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COMET 67P/CHURYUMOV-GERASIMENKO: CLOSE-UP ON DUST PARTICLE FRAGMENTS

M. Hilchenbach J. Kissel Y. Langevin 1 Christelle Briois 2 H. von Hoerner A. Koch R. Schulz J. Sile'N K. Altwegg L. Colangeli H. Cottin C. Engrand 3 H. Fischer A. Glasmachers E. Grün G. Haerendel H. Henkel H. Höfner K. Hornung E.K. Jessberger H. Lehto K. Lehto F. Raulin Léna Le Roy J. Rynö W. Steiger T. Stephan Laurent Thirkell 2 R. Thomas 2 K. Torkar K. Varmuza K.-P. Wanczek N. Altobelli D. Baklouti 1 Anais Bardyn 2 N. Fray H. Krüger N. Ligier 1 Z. Lin Philippe Martin 2 S. Merouane F.R. Orthous-Daunay John Paquette Claire Revillet 2 S. Siljeström O. Stenzel B. Zaprudin
1 IAS - Institut d'astrophysique spatiale
2 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
3 CSNSM AS - Centre de Sciences Nucléaires et de Sciences de la Matière
Abstract : The COmetary Secondary Ion Mass Analyser instrument on board ESA's Rosetta mission has collected dust particles in the coma of comet 67P/Churyumov-Gerasimenko. During the early-orbit phase of the Rosetta mission, particles and particle agglomerates have been imaged and analyzed in the inner coma at distances between 100 km and 10 km off the cometary nucleus and at more than 3 AU from the Sun. We identified 585 particles of more than 14 μm in size. The particles are collected at low impact speeds and constitute a sample of the dust particles in the inner coma impacting and fragmenting on the targets. The sizes of the particles range from 14 μm up to sub-millimeter sizes and the differential dust flux size distribution is fitted with a power law exponent of -3.1. After impact, the larger particles tend to stick together, spread out or consist of single or a group of clumps, and the flocculent morphology of the fragmented particles is revealed. The elemental composition of the dust particles is heterogeneous and the particles could contain typical silicates like olivine and pyroxenes, as well as iron sulfides. The sodium to iron elemental ratio is enriched with regard to abundances in CI carbonaceous chondrites by a factor from ˜1.5 to ˜15. No clear evidence for organic matter has been identified. The composition and morphology of the collected dust particles appear to be similar to that of interplanetary dust particles.
Keywords : fragmented particles flocculent morphology cometary nuclei cosmic dust interplanetary matter meteorites minerals particle size planetary composition COmetary Secondary Ion Mass Analyser instrument data ESA Rosetta mission comet 67P/Churyumov-Gerasimenko coma early-orbit phase particle agglomerates cometary nucleus Sun low impact speeds particle sizes submillimeter sizes differential dust flux size distribution power law exponent dust particle elemental composition silicates olivine pyroxenes iron sulfides sodium-to-iron elemental ratio CI carbonaceous chondrites organic matter interplanetary dust particle morphology dust particle fragments
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M. Hilchenbach, J. Kissel, Y. Langevin, Christelle Briois, H. von Hoerner, et al.. COMET 67P/CHURYUMOV-GERASIMENKO: CLOSE-UP ON DUST PARTICLE FRAGMENTS. Astrophysical Journal Letters, IOP Science, 2016, 816 (2), pp.L32. ⟨10.3847/2041-8205/816/2/L32⟩. ⟨in2p3-01291758⟩

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