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The petrochemistry of Jake-M: A martian mugearite

MSL Science Team, E. M. Stolper*, M. B. Baker, M. E. Newcombe, M. E. Schmidt, A. H. Treiman, A. Cousin, M. D. Dyar, M. R. Fisk, R. Gellert, P. L. King, L. Leshin, S. Maurice, S. M. McLennan, M. E. Minitti, G. Perrett, S. Rowland, V. Sautter, R. C. Wiens, Osku KemppinenNathan Bridges, Jeffrey R. Johnson, David Cremers, James F. Bell, Lauren Edgar, Jack Farmer, Austin Godber, Meenakshi Wadhwa, Danika Wellington, Ian McEwan, Claire Newman, Mark Richardson, Antoine Charpentier, Laurent Peret, Jennifer Blank, Gerald Weigle, Shuai Li, Ralph Milliken, Kevin Robertson, Vivian Sun, Christopher Edwards, Bethany Ehlmann, Kenneth Farley, Jennifer Griffes, John Grotzinger, Hayden Miller, Sam Clegg, David K. Martin, Michael D. Smith, Sharon A. Wilson, Robert Downs

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

154 Citations (Scopus)

Abstract

"Jake-M," the first rock analyzed by the Alpha Particle X-ray Spectrometer instrument on the Curiosity rover, differs substantially in chemical composition from other known martian igneous rocks: It is alkaline (>15% normative nepheline) and relatively fractionated. Jake-M is compositionally similar to terrestrial mugearites, a rock type typically found at ocean islands and continental rifts. By analogy with these comparable terrestrial rocks, Jake-M could have been produced by extensive fractional crystallization of a primary alkaline or transitional magma at elevated pressure, with or without elevated water contents. The discovery of Jake-M suggests that alkaline magmas may be more abundant on Mars than on Earth and that Curiosity could encounter even more fractionated alkaline rocks (for example, phonolites and trachytes).

Original languageEnglish
Article number1239463
JournalScience
Volume341
Issue number6153
DOIs
Publication statusPublished - 2013
Externally publishedYes

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