scholarly journals An experimental test for the mass independent isotopic fractionation mechanism proposed for ozone

2019 ◽  
Vol 523 ◽  
pp. 191-197 ◽  
Author(s):  
François Robert ◽  
Lambert Baraut-Guinet ◽  
Pierre Cartigny ◽  
Peter Reinhardt
2021 ◽  
Vol 923 (2) ◽  
pp. 196
Author(s):  
Min Liu ◽  
Pan Jiang ◽  
Liya Lu ◽  
Tonghui Yin ◽  
Liying Ma ◽  
...  

Abstract The origin and evolution of the 14N/15N ratio of Titan’s atmosphere has long been a subject of debate. Clearly a better understanding of the N isotopic fractionation mechanism would greatly help resolve this. Photodissociation of N2 by solar radiation has been suggested to either play a negligible role in fractionating the N isotopes in Titan, due to its rather low escape velocity, or to preferentially remove 15N through self-shielding controlled photochemical reactions. Here, we systematically measure the branching ratios of 14N15N between N(4S)+N(2P) and N(4S)+N(2D) channels. We find that many of its absorption states predominantly dissociate into N(4S)+N(2P) with a strong isotope effect between 14N2 and 14N15N. Since N atoms produced from N(4S)+N(2P) acquire velocities close to Titan’s escape velocity, these findings provide a new N isotope fractionation mechanism for Titan that has not been considered before, potentially providing important constraints on the origin and evolution of Titan’s N2-dominated atmosphere.


2021 ◽  
Vol 40 (9) ◽  
pp. 43-52
Author(s):  
Lianhua He ◽  
Jihua Liu ◽  
Hui Zhang ◽  
Jingjing Gao ◽  
Aimei Zhu ◽  
...  

1989 ◽  
Vol 44 (5) ◽  
pp. 435-444 ◽  
Author(s):  
S. K. Bhattacharya ◽  
M. H. Thiemens

The isotopic fractionation associated with the O + CO reaction has been studied using oxygen atoms produced by room temperature O2 photolysis at two different wavelengths, 185 and 130 nm. A large mass-independent isotopic fractionation is observed in the product CO2, extending the range of this type of reaction beyond O + O2 and SF5 + SF5. Kinetic evaluation of the data restricts the source of the mass-independent fractionation mechanism to the O + CO recombination step rather than O2 photolysis, secondary ozone formation, or O2 photodissociation. At least one, and most likely two other fractionation processes appear to occur in the experiments, and interpretation of the isotopic results is tentative at present. Based on the relevant reaction rates and the value for the reduced partition function for isotopic exchange between O and CO, it is suggested that this process may occur prior to the δ17O≅δ18O recombination process. Secondary CO2 photolysis may superimpose an additional fractionation. The experimental data are also examined in the context of a model based upon energy randomization rates versus the lifetime of the activated complex.


2008 ◽  
Vol 27 (3, Suppl) ◽  
pp. S197-S206 ◽  
Author(s):  
Andrew W. Hertel ◽  
Emily A. Finch ◽  
Kristina M. Kelly ◽  
Christie King ◽  
Harry Lando ◽  
...  

2011 ◽  
Author(s):  
Jay O. Castaneda ◽  
Suzanne Segerstrom
Keyword(s):  

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