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
Publication DOI:
License:
Creative Commons Attribution 4.0 International [CC-BY-4.0]
Funding source(s):
National Aeronautics and Space Administration: NNH18ZDA001N
User Contributed Keyword(s):
Lunar, petrology, EMPA, EMP, EPMA, SEM, xCT, BSE, Noble gas, Ne, Ar, basalts, regolith, impact-melts, anorthosite, mg-suite, Moon
Data Available On:
2024-09-30
Resource Type:
Collection
Download File(s)
File Name
File Size
File Checksum
3144-1_ADA_Cohen_et_al_73002_EMP.xlsx
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3144-2_ADA_Cohen_et_al_73002_metadata_images.xlsx
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3144-3_ADA_Cohen_et_al_73002_NobleGas.xlsx
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3144-4_ADA_Cohen_et_al_73002_XRF.xlsx
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3144-5_ADA_Cohen_et_al_BSE_73002_183A.tif
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3144-6_ADA_Cohen_et_al_BSE_73002_183B.tif
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3144-7_ADA_Cohen_et_al_BSE_73002_183C.tif
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3144-8_ADA_Cohen_et_al_BSE_73002_184A.tif
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3144-9_ADA_Cohen_et_al_BSE_73002_184B.tif
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3144-10_ADA_Cohen_et_al_BSE_73002_184C.tif
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3144-11_ADA_Cohen_et_al_BSE_73002_184D.tif
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3144-12_ADA_Cohen_et_al_BSE_73002_186A.tif
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3144-13_ADA_Cohen_et_al_BSE_73002_186B.tif
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3144-14_ADA_Cohen_et_al_BSE_73002_187A.tif
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3144-15_ADA_Cohen_et_al_BSE_73002_187B_bottom.tif
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3144-16_ADA_Cohen_et_al_BSE_73002_187B_top.tif
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3144-17_ADA_Cohen_et_al_BSE_73002_187C.tif
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3144-18_ADA_Cohen_et_al_BSE_73002_187D.tif
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3144-19_ADA_Cohen_et_al_BSE_73002_188A.tif
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3144-20_ADA_Cohen_et_al_BSE_73002_188B.tif
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3144-21_ADA_Cohen_et_al_BSE_73002_188C.tif
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3144-22_ADA_Cohen_et_al_BSE_73002_189A.tif
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3144-23_ADA_Cohen_et_al_BSE_73002_189B.tif
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3144-24_ADA_Cohen_et_al_BSE_73002_189C.tif
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3144-25_ADA_Cohen_et_al_BSE_73002_189D.tif
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3144-26_ADA_Cohen_et_al_RGB_73002_183A_context-fig.pdf
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3144-27_ADA_Cohen_et_al_RGB_73002_183B_ContextImage.pdf
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3144-28_ADA_Cohen_et_al_RGB_73002_183C_ContextImage.pdf
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3144-29_ADA_Cohen_et_al_RGB_73002_184B_ContextImage.pdf
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3144-30_ADA_Cohen_et_al_RGB_73002_184C_Context.pdf
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3144-31_ADA_Cohen_et_al_RGB_73002_186A_context-fig.pdf
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3144-32_ADA_Cohen_et_al_RGB_73002_186B_Context.pdf
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3144-33_ADA_Cohen_et_al_RGB_73002_187A_Context.pdf
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3144-34_ADA_Cohen_et_al_RGB_73002_187B-Bottom_Context.pdf
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3144-35_ADA_Cohen_et_al_RGB_73002_187B-Top_Context.pdf
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3144-36_ADA_Cohen_et_al_RGB_73002_187C_Context.pdf
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3144-37_ADA_Cohen_et_al_RGB_73002_187D_Context.pdf
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3144-38_ADA_Cohen_et_al_RGB_73002_188A_Context.pdf
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3144-39_ADA_Cohen_et_al_RGB_73002_188B_Context.pdf
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3144-40_ADA_Cohen_et_al_RGB_73002_188C_Context.pdf
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3144-41_ADA_Cohen_et_al_RGB_73002_189A_Context.pdf
341.38 KB
3144-42_ADA_Cohen_et_al_XCT_73002-183_Tiff_Video.m4v
10.34 MB
3144-42_ADA_Cohen_et_al_RGB_73002_189C_contextimage.pdf
315.09 KB
3144-44_ADA_Cohen_et_al_XCT_73002-184_Tiff_Video.m4v
4.21 MB
3144-45_ADA_Cohen_et_al_XCT_73002-186_Tiff_Video.m4v
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3144-46_ADA_Cohen_et_al_XCT_73002-187_Tiff_Video.m4v
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3144-47_ADA_Cohen_et_al_XCT_73002-188_Tiff_Video.m4v
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3144-48_ADA_Cohen_et_al_XCT_73002-189_Tiff_Video.m4v
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