Compilation of Composition, Mineralogy, and Noble-Gas Content of Apollo 17 Particles and Soils and from the 73002 Drive Tube
Creator(s):
Cohen, Barbara A
Abstract:
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 this dataset:
Cohen, B. A., 2024. Compilation of Composition, Mineralogy, and Noble-Gas Content of Apollo 17 Particles and Soils and from the 73002 Drive Tube, Version 1.0. Interdisciplinary Earth Data Alliance (IEDA). https://doi.org/10.60520/IEDA/113144. Accessed 2025-08-31.
DOI Creation Date:
2024-03-15
Related Publication(s):
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