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Condensed-Phase Photochemical Processes in Titan's Aerosols and Surface: The Role of Longer Wavelength PhotochemistryWe will discuss photochemical properties of Titan's organic molecules in the condensed phase as solid aerosols or surface material, from small linear polyyenes (polyacetylenes and polycyanoacetylenes) such as C2H2, C4N2, HC5N, etc. In particular we will focus on photochemistry caused by longer wavelength UV-VIS photons (greater than 250 nm) photons that make it through Titan's atmosphere to the haze region (approximately 100 km) and on to the surface of Titan.
Document ID
20150007001
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/43927
Authors
Gudipati, Murthy S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jacovi, Ronen (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lignell, Antti (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Couturier, Isabelle (Provence Univ. Marseille, France)
Date Acquired
April 30, 2015
Publication Date
October 2, 2011
Subject Category
Lunar And Planetary Science And Exploration
Atomic And Molecular Physics
Inorganic, Organic And Physical Chemistry
Meeting Information
Meeting: EPSC-DPS Joint Meeting 2011
Location: Nantes
Country: France
Start Date: October 2, 2011
End Date: October 7, 2011
Sponsors: European Planetary Science Congress, American Astronomical Society
Distribution Limits
Public
Copyright
Other
Keywords
Surface area
atmosphere
photochemistry
Titan

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