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Composition, Mineralogy, and Noble-Gas Content of Apollo 17 Particles and Soils from the 73002 Drive TubeAs part of the Apollo Next-Generation Sample Analysis (ANGSA) program, our Moon United team studied particles and soil samples from the 73001/2 drive tube to understand the lithologies at the sample site and provide constraints on the regolith age. We report the bulk composition, mineralogy, petrology, and noble-gas assays of 21 lunar particles and two soils. Our petrologic and noble-gas data constrain the origin and exposure and gardening history of the lunar regolith at the Apollo 17 site and thereby provide crucial context to the exposure history experienced by volatile and organic compounds in these samples.
Document ID
20240003410
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
B. A. Cohen
(Goddard Space Flight Center Greenbelt, United States)
N. M. Curran
(Catholic University of America Washington D.C., District of Columbia, United States)
S. N. Valencia
(University of Maryland, Baltimore County Baltimore, Maryland, United States)
E. S. Bullock
(Carnegie Institution for Science Washington, United States)
C. M. Corrigan
(Smithsonian Institution Washington, United States)
Date Acquired
March 19, 2024
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 55th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 11, 2024
End Date: March 15, 2024
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 718798.04.01.01.05
CONTRACT_GRANT: 80GSFC21M0002
CONTRACT_GRANT: 80NSSC19D0001
CONTRACT_GRANT: NNJ14ZKA001N
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
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