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- W2741424100 abstract "Theoretical models of solar nebula and early solar system chemistry which take into account the interplay between chemical, physical, and dynamical processes have great utility for deciphering the origin and evolution of the abundant chemically reactive volatiles (H, O, C, N, S) observed in comets. In particular, such models are essential for attempting to distinguish between presolar and solar nebula products _and for quantifying the nature and duration of nebular and early solar system proces.sing to which the volatile constituents of comets have been subjected. This talk will focus on the diverse processes and energy sources responsible for chemical processing in the solar nebula and early solar system. The processes to be considered include homogeneous and heterogeneous thermochemical and photochemical reactions, and disequilibration resulting from fluid transport, condensation, and cooling whenever they occur on time.scales shorter than those for chemical reactions. The energy sources to be considered include the thermal energy of the nebula, shock waves and photons fro!o lightning discharges, proto-solar and stellar photons, and radioactive decay processes. Plausible models for the chemical compositions of gases and volatile-bearing grains as a function of space and time in the nebula and in subnebulae arou.nd the giant plar_ets will be discussed." @default.
- W2741424100 created "2017-08-08" @default.
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- W2741424100 date "1988-01-01" @default.
- W2741424100 modified "2023-09-27" @default.
- W2741424100 title "CHEMISTRY IN THE SOLAR NEBULA AND EARLY SOLAR SYSTEM: IMPLICATIONS FOR THE CHEM-" @default.
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- W2741424100 hasPublicationYear "1988" @default.
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