Prebiotic Atmospheric Chemistry on Titan


Roger Yelle


S. Horst, M. Allen, R. Amils, S. K. Atreya G. Bampasidis, A. Bar-Nun, P. Beauchamp, M. Cabane, M. Capria, R. Carlson, N. Carrasco, A. Coates, J. Cooper,M. Combes, T. Cours, H. Cottin, A. Coustenis, T. Cravens, J. Cui, R. de Kok, I. dePater, M. Dobrijevic, G. Durry, Y. Dutil, O. Dutuit, M. Fulchignoni, M. Galand,Y. Gao, D. Gautier, M. Gurwell, E. Hebrard, F. Hersant, H. Imanaka; W. Ip, R. Jaumann, A. Jolly, S. Karoly, E. Kostiuk, L.-M. Lara, P. Lavvas, S. Lebonnois, J.-P. Lebreton, M. Leese, S. Le Mou_elic, T. Livengood, R. Lopes, J. Lopez-Moreno, J. Lunine, P. Mahaffy, V. Mangano, T. McCord, R. Modolo, A. Morse, O. Mousis, I. Muller-Wodarg, A. Mura, G. Murthy C. Nixon, D. Nna-Mvondo, L. Norman, G. Ortega, G. Orton, M. Patel, A. Pavlov, C. Plainaki, P. Rannou K. Reh, M. Rengel, F. Robb, S. Rodriguez, R. Rodrigo, E. Schaller, B. Schmitt, D. Schulze-Makuch, E. Sciamma O''Brien, J. Soderblom, A. Somogyi, E. Sittler, D. Strobel, L. Spilker, T. Spilker, M. Smith, A. Steele, K. Stephan, N. Strange, C. Szopa, R. Thissen, F. Tosi, D. Toublanc, M. Trainer S. Tripathi, S. Ulamec, S. Vinatier, V. Vuitton, J.-E. Wahlund, J. H. Waite, M. Yamauchi, J. Zarnecki

Panel Selection:

Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.


University of Arizona

Cassini measurements reveal that organic molecules with molecular weights of hundreds of amu are formed by photochemistry in Titan''s upper atmosphere. Investigating this chemistry is important for understanding the production of biological building blocks by naturally occurring processes.


Please let us know if you find any discrepancies or inaccuracies.

Keep Exploring

Discover More Topics From NASA