Journal articles
A radar package for asteroid subsurface investigations: Implications of implementing and integration into the MASCOT nanoscale landing platform from science requirements to baseline design
Alain Hérique
1
Dirk Plettemeier
2
Caroline Lange
3
Jan Thimo Grundmann
3
Valérie Ciarletti
4
Tra-Mi Ho
3
Wlodek Kofman
1, 5
Benoit Agnus
6
Jun Du
5
Wenzhe Fa
5
Oriane Gassot
1
Ricardo Granados-Alfaro
1
Jerzy Grygorczuk
7
Ronny Hahnel
2
Christophe Hoarau
8
Martin Laabs
2
Christophe Le Gac
6
Marco Mütze
2, 6
Sylvain Rochat
1
Yves Rogez
1
Marta Tokarz
9
Petr Schaffer
2
André-Jean Vieau
6
Jens Biele
10
Christopher Buck
11
Jesus Gil Fernandez
11
Christian Krause
10
Raquel Rodriguez Suquet
12
Stephan Ulamec
13
Alain Hérique 1
Author IdHAL : alain-herique ORCID : https://orcid.org/0000-0003-3699-883X
Dirk Plettemeier 2
Author
Caroline Lange 3
Author
Jan Thimo Grundmann 3
Author
Valérie Ciarletti 4
Author IdHAL : valerie-ciarletti ORCID : https://orcid.org/0000-0001-9483-0539
Tra-Mi Ho 3
Author
Wlodek Kofman 1, 5
Author IdHAL : wlodek-kofman ResearcherId : http://www.researcherid.com/rid/C-4556-2008 ORCID : https://orcid.org/0000-0002-6744-8796
Benoit Agnus 6
Author
Christopher Buck 11
Author
Jesus Gil Fernandez 11
Author
Christian Krause 10
Author
Raquel Rodriguez Suquet 12
Author
Stephan Ulamec 13
Author IdHAL : stephan-ulamec
1
IPAG - Institut de Planétologie et d'Astrophysique de Grenoble (414, Rue de la Piscine BP 53 38041 Grenoble Cedex 9 - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNES - Centre National d'Études Spatiales [Toulouse] (18 avenue Edouard Belin 31401 Toulouse - France)
- CNRS - Centre National de la Recherche Scientifique (France)
- OSUG - Observatoire des Sciences de l'Univers de Grenoble (414 Rue de la piscine - BP 53 38041 GRENOBLE CEDEX 9 - France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- IRSTEA - Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (France)
- USMB [Université de Savoie] [Université de Chambéry] - Université Savoie Mont Blanc (27, rue Marcoz - 73000 Chambéry - France)
- CNRS - Centre National de la Recherche Scientifique : UMS832 (France)
- UGA [2016-2019] - Université Grenoble Alpes [2016-2019] (CS 40700 - 38058 Grenoble cedex - France)
2
TU Dresden - Technische Universität Dresden = Dresden University of Technology (TU Dresden 01062 Dresden - Germany)
3
DLR Institute of Space Systems (Robert Hooke Straße 7, 28359 Bremen - Germany)
- DLR - German Aerospace Center (Germany)
4
PLANETO - LATMOS (France)
- LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- SU - Sorbonne Université : UMR8190 (21 rue de l’École de médecine - 75006 Paris - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
5
CBK - Space Research Centre of Polish Academy of Sciences (Bartycka 18A, 00-716 Warsaw, Poland - Poland)
6
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- SU - Sorbonne Université : UMR8190 (21 rue de l’École de médecine - 75006 Paris - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
7
IRSGIS - Institute of Remote Sensing and Geographic Information System (School of Earth and Space Sciences, Peking University, Beijing - China)
- School of Earth and Space Sciences [Beijing] (Peking University, Haidian District, Beijing - China)
- Peking University [Beijing] (No.5 Yiheyuan Road Haidian District, Beijing, P.R.China 100871 - China)
8
ElecLab - Electronique (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- NEEL - Institut Néel (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
- CNRS - Centre National de la Recherche Scientifique : UPR2940 (France)
- UGA [2016-2019] - Université Grenoble Alpes [2016-2019] (CS 40700 - 38058 Grenoble cedex - France)
9
ASTRONIKA Sp. Zo.o. (00-716 Warszawa - Poland)
10
DLR - German Aerospace Center (Germany)
11
ESTEC - European Space Research and Technology Centre (Keplerlaan 1, 2201 Noordwijk - Netherlands)
- ESA - European Space Agency (France)
12
CNES - Centre National d'Études Spatiales [Toulouse] (18 avenue Edouard Belin 31401 Toulouse - France)
13
DLR - Deutsches Zentrum für Luft- und Raumfahrt (Germany)
Abstract : The internal structure of asteroids is still poorly known and has never been analyzed directly by measurements. Our knowledge relies entirely on inferences from remote sensing observations of the surface and theoretical modeling. Direct measurements are crucial to characterize an asteroid's internal structure and heterogeneity from sub-metric to global scale. The radar package developed in the frame of the phase A/B1 of the Asteroid Impact Mission (AIM) as part of the larger Asteroid Impact & Deflection Assessment (AIDA) mission is a mature instrument suite to answer this question and to improve our ability to understand and model the mechanisms driving Near Earth Asteroids (NEA). It is of main interest for science, exploration and planetary defense. This instrument suite consists of a monostatic high frequency radar (HFR) to investigate the stratigraphy of surface regolith and a bistatic low frequency radar (LFR) to characterize the deep interior. The chosen platform to deliver the surface unit of the LFR and other instruments for a close-up study of the target asteroid is the MASCOT nanolander, which already flies on Hayabusa2 (HY2) in a mineralogy scout configuration. In this paper, we present the chosen instrumentation for radar science, baseline mission requirements and the initial design for integration into the lander platform, including all peculiarities and constraints.
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Journal articles
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https://hal-insu.archives-ouvertes.fr/insu-01757087
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Submitted on : Friday, April 6, 2018 - 4:35:25 PM
Last modification on : Wednesday, April 14, 2021 - 3:39:12 AM
Contributor : Catherine Cardon <>
Submitted on : Friday, April 6, 2018 - 4:35:25 PM
Last modification on : Wednesday, April 14, 2021 - 3:39:12 AM
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- HAL Id : insu-01757087, version 1
- DOI : 10.1016/j.actaastro.2018.03.058
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Citation
Alain Hérique, Dirk Plettemeier, Caroline Lange, Jan Thimo Grundmann, Valérie Ciarletti, et al.. A radar package for asteroid subsurface investigations: Implications of implementing and integration into the MASCOT nanoscale landing platform from science requirements to baseline design. Acta Astronautica, Elsevier, 2019, 156, pp.317-329. ⟨10.1016/j.actaastro.2018.03.058⟩. ⟨insu-01757087⟩
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