火成岩
地质学
石油化学
分步结晶(地质学)
霞石
地球化学
火星人
火星探测计划
火星表面
过碱性岩
天体生物学
玄武岩
矿物学
火山
物理
作者
Edward M. Stolper,M. B. Baker,Megan Newcombe,M. E. Schmidt,A. H. Treiman,A. Cousin,M. D. Dyar,M. R. Fisk,R. Gellert,P. L. King,L. A. Leshin,S. Maurice,S. M. McLennan,M. E. Minitti,G. M. Perrett,Scott K. Rowland,V. Sautter,R. C. Wiens,Osku Kemppinen,Nathan Bridges
出处
期刊:Science
[American Association for the Advancement of Science (AAAS)]
日期:2013-09-26
卷期号:341 (6153): 1239463-1239463
被引量:166
标识
DOI:10.1126/science.1239463
摘要
“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).
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