The photochemical fractionation of nitrogen isotopologues in Titan's atmosphere

Nitrogen isotopologues could give in principle valuable constraints on the formation and evolution of Titan's atmosphere and its interior over geological time. For this purpose, we developed the first photochemical model dedicated to the study of the fractionation of several nitrogen isotopologues. Emphasis has been placed on several nitriles: HCN, CH3CN, HC3N, C2H3CN, C2H5CN. We show that the HCN/HC15N and HC3N/HC315N ratios are very sensitive to the production of magnetospheric electrons. So, these compounds can serve as probes to study the putative evolution with time of the production of magnetospheric electrons throughout the atmosphere. We also show that the CH3CN/CH3C15N and C2H5CN/C2H5C15N ratios are highly sensitive to cosmic rays. So, they can serve as probes to estimate their effect in the lower atmosphere of Titan (100-300 km). Detection of new isotopologues (particularly CH3C15N) could give strong constraints to photochemical models and could improve our understanding of the main physical and chemical processes at work in Titan's atmosphere.