Similarities in element  content between comet 67P/Churyumov–Gerasimenko coma dust and selected meteorite samples

Abstract We have analysed the element composition and the context of particles collected within the coma of 67P/Churyumov–Gerasimenko with Rosetta’s COmetary Secondary Ion Mass Analyzer (COSIMA). A comparison has been made between on board cometary samples and four meteorite samples measured in the...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2017, Vol.469 (Suppl_2), p.S492-S505
Hauptverfasser: Stenzel, Oliver J., Hilchenbach, Martin, Merouane, Sihane, Paquette, John, Varmuza, Kurt, Engrand, Cécile, Brandstätter, Franz, Koeberl, Christian, Ferrière, Ludovic, Filzmoser, Peter, Siljeström, Sandra
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Sprache:eng
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Zusammenfassung:Abstract We have analysed the element composition and the context of particles collected within the coma of 67P/Churyumov–Gerasimenko with Rosetta’s COmetary Secondary Ion Mass Analyzer (COSIMA). A comparison has been made between on board cometary samples and four meteorite samples measured in the laboratory with the COSIMA reference model. Focusing on the rock-forming elements, we have found similarities with chondrite meteorites for some ion count ratios. The composition of 67P/Churyumov–Gerasimenko particles measured by COSIMA shows an enrichment in volatile elements compared to that of the investigated Renazzo (CR2) carbonaceous meteorite sample.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stx1908