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Mars atmosphere. The imprint of atmospheric evolution in the D/H of Hesperian clay minerals on Mars

The deuterium-to-hydrogen (D/H) ratio in strongly bound water or hydroxyl groups in ancient martian clays retains the imprint of the water of formation of these minerals. Curiosity's Sample Analysis at Mars (SAM) experiment measured thermally evolved water and hydrogen gas released between 550°... Full description

1st Person: Mahaffy, P R
Additional Persons: Webster, C R; Stern, J C; Brunner, A E; Atreya, S K; Conrad, P G; Domagal-Goldman, S; Eigenbrode, J L; Flesch, G J; Christensen, L E; Franz, H B; Freissinet, C; Glavin, D P; Grotzinger, J P; Jones, J H; Leshin, L A; Malespin, C; McAdam, A C; Ming, D W; Navarro-Gonzalez, R; Niles, P B; Owen, T; Pavlov, A A; Steele, A; Trainer, M G; Williford, K H; Wray, J J
Source: in Science Vol. 347, No. 6220 (2015), p. 412
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Type of Publication: Article
Language: English
Published: 2015
Online: http://www.ncbi.nlm.nih.gov/pubmed/25515119
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