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Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta

MPS-Authors
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Paquette,  John
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Stenzel,  Oliver Joachim
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Fischer,  Henning
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Merouane,  Sihane
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Kissel,  Jochen
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Hilchenbach,  Martin
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Bardyn, A., Baklouti, D., Cottin, H., Fray, N., Briois, C., Paquette, J., et al. (2017). Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta. Monthly Notices of the Royal Astronomical Society, 469(Suppl. 2), S712-S722. doi:10.1093/mnras/stx2640.


Cite as: http://hdl.handle.net/21.11116/0000-0001-1B86-A
Abstract
Cometary ices are rich in CO2, CO and organic volatile compounds, but the carbon content of cometary dust was only measured for the Oort Cloud comet 1P/Halley, during its flyby in 1986. The COmetary Secondary Ion Mass Analyzer (COSIMA)/Rosetta mass spectrometer analysed dust particles with sizes ranging from 50 to 1000 μm, collected over 2 yr, from 67P/Churyumov-Gerasimenko (67P), a Jupiter family comet. Here, we report 67P dust composition focusing on the elements C and O. It has a high carbon content (atomic $${\rm{C}}/{\rm{Si}} = 5.5{\rm{\ }}_{ - 1.2}^{ + 1.4}\ \ {\rm{on\ average}}$ $) close to the solar value and comparable to the 1P/Halley data. From COSIMA measurements, we conclude that 67P particles are made of nearly 50 per cent organic matter in mass, mixed with mineral phases that are mostly anhydrous. The whole composition, rich in carbon and non-hydrated minerals, points to a primitive matter that likely preserved its initial characteristics since the comet accretion in the outer regions of the protoplanetary disc.