier, P. Hoppe, M. Trieloff, S. Hsu5, A. Mocker1, 2, K. Fiege2, 4, S. F. Green, A. Bischoff, F. Esposito, R. Laufer, T. W. Hyde, G. Herdrich1, S. Fasoulas1, A. Jäckel, G. Jones, P. Jenniskens, E. Khalisi2, G. Moragas-Klostermeyer1, 2, F. Spahn, H. U. Keller4, P. Frisch, Anny Chantal Levasseur-Regourd6, 7, 8, N. Pailer, K. Altwegg, C. Engrand9, S. Auer, J. Silen, S. Sasaki, M. Kobayashi, Julien Schmidt, J. Kissel, B. Marty10, P. Michel11, P. Palumbo, O. Vaisberg, J. Baggaley, A. Rotundi, H. P. Röser1
1 :  IRS - Institut für Raumfahrtsysteme
Universität Stuttgart
Allemagne
2 :  Max Planck Institute for Nuclear Physics
Max-Planck-Institut
Allemagne
3 :  Max-Planck-Institut für Sonnensystemforschung
Max-Planck-Institut für sonnensystemforschung
Allemagne
4 :  Technische Universität Braunschweig
http://www.tu-braunschweig.de/
Technische Universität Braunschweig
TU Braunschweig 38092 Braunschweig Allemagne
Allemagne
5 :  LASP - Laboratory for Atmospheric and Space Physics
http://lasp.colorado.edu/home/
University of Colorado at Boulder
1234 Innovation Drive, Boulder, CO 80303-7814
États-Unis
6 :  UPMC - Université Pierre et Marie Curie - Paris 6
http://www.upmc.fr/
Université Pierre et Marie Curie (UPMC) - Paris VI
4 place Jussieu - 75005 Paris
France
7 :  LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
http://www.latmos.ipsl.fr
CNRS : UMR8190 – Université Pierre et Marie Curie (UPMC) - Paris VI – Université de Versailles Saint-Quentin-en-Yvelines (UVSQ) – INSU
France
8 :  IPSL - Institut Pierre-Simon-Laplace
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 (UVSQ) – École normale supérieure [ENS] - Paris
4 Place Jussieu 75252 PARIS CEDEX 05
France
9 :  CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse
http://www-csnsm.in2p3.fr/
CNRS : UMR8609 – IN2P3 – Université Paris XI - Paris Sud
batiments 104 et 108 - 91405 Orsay Campus
France
10 :  CRPG - Centre de recherches petrographiques et géochimiques
http://www.crpg.cnrs-nancy.fr
CNRS : UPR2300 – INSU
15 Rue Notre Dame des Pauvres - BP 20 54501 VANDOEUVRE LES NANCY CEDEX
France
11 :  OCA - Observatoire de la Cote d'Azur
http://www.oca.eu/
CNRS : UMS2202
B.P. 4229 06304 Nice Cedex 4
France
impec
CSNSM AS
The Stardust mission returned cometary, interplanetary and (probably) interstellar dust in 2006 to Earth that have been analysed in Earth laboratories worldwide. Results of this mission have changed our view and knowledge on the early solar nebula. The Rosetta mission is on its way to land on comet 67P/Churyumov-Gerasimenko and will investigate for the first time in great detail the comet nucleus and its environment starting in 2014. Additional astronomy and planetary space missions will further contribute to our understanding of dust generation, evolution and destruction in interstellar and interplanetary space and provide constraints on solar system formation and processes that led to the origin of life on Earth. One of these missions, SARIM-PLUS, will provide a unique perspective by measuring interplanetary and interstellar dust with high accuracy and sensitivity in our inner solar system between 1 and 2 AU. SARIM-PLUS employs latest in-situ techniques for a full characterisation of individual micrometeoroids (flux, mass, charge, trajectory, composition) and collects and returns these samples to Earth for a detailed analysis. The opportunity to visit again the target comet of the Rosetta mission 67P/Churyumov-Gerasimeenternko, and to investigate its dusty environment six years after Rosetta with complementary methods is unique and strongly enhances and supports the scientific exploration of this target and the entire Rosetta mission. Launch opportunities are in 2020 with a backup window starting early 2026. The comet encounter occurs in September 2021 and the reentry takes place in early 2024. An encounter speed of 6 km/s ensures comparable results to the Stardust mission.

Articles dans des revues avec comité de lecture
02/2012
Experimental Astronomy
33
723-751
© Springer Science+Business Media B.V. 2012

CSNSM AS
Interstellar dust – Cometary dust – Churyumov Gerasimenko – Interplanetary dust – IMF – Cosmic vision – Sample return – Dust collector – Mass spectrometry