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- W45807432 abstract "The complexity of carbonaceous molecules and their abundance and timescale of formation in our evolving universe are crucial questions within cosmic chemistry. Interestingly, the organic chemistry in space seems to follow common pathways throughout space and time. Carbonaceous molecules in the gas or solid state, refractory or icy, are observed in similar abundances and composition in our and distant galaxies. Observations of galaxies at high red-shift, probes into the early universe, show carbonaceous molecules and dust formation. The largest fraction of carbon in the universe is incorporated into aromatic molecules such as gaseous polycyclic aromatic hydrocarbons as well as solid aromatic structures. Molecular clouds are the birthplace of stars, planets and small bodies. Therefore, a lineage between carbon reservoirs in the interstellar medium and in the solar system is expected. We attempt to compile the current knowledge on the connection between interstellar and solar system material, based on observations of interstellar dust and gas, cometary volatiles, simulation experiments, and the analysis of extraterrestrial matter. Those combined results are used to investigate the most abundant and stable carbonaceous material that was delivered to young planets and probably used to build life." @default.
- W45807432 created "2016-06-24" @default.
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- W45807432 date "2008-02-15" @default.
- W45807432 modified "2023-09-27" @default.
- W45807432 title "Cosmic Carbon Chemistry" @default.
- W45807432 doi "https://doi.org/10.1021/bk-2008-0981.ch012" @default.
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