Compilation of Composition, Mineralogy, and Noble-Gas Content of Apollo 17 Particles and Soils and from the 73002 Drive Tube
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Description
As part of the Apollo Next-Generation Sample Analysis (ANGSA) program, we provide bulk composition, mineralogy, petrology, and noble-gas assays of lunar particles and soils from the top half of the 73001/2 double-drive tube (i.e., 73002) studied by the ANGSA consortium. The particles are derived from lithologies of the South Massif, including anorthosites, anorthositic breccias, high-Ti basalts, noritic impact-melt breccias, agglutinates, and regolith breccias.
How To Cite
Cohen, B., 2024. Compilation of Composition, Mineralogy, and Noble-Gas Content of Apollo 17 Particles and Soils and from the 73002 Drive Tube, Version 1.0. Astromaterials Data Archive. https://doi.org/10.60520/IEDA/113144 Accessed 2026-09-29.
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Related Publication
Cohen, B. A., Curran, N. M., Valencia, S. N., Corrigan, C. M., Bullock, E. S., Alevy, E. G., et al. (2025). Composition, mineralogy, and noble gas content of Apollo 17 particles and soils from the 73002 drive tube. Journal of Geophysical Research: Planets, 130, e2024JE008329. https://doi.org/10.1029/2024JE008329
Funding Sources
NASA NNH18ZDA001N
