Primitive olivine-phyric shergottite NWA 5789: Petrography, mineral chemistry, and cooling history imply a magma similar to Yamato-980459
Article first published online: 24 JAN 2011
© The Meteoritical Society, 2011
Meteoritics & Planetary Science
Volume 46, Issue 1, pages 116–133, January 2011
How to Cite
GROSS, J., TREIMAN, A. H., FILIBERTO, J. and HERD, C. D. K. (2011), Primitive olivine-phyric shergottite NWA 5789: Petrography, mineral chemistry, and cooling history imply a magma similar to Yamato-980459. Meteoritics & Planetary Science, 46: 116–133. doi: 10.1111/j.1945-5100.2010.01152.x
- Issue published online: 11 FEB 2011
- Article first published online: 24 JAN 2011
- (Received 28 April 2010; revision accepted 30 September 2010)
Table S1. Microprobe analyses of olivine.
Table S2. Microprobe analyses of pyroxene.
Table S3. Microprobe analyses of plagioclase.
|MAPS_1152_sm_online-supplemental-olivine.xls||244K||Supporting info item|
|MAPS_1152_sm_online-supplemental-plagioclase.xls||34K||Supporting info item|
|MAPS_1152_sm_online-supplemental-pyroxene.xls||85K||Supporting info item|
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