Aggregate dust particles at comet 67P/Churyumov–Gerasimenko

Mark S. Bentley (), Roland Schmied, Thurid Mannel, Klaus Torkar, Harald Jeszenszky, Jens Romstedt, Anny-Chantal Levasseur-Regourd, Iris Weber, Elmar K. Jessberger, Pascale Ehrenfreund, Christian Koeberl and Ove Havnes
Additional contact information
Mark S. Bentley: Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6
Roland Schmied: Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6
Thurid Mannel: Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6
Klaus Torkar: Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6
Harald Jeszenszky: Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6
Jens Romstedt: European Space Research and Technology Centre, Future Missions Office (SREF)
Anny-Chantal Levasseur-Regourd: UPMC (Sorbonne Université)LATMOS-IPSL, BC 102, 4 place Jussieu
Iris Weber: Institut für Planetologie, Universität Münster, Wilhelm-Klemm-Strasse 10
Elmar K. Jessberger: Institut für Planetologie, Universität Münster, Wilhelm-Klemm-Strasse 10
Pascale Ehrenfreund: Leiden Observatory, Postbus 9513
Christian Koeberl: University of Vienna, Althanstrasse 14
Ove Havnes: UiT The Arctic University of Norway

Nature, 2016, vol. 537, issue 7618, 73-75

Abstract: dust particles at comet 67P/Churyumov–Gerasimenko confirm that the particles are aggregates of smaller, elongated grains even at the smallest sizes examined.

Date: 2016
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DOI: 10.1038/nature19091

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