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Primordial argon isotope fractionation in the atmosphere of Mars measured by the SAM instrument on Curiosity and implications for atmospheric loss

[1] The quadrupole mass spectrometer of the Sample Analysis at Mars (SAM) instrument on Curiosity rover has made the first high-precision measurement of the nonradiogenic argon isotope ratio in the atmosphere of Mars. The resulting value of (36)Ar/(38)Ar = 4.2 ± 0.1 is highly significant for it prov...

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Detalles Bibliográficos
Autores principales: Atreya, Sushil K, Trainer, Melissa G, Franz, Heather B, Wong, Michael H, Manning, Heidi L K, Malespin, Charles A, Mahaffy, Paul R, Conrad, Pamela G, Brunner, Anna E, Leshin, Laurie A, Jones, John H, Webster, Christopher R, Owen, Tobias C, Pepin, Robert O, Navarro-González, R
Formato: Online Artículo Texto
Lenguaje:English
Publicado: BlackWell Publishing Ltd 2013
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4373143/
https://www.ncbi.nlm.nih.gov/pubmed/25821261
http://dx.doi.org/10.1002/2013GL057763
Descripción
Sumario:[1] The quadrupole mass spectrometer of the Sample Analysis at Mars (SAM) instrument on Curiosity rover has made the first high-precision measurement of the nonradiogenic argon isotope ratio in the atmosphere of Mars. The resulting value of (36)Ar/(38)Ar = 4.2 ± 0.1 is highly significant for it provides excellent evidence that “Mars” meteorites are indeed of Martian origin, and it points to a significant loss of argon of at least 50% and perhaps as high as 85–95% from the atmosphere of Mars in the past 4 billion years. Taken together with the isotopic fractionations in N, C, H, and O measured by SAM, these results imply a substantial loss of atmosphere from Mars in the posthydrodynamic escape phase.