Dust of comet 67P/Churyumov-Gerasimenko collected by Rosetta/MIDAS: classification and extension to the nanometer scale

Context. The properties of the smallest subunits of cometary dust contain information on their origin and clues to the formation of planetesimals and planets. Compared to interplanetary dust particles or particles collected during the Stardust mission, dust collected in the coma of comet 67P/Churyum...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2019-10, Vol.630, p.A26
Hauptverfasser:	Mannel, T., Bentley, M. S., Boakes, P. D., Jeszenszky, H., Ehrenfreund, P., Engrand, C., Koeberl, C., Levasseur-Regourd, A. C., Romstedt, J., Schmied, R., Torkar, K., Weber, I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Agglomeration Aggregates Astrophysics Atomic force microscopes Atomic force microscopy Comet heads Comets comets: individual: 67P/Churyumov-Gerasimenko Dust Fractal geometry Interplanetary dust Micrometers Morphology Normal distribution Packing density Particle size distribution Planet formation planets and satellites: formation Properties (attributes) protoplanetary disks Rosetta mission Sciences of the Universe space vehicles space vehicles: instruments Spatial resolution Stardust Mission Structural analysis techniques: miscellaneous Voyager 1 spacecraft
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