Origin of water and mantle-crust interactions on Mars inferred from hydrogen isotopes and volatile element abundances of olivine-hosted melt inclusions of primitive shergottites

Earth and Planetary Science Letters

Volumn 357-358, Issue , 2012, Pages 119-129

  Usui, Tomohiro ^a,b   Alexander, Conel M O'D ^c   Wang, Jianhua ^c   Simon, Justin I ^a   Jones, John H ^a  

^a NASA JOHNSON SPACE CENTER   (United States)

^b LUNAR AND PLANETARY INSTITUTE   (United States)

^c GEOPHYSICAL LABORATORY   (United States)

Author keywords

Hydrogen isotope; Ion microprobe; Mantle crust interaction; Olivine hosted melt inclusion; Primordial Martian water; Volatile element

Indexed keywords

HYDROGEN ISOTOPE; ION MICROPROBE; MANTLE-CRUST INTERACTION; MELT INCLUSIONS; VOLATILE ELEMENTS;

BASALT; HYDROGEN; ISOTOPES; OLIVINE;

RESERVOIRS (WATER);

BASALT; CHONDRITE; CRUSTAL STRUCTURE; HYDROGEN ISOTOPE; ION MICROPROBE; MANTLE STRUCTURE; MARS; MELT INCLUSION; OLIVINE; SHERGOTTITE; VOLATILE ELEMENT;

EID: 84867612784     PISSN: 0012821X     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.epsl.2012.09.008     Document Type: Article

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