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Nitrogen in Titan’s Atmospheric Aerosol Factory

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Book cover The Early Evolution of the Atmospheres of Terrestrial Planets

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 35))

Abstract

Titan’s organic aerosols are presumed to contain a large amount of nitrogen as inferred from the in situ measurements of the ACP instrument on board the Huygens probe. They show major emissions of ammonia and hydrogen cyanide after pyrolysis of the refractory nuclei of the atmospheric aerosols. Molecular nitrogen is a rather chemically inert molecule and the processes leading to the high nitrogen content of Titan’s aerosols are far from being understood. Here we synthesize the results obtained on Titan’s nitrogen composition from analysis of laboratory analogues produced with the PAMPRE experimental setup. These analogues are compared with the in situ measurements of the Cassini CAPS-IBS instrument.

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Acknowledgements

This work was financially supported by the ANR contract ANR-09-JCJC-0038.

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Correspondence to Nathalie Carrasco .

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Carrasco, N., Westlake, J., Pernot, P., Waite, H. (2013). Nitrogen in Titan’s Atmospheric Aerosol Factory. In: Trigo-Rodriguez, J., Raulin, F., Muller, C., Nixon, C. (eds) The Early Evolution of the Atmospheres of Terrestrial Planets. Astrophysics and Space Science Proceedings, vol 35. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-5191-4_11

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  • DOI: https://doi.org/10.1007/978-1-4614-5191-4_11

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