Supporting chemical information for "Two slowly cooled and chemically diverse basalt clasts identified in ANGSA core 73001"
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Description
Dataset corresponds to electron microprobe mineral analyses collected for two Apollo 17 basalts. Data were collected at the University of Arizona using the Cameca SX-100 electron microprobe.
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How To Cite
Wilbur, Z., Tatsch, A., Barnes, J., Stadermann, A., Eckley, S., Erickson, T., Gross, J., Shearer, C., Zeigler, R., McCubbin, F., 2025. Supporting chemical information for "Two slowly cooled and chemically diverse basalt clasts identified in ANGSA core 73001", Version 1.0. Astromaterials Data Archive. https://doi.org/10.60520/IEDA/114151 Accessed 2026-09-29.
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Related Publication
Wilbur Z. E., Tatsch A. N., Barnes J. J., Stadermann A. C., Eckley S. A., Erickson T. M., Gross J., Shearer C. K., Zeigler R. A., McCubbin F. M., & the Angsa Science Team. (2025). Two slowly cooled and chemically diverse basalt clasts identified in ANGSA core 73001. Journal of Geophysical Research: Planets, 130(9), e2025JE009113.
Funding Sources
NASA 80NSSC19K0803
NASA 80NSSC21K0516
