1996
DOI: 10.1007/bf02459908
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Organic photohemistry in the atmosphere of jupiter and saturn

Abstract: The regioselectivity of all these reactions is detailed and reaction pathways are proposed.The relevance to the photolysis of the atmosphere of Jupiter and Saturn is discussed.

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“…That a fluid medium is necessary for harboring life is the most speculative of the proposed criteria, as the possibility that life could exist in dense atmospheres has also been suggested (Sagan and Salpeter, 1976). There is, for example, experimental and observational evidence for organic synthesis in Jupiter's atmosphere (Sagan et al, 1967;Raulin and Bossard, 1985;Guillemin, 2000). However, it is difficult to envision how the boundary conditions necessary for compartmentalizing the flow of energy and restricting the population of interacting molecules could be established under such conditions.…”
Section: Requirements For Lifementioning
confidence: 94%
“…That a fluid medium is necessary for harboring life is the most speculative of the proposed criteria, as the possibility that life could exist in dense atmospheres has also been suggested (Sagan and Salpeter, 1976). There is, for example, experimental and observational evidence for organic synthesis in Jupiter's atmosphere (Sagan et al, 1967;Raulin and Bossard, 1985;Guillemin, 2000). However, it is difficult to envision how the boundary conditions necessary for compartmentalizing the flow of energy and restricting the population of interacting molecules could be established under such conditions.…”
Section: Requirements For Lifementioning
confidence: 94%