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MarcoPolo-R near earth asteroid sample return mission

Authors :
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Binzel, Richard P
Michel, P.
Böhnhardt, H.
Campo Bagatin, A.
Cerroni, P.
Dotto, E.
Fitzsimmons, A.
Lara, L.-M.
Licandro, J.
Marty, B.
Muinonen, K.
Nathues, A.
Oberst, J.
Robert, F.
Saladino, R.
Ulamec, S.
Zolensky, M.
Barucci, Maria Antonietta
Cheng, A. F.
Benner, L. A. M.
Bland, P. A.
Brucato, J. R.
Franchi, I. A.
Green, S. F.
Rivkin, A. S.
Trigo-Rodriguez, J. M.
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Binzel, Richard P
Michel, P.
Böhnhardt, H.
Campo Bagatin, A.
Cerroni, P.
Dotto, E.
Fitzsimmons, A.
Lara, L.-M.
Licandro, J.
Marty, B.
Muinonen, K.
Nathues, A.
Oberst, J.
Robert, F.
Saladino, R.
Ulamec, S.
Zolensky, M.
Barucci, Maria Antonietta
Cheng, A. F.
Benner, L. A. M.
Bland, P. A.
Brucato, J. R.
Franchi, I. A.
Green, S. F.
Rivkin, A. S.
Trigo-Rodriguez, J. M.
Source :
Springer Netherlands
Publication Year :
2017

Abstract

MarcoPolo-R is a sample return mission to a primitive Near-Earth Asteroid (NEA) proposed in collaboration with NASA. It will rendezvous with a primitive NEA, scientifically characterize it at multiple scales, and return a unique sample to Earth unaltered by the atmospheric entry process or terrestrial weathering. MarcoPolo-R will return bulk samples (up to 2 kg) from an organic-rich binary asteroid to Earth for laboratory analyses, allowing us to: explore the origin of planetary materials and initial stages of habitable planet formation; identify and characterize the organics and volatiles in a primitive asteroid; understand the unique geomorphology, dynamics and evolution of a binary NEA. This project is based on the previous Marco Polo mission study, which was selected for the Assessment Phase of the first round of Cosmic Vision. Its scientific rationale was highly ranked by ESA committees and it was not selected only because the estimated cost was higher than the allotted amount for an M class mission. The cost of MarcoPolo-R will be reduced to within the ESA medium mission budget by collaboration with APL (John Hopkins University) and JPL in the NASA program for coordination with ESA’s Cosmic Vision Call. The baseline target is a binary asteroid (175706) 1996 FG3, which offers a very efficient operational and technical mission profile. A binary target also provides enhanced science return. The choice of this target will allow new investigations to be performed more easily than at a single object, and also enables investigations of the fascinating geology and geophysics of asteroids that are impossible at a single object. Several launch windows have been identified in the time-span 2020–2024. A number of other possible primitive single targets of high scientific interest have been identified covering a wide range of possible launch dates. The baseline mission scenario of MarcoPolo-R to 1996 FG3 is as follows: a single primary spacecraft provided by ESA, carrying

Details

Database :
OAIster
Journal :
Springer Netherlands
Notes :
application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1018412748
Document Type :
Electronic Resource