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- W1654421173 abstract "We have analyzed three shergottites (ALH 77005, EET 79001, Zagami), one orthopyroxenite (ALH 84001) and one nakhalite (Nakhla) by instrumental neutron activation analysis (INAA) for major, minor and trace elements, radiochemical neutron activation analysis (RNAA) for siderophiles and inductively-coupled plasma mass spectrometry (ICP-MS) for REE, Th and U. Our INAA data are generally in good agreement with the literature values for individual meteorites [1–3]. In spite of a large variety of petrological types, the constancy in Fe and, especially, Mn is remarkable. Very close coherence of Mn with Fe due to the similarity in ionic radius of Fe2+ and Mn2+ is obvious for martian materials, as observed for the terrestrial and lunar rocks." @default.
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- W1654421173 date "1998-07-01" @default.
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- W1654421173 title "Chemical Composition of Martian Meteorites" @default.
- W1654421173 hasPublicationYear "1998" @default.
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