A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Similarities in element content between comet 67P/Churyumov–Gerasimenko coma dust and selected meteorite samples
Tekijät: Oliver J. Stenzel, Martin Hilchenbach, Sihane Merouane, John Paquette, Kurt Varmuza, Cécile Engrand, Franz Brandstätter, Christian Koeberl, Ludovic Ferrière, Peter Filzmoser, Sandra Siljeström; the COSIMA team
Julkaisuvuosi: 2017
Journal: Monthly Notices of the Royal Astronomical Society
Vuosikerta: 469
Numero: Supplement: 2
Aloitussivu: S492
Lopetussivu: S505
Sivujen määrä: 14
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/stx1908
Verkko-osoite: https://academic.oup.com/mnras/article/469/Suppl_2/S492/4060708
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/38998460
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.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
