Abstract
Ozone (O3) is a key atmospheric gas in considerations of the photochemistry/chemistry of the paleoatmosphere, chemical evolution, and the origin and evolution of life. The photochemistry/chemistry of atmospheric O3 in the paleoatmosphere is investigated using a one-dimensional photochemical model that includes the chemistry of the oxygen, nitrogen, hydrogen, carbon, and chlorine gases. The role of cometary influx of H2O on the photochemistry of the paleoatmosphere is also examined. Recently, it has been suggested that our planet received a significant portion of the volatiles presently in the atmospheric/oceanic/biospheric system from cometary volatile influx. Several consequences of a cometary H2O influx on the photochemistry and structure of the paleoatmosphere are presented.
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Levine, J.S., Augustsson, T.R., Boughner, R.E., Natarajan, M., Sacks, L.J. (1981). Comets and the Photochemistry of the Paleoatmosphere. In: Ponnamperuma, C. (eds) Comets and the Origin of Life. Proceedings of the College Park Colloquia, vol 5. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-8528-5_13
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DOI: https://doi.org/10.1007/978-94-009-8528-5_13
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