Similarities in element content between comet 67P/Churyumov–Gerasimenko coma dust and selected meteorite samples
Author(s) -
O. Stenzel,
M. Hilchenbach,
S. Merouane,
John Paquette,
Курт Вармуза,
C. Engrand,
F. Brandstätter,
Christian Koeberl,
L. Ferrière,
Peter Filzmoser,
Sandra Siljeström
Publication year - 2017
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stx1908
Subject(s) - meteorite , comet , physics , context (archaeology) , chondrite , astrobiology , coma (optics) , astrophysics , carbonaceous chondrite , geology , paleontology
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.
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