title: Chemical evolution on Titan: comparisons to the prebiotic earth.
abstract: Models for the origin of Titan's atmosphere, the processing of the atmosphere and surface and its exobiological role are reviewed. Titan has gained widespread acceptance in the origin of life field as a model for the types of evolutionary processes that could have occurred on prebiotic Earth. Both Titan and Earth possess significant atmospheres (> or = 1 atm) composed mainly of molecular nitrogen with smaller amounts of more reactive species. Both of these atmospheres are processed primarily by solar ultraviolet light with high energy particles interactions contributing to a lesser extent. The products of these reactions condense or are dissolved in other atmospheric species (aerosols/clouds) and fall to the surface. There these products may have been further processed on Titan and the primitive Earth by impacting comets and meteorites. While the low temperatures on Titan (approximately 72-180 K) preclude the presence of permanent liquid water on the surface, it has been suggested that tectonic activity or impacts by meteors and comets could produce liquid water pools on the surface for thousands of years. Hydrolysis and oligomerization reactions in these pools might form chemicals of prebiological significance. Other direct comparisons between the conditions on present day Titan and those proposed for prebiotic Earth are also presented.
authors.affiliation: Department of Chemistry and Physics, Northwestern State University, Natchitoches, LA 71497, USA.
authors.forename: D W
authors.initials: DW
authors.lastname: Clarke
authors.forename: J P
authors.initials: JP
authors.lastname: Ferris
mesh_terms: D001272:Atmosphere; D002241:Carbohydrates / Q000032:analysis; D018534:Earth, Planet; D019418:Evolution, Chemical; D005615:Freezing; D019110:Meteoroids; D018539:Saturn; D013995:Time; D014867:Water
chemical_list: D002241:Carbohydrates; D014867:Water