1. Production of nitrogen oxides by lightning and coronae discharges in simulated early Earth, Venus and Mars environments
- Author
-
P. Coll, Rafael Navarro-González, François Raulin, D. Nna Mvondo, and C. P. McKay
- Subjects
Atmospheric Science ,Extraterrestrial Environment ,Earth, Planet ,Nitrous Oxide ,Aerospace Engineering ,Nitrogen oxides production ,Mars ,Venus ,Atmospheric sciences ,Nitric Oxide ,Lightning ,chemistry.chemical_compound ,Electricity ,Planet ,Nitrogen Fixation ,Maximum energy yield ,Electrical discharges ,Primitive atmospheres ,Range (particle radiation) ,biology ,Chemistry ,Atmosphere ,Astronomy and Astrophysics ,Earth ,Mars Exploration Program ,Nitrous oxide ,Carbon Dioxide ,Early Earth ,biology.organism_classification ,Coronae discharges ,Geophysics ,Space and Planetary Science ,General Earth and Planetary Sciences ,Evolution, Planetary ,Earth (classical element) ,Lightnings ,Nitrogen fixation rates - Abstract
7 pages, 1 figure., The original publication is available at http://www.sciencedirect.com/science/journal/02731177, We present measurements for the production of nitrogen oxides (NO and N2O) in CO2-N2 mixtures that simulate different stages of the evolution of the atmospheres of the Earth, Venus and Mars. The nitrogen fixation rates by two different types of electrical discharges, namely lightning and coronae, were studied over a wide range in CO2 and N2 mixing ratios. Nitric oxide (NO) is formed with a maximum energy yield estimated to be ~1.3×10^16 molecule/J at 80% CO2 and ~1.3×10^14 molecule/J at 50% CO2 for lightning and coronae discharges, respectively. Nitrous oxide (N2O) is only formed by coronae discharge with a maximum energy yield estimated to be ~1.2×10^13 molecule/J at 50% CO2. The pronounced difference in NO production in lightning and coronae discharges and the lack of formation of N2O in lightning indicate that the physics and chemistry involved in nitrogen fixation differs substantially in these two forms of electric energy., This work was supported by grants from the National Autonomous University of Mexico (DGAPAIN102796), the National Council of Science and Technology of Mexico (CONACyT 32531-T), the French-Mexican scientific research program ECOS/CONACyT-SEP-ANNUIES (M97U01), and the NASA Astrobiology program.
- Published
- 2001