The imprint of atmospheric evolution in the D/H of hesperian clay minerals on Mars

Science

Volumn 347, Issue 6220, 2015, Pages 412-414

  Mahaffy, P R ^a   Webster, C R ^b   Stern, J C ^a   Brunner, A E ^a,c,d   Atreya, S K ^e   Conrad, P G ^a   Domagal Goldman, S ^a   Eigenbrode, J L ^a   Flesch, G J ^b   Christensen, L E ^b   Franz, H B ^a,d   Freissinet, C ^a,f   Glavin, D P ^a   Grotzinger, J P ^g   Jones, J H ^h   Leshin, L A ⁱ   Malespin, C ^a   McAdam, A C ^a   Ming, D W ^h   Navarro Gonzalez, R ^j   Niles, P B ^h   Owen, T ^k   Pavlov, A A ^a   Steele, A ^l   Trainer, M G ^a   Williford, K H ^b   Wray, J J ^m   more..

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c ARIZONA STATE UNIVERSITY   (United States)

^d UNIVERSITY OF MARYLAND   (United States)

^e UNIVERSITY OF MICHIGAN   (United States)

^f OAK RIDGE ASSOCIATED UNIVERSITIES   (United States)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h NASA JOHNSON SPACE CENTER   (United States)

ⁱ WORCESTER POLYTECHNIC INSTITUTE   (United States)

^j UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^k UNIVERSITY OF HAWAII   (United States)

^l GEOPHYSICAL LABORATORY   (United States)

^m GEORGIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

DEUTERIUM; HYDROGEN; HYDROXYL GROUP; SEA WATER; SURFACE WATER; WATER;

ARTICLE; ASTRONOMY; ATMOSPHERE; ATOM; CLAY; CRYSTAL STRUCTURE; CRYSTALLIZATION; FRACTIONATION; GEOLOGICAL TIME; HIGH TEMPERATURE; LOW TEMPERATURE; MASS SPECTROMETRY; PRIORITY JOURNAL; SPACE; ULTRAVIOLET RADIATION;

HESPERIA;

EID: 84921710917     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1260291     Document Type: Article

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