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- W1617859292 abstract "Composition data show that production from different nucleosynthetic sites and a sequence of condensation processes characterize the history of matter found in the smaller objects of the solar system. We present estimates for molecular and elemental abundances in the material released by Halley’s comet. They are based on data of the gas and dust composition in the coma. Highly volatile material is very abundant, consistent with condensation and accretion at very low temperature. Isotopic data obtained with different methods in material of cometary origin support the view that comets are regular members of the solar system which, however, have preserved the original characteristics of the condensed and accreted matter better than other bodies in this system." @default.
- W1617859292 created "2016-06-24" @default.
- W1617859292 creator A5044173187 @default.
- W1617859292 date "1988-01-01" @default.
- W1617859292 modified "2023-10-03" @default.
- W1617859292 title "Composition in Halley’s Comet: Clues to Origin and History of Cometary Matter" @default.
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- W1617859292 doi "https://doi.org/10.1007/978-3-642-74188-3_1" @default.
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