Journal
ICARUS
Volume 254, Issue -, Pages 259-261Publisher
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2015.03.025
Keywords
Atmospheres, evolution; Titan, atmosphere; Mars, atmosphere; Atmospheres, composition; Atmospheres, dynamics
Categories
Funding
- NASA [NNX13AQ99G]
- CNES
- A*MIDEX project [ANR-11-IDEX-0001-02]
- Investissements d'Avenir French Government program
- NASA [NNX13AQ99G, 464448] Funding Source: Federal RePORTER
Ask authors/readers for more resources
We present here a comparative planetology study of evolution of N-14/N-15 at Mars and Titan. Studies show that N-14/N-15 can evolve a great deal as a result of escape in the atmosphere of Mars, but not in Titan's atmosphere. We explain this through the existence of an upper limit to the amount of fractionation allowed to occur due to escape that is a function of the escape flux and the column density of nitrogen. (C) 2015 Elsevier Inc. All rights reserved.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available
Share Paper
