Efficiency of Haze Production in Titan's Primordial Atmosphere

Details Efficiency of Haze Production in Titan's Primordial Atmosphere Efficiency of Haze Production in Titan's Primordial Atmosphere

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ttt..work...82w&link_type=abstract

Through Time; A Workshop On Titan's Past, Present and Future, NASA Goddard Space Flight Center, April 6th - 8th, 2010. Edited b

Computer Science

Scientific paper

Titan's primordial atmosphere encountered an enhanced solar flux, which along with warmer temperatures, encouraged the conversion of primordial ammonia to the nitrogen gas that is dominant today. These conditions also likely had a significant effect on the chemistry responsible for the formation of haze precursors in Titan's atmosphere, as the atmosphere also contained copious methane and water vapor. A preliminary investigation into the efficiency and mechanisms of haze production during this evolutionary period will be presented. Constraints on haze production throughout Titan's evolution are important in characterizing the nature of Titan's thermal structure during this period as well as gaining insight into the role organic compounds played in Titan's evolutionary processes.

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