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Silicate mineralogy of martian meteorites

Papike, J. J., Karner, J. M., Shearer, C. K., Burger, P. V.(2009). Silicate mineralogy of martian meteorites. Geochimica et Cosmochimica Acta, 73(24), 7443-7485. https://doi.org/10.1016/j.gca.2009.09.008

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Datasets

numbertitleMethodsvariables analyzed
2Average plagioclase (maskelynite) composition for each meteoriteEMP, CALCK2O, ALBITE, Fe2O3, TOTAL, ORTHOCLASE, CaO, SiO2, MgO, Na2O, Al2O3, ANORTHITE
3Average olivine composition for each meteoriteEMPAl2O3, Co, Ni, Cr2O3, FeO, MgO, TOTAL, CaO, MnO, SiO2, TiO2
4Average pyroxene composition for eachEMP, CALCTOTAL, Na2O, SiO2, ENSTATITE, Cr2O3, Fe2O3, CaO, WOLLASTONITE, FERROSILITE, TiO2, FeO, Al2O3, MgO, MnO

Methods

method namelaboratorymethod comment More details are available for the following variables
CALCULATEDUNKNOWNN/A
ELECTRON MICROPROBEUNIVERSITY OF NEW MEXICOJEOL 733 Superprobe equipped with a back-scattered electron detector, a thin-window energy dispersive spectrometer, and five WDS, all controlled by an Oxford eXL II analyzer system. Plagioclase analysis conditions: accelerating voltage of 15 kV, a beam current of 20 nA, and a beam diameter of 10 lm. A beam diameter of 10 lm minimized loss of vola- tile elements such as Na and K during feldspar analyses. OL & PX grains analyzed under the same conditions as plagioclase, except that the beam size 1 lm.

Samples

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