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Physical Characterization of Asteroids Candidates of Marco Polo Mission

Authors :
Birlan, Mirel
Binzel, Richard P.
Nedelcu, Dan Alin
Vernazza, Pierre
Barucci, Maria Antonella
Gasc, S.
Fulchignoni, Marcello
Dotto, Elisabetta
Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)
Department of Earth Atmospheric and Planetary Sciences, MIT
AIRA, Romania
ESTEC / ESA, Netherlands
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Pôle Planétologie du LESIA
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Université Paris Cité (UPCité)
INAF/OAR, Italy
Source :
Bulletin of the American Astronomical Society, AAS/Division for Planetary Sciences Meeting #41, AAS/Division for Planetary Sciences Meeting #41, Oct 2009, Fajardo, Puerto Rico, Puerto Rico
Publication Year :
2009
Publisher :
HAL CCSD, 2009.

Abstract

International audience; The principal scientific objective of the Marco Polo mission is to return unaltered NEO materials. Marco Polo will allow us to analyze the samples in terrestrial laboratories, thereby obtaining measurements that cannot yet beperformed from a robotic spacecraft. The selection of the target asteroids for the mission has important consequences in terms of mission design, constraints, and operational requirements. A list of asteroids as possible targets for the Marco Polo mission has been drawn, taken into account both dynamical and physical constraints. The key parameters of this list were the accessibility of the object (the delta-V amount for the encounter with the target) and the desirable, primitive composition requirements of the target deduced from the groundbased data (mainly from colors and spectroscopy).

Details

Language :
English
Database :
OpenAIRE
Journal :
Bulletin of the American Astronomical Society, AAS/Division for Planetary Sciences Meeting #41, AAS/Division for Planetary Sciences Meeting #41, Oct 2009, Fajardo, Puerto Rico, Puerto Rico
Accession number :
edsair.dedup.wf.001..e9eac9a488fe1f9410477bb2305c9ac3