Marco Polo - A Mission to Return a Sample from a Near-Earth Object - Science Requirements and Operational Scenarios
- Creators
- Koschny, Detlef
- Barucci, Maria Antonella
- Yoshikawa, Makoto
- Böhnhardt, Hermann
- Brucato, John
- Coradini, Marcello
- Dotto, Elisabetta
- Franchi, I.
- F. Green, Simon
- Josset, Jean-Luc
- Kawaguchi, Junichiro
- Michel, Patrick
- Muinonen, Karri
- Oberst, Jürgen
- Yano, Hajime
- Binzel, Richard P.
- Agnolon, David
- Romstedt, Jens
- Others:
- ESA-ESTEC
- Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA) ; 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 Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
- JSPEC/ JAXA
- Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau (MPS)
- INAF-Osservatorio Astrofisico di Arcetri (INAF-OAA)
- European Space Agency (ESA)
- INAF-Osservatorio Astronomico di Roma (INAF-OAR)
- Open University
- SPACE-X, Space Exploration Institute
- Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)
- Jakokoski Observatory, University of Helsinki
- Institute for Planetary Sciences, DLR
- Massachusetts Institute of Technology, Cambridge
Description
Marco Polo is a mission to return a sample from a near-Earth object of primitive type (class C or D). It is foreseen as a collaborative effort between the Japan Aerospace Exploration Agency (JAXA) and the European Space Agency (ESA). Marco Polo is currently in a Phase-A study (status as of summer 2009). This paper focuses on the scientific requirements provided to the industrial study consortia in Europe as well as the possible mission scenario at the target object in order to achieve the overall mission science objectives. The main scientific reasons for going to a near-Earth object are to understand the initial conditions and evolution history of the solar nebula, to understand how major events (e.g. agglomeration, heating) influence the history of planetesimals, whether primitive class objects contain presolar material, what the organics were in primitive materials, how organics could shed light on the origin of molecules necessary for life, and what the role of impacts by NEOs would be in the origin and evolution of life on Earth.
Abstract
International audience
Additional details
- URL
- https://hal.archives-ouvertes.fr/hal-03732338
- URN
- urn:oai:HAL:hal-03732338v1
- Origin repository
- UNICA