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Isotopes of nitrogen on Mars: Atmospheric measurements by Curiosity's mass spectrometer

[1] The Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) measured a Mars atmospheric(14)N/(15)N ratio of 173 ± 11 on sol 341 of the mission, agreeing with Viking's measurement of 168 ± 17. The MSL/SAM value was based on Quadrupole Mass Spectrometer measurement...

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Detalles Bibliográficos
Autores principales: Wong, Michael H, Atreya, Sushil K, Mahaffy, Paul N, Franz, Heather B, Malespin, Charles, Trainer, Melissa G, Stern, Jennifer C, Conrad, Pamela G, Manning, Heidi L K, Pepin, Robert O, Becker, Richard H, McKay, Christopher P, Owen, Tobias C, Navarro-González, Rafael, Jones, John H, Jakosky, Bruce M, Steele, Andrew
Formato: Online Artículo Texto
Lenguaje:English
Publicado: BlackWell Publishing Ltd 2013
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4459194/
https://www.ncbi.nlm.nih.gov/pubmed/26074632
http://dx.doi.org/10.1002/2013GL057840
Descripción
Sumario:[1] The Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) measured a Mars atmospheric(14)N/(15)N ratio of 173 ± 11 on sol 341 of the mission, agreeing with Viking's measurement of 168 ± 17. The MSL/SAM value was based on Quadrupole Mass Spectrometer measurements of an enriched atmospheric sample, with CO(2) and H(2)O removed. Doubly ionized nitrogen data at m/z 14 and 14.5 had the highest signal/background ratio, with results confirmed by m/z 28 and 29 data. Gases in SNC meteorite glasses have been interpreted as mixtures containing a Martian atmospheric component, based partly on distinctive(14)N/(15)N and(40)Ar/(14)N ratios. Recent MSL/SAM measurements of the(40)Ar/(14)N ratio (0.51 ± 0.01) are incompatible with the Viking ratio (0.35 ± 0.08). The meteorite mixing line is more consistent with the atmospheric composition measured by Viking than by MSL.