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- W2891345975 abstract "Abstract The overall goal of the ESA Rosetta mission was to help decipher the origin and evolution of our solar system. Looking at the chemical composition of comet 67P/Churyumov-Gerasimenko is one way of doing this. The amount of very volatile species found and the insight into their isotopic abundances show that at least some presolar ice has survived the formation of the solar system. It shows that the solar nebula was not homogenized in the region where comets formed. The D/H ratio in water furthermore indicates that Jupiter family comets and Oort cloud comets probably formed in the same regions and their difference is then purely due to their different dynamical history. The organics found in 67P are very diverse, with abundant CH- and CHO- bearing species. Sulphur bearing species like S 3 and S 4 and others show evidence of dust grain chemistry in molecular clouds." @default.
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- W2891345975 date "2017-03-01" @default.
- W2891345975 modified "2023-10-18" @default.
- W2891345975 title "Chemical highlights from the Rosetta mission" @default.
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- W2891345975 doi "https://doi.org/10.1017/s1743921317007852" @default.
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