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Authors
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Wada, Koji
Grott, Matthias
Michel, Patrick
Walsh, Kevin J.
Barucci, Antonella M.
Biele, Jens
Blum, Jürgen
Ernst, Carolyn M.
Grundmann, Jan Thimo
Gundlach, Bastian
Hagermann, Axel
Hamm, Maximilian
Jutzi, Martin
Kim, Myung-Jin
Kührt, Ekkehard
Le Corre, Lucille
Libourel, Guy
Lichtenheldt, Roy
Maturilli, Alessandro
Messenger, Scott R.
Michikami, Tatsuhiro
Miyamoto, Hideaki
Mottola, Stefano
Müller, Thomas
Nakamura, Akiko M.
Nittler, Larry R.
Ogawa, Kazunori
Okada, Tatsuaki
Palomba, Ernesto
Sakatani, Naoya
Schröder, Stefan E.
Senshu, Hiroki
Takir, Driss
Zolensky, Michael E.
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Funding
Funding for this research was provided by:
Japan Society for the Promotion of Science (15K05273)
CNES
NASA Emerging Worlds and Hayabusa2 Participating Scientist Programs
SERVII Center for Lunar Science and Exploration
European Union's Horizon 2020 Research and Innovation Programme (687378)
National Aeronautics and Space Administration (Contract NNM10AA11C issued through the New Frontiers Program)
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Article History
Received: 25 June 2018
Accepted: 29 October 2018
First Online: 11 December 2018
Authors’ information
: KW is a PI of the International Regolith Science Group (IRSG) which is a branch of the Interdisciplinary Science Team in the Hayabusa2 project. KW, MG, PM, KJW, and HM are core members of IRSG.
: The authors declare that they have no competing interests.
: Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
