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Comparative Planetary Mineralogy: Co, Ni Systematics in Chromite from Planetary BasaltsSpinel is a minor but important phase in planetary basalts because its variable composition often reflects basalt petrogenesis. For example, complicated zoning trends in spinel can give clues to melt evolution [1], and V concentrations in chromite lend insight into magma oxygen fugacity (fO2) conditions [2]. Nickel and Co are two elements that are commonly used as a measure of melt fractionation, and their partitioning between olivine and melt is fairly well understood. Less clear is their partitioning into spinel, although [3] has explored Ni and Co systematics in experimental charges. This study documents Ni and Co behavior in early crystallizing spinel (chromite) from several planetary basalts in an attempt to compare our results with [3], and also gain insight into basalt evolution on the three planets.
Document ID
20050170562
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Karner, J. M.
(New Mexico Univ. Albuquerque, NM, United States)
Shearer, C. K.
(New Mexico Univ. Albuquerque, NM, United States)
Papike, J. J.
(New Mexico Univ. Albuquerque, NM, United States)
Righter,K.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Publication Information
Publication: Lunar and Planetary Science XXXVI, Part 11
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Public Use Permitted.
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