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Composition and Maturity of Apollo 16 Regolith Core 60013/14Samples from every half-centimeter dissection interval of double drive tube 60013/14 (sections 60013 and 60014) were analyzed by magnetic techniques for Fe concentration and surface maturity parameter I(sub s)/ Fe(O), and by neutron activation for concentrations of 25 lithophile and siderophile elements. Core 60013/14 is one of three regolith cores taken in a triangular array 40-50 m apart on the Cayley plains during Apollo 16 mission to the Moon. The core can be divided into three zones based both on I(sub s)/FeO and composition. Unit A (0-44 cm depth) is compositionally similar to other soils from the surface of the central region of the site and is mature throughout, although maturity decreases with depth. Unit B (44-59 cm) is submature and compositionally more feldspathic than Unit A. Regions of lowest maturity in Unit B are characterized by lower Sm/Sc ratios than any soil obtained from the Cayley plains as a result of some unidentified lithologic component with low surface maturity. The component is probably some type of mafic anorthosite that does not occur in such high abundance in any of the other returned soils. Unit C (59-62 cm) is more mature than Unit B and compositionally equivalent to an 87: 13 mixture of soil such as that from Unit A and plagioclase such as found in ferroan anorthosite. Similar soils, but containing greater abundances of anorthosite (plagioclase), are found at depth in the other two cores of the array. These units of immature to submature soil enriched to varying degrees (compared to the mature surface soil) in ferroan anorthosite consisting of approx. 99% plagioclase are the only compositionally distinct subsurface similarities among the three cores. Each of the cores contains other units that are compositionally dissimilar to any soil unit in the other two cores. These compositionally distinct units probably derive from local subsurface blocks deposited by the event(s) that formed the Cayley plains. The ferroan anorthosite with approx. 99% plagioclase, however, must represent some subsurface lithology that is significant on the scale of tens of meters. The compositional uniformity of the surface soil (0-10 cm depth) over distances of kilometers reflects the large-scale uniformity of the plains deposits; the fine- structure reflects small-scale nonuniformity and the inefficiency of the impact-mixing process at depths as shallow as even one meter.
Document ID
19980019865
Acquisition Source
Johnson Space Center
Document Type
Contractor Report (CR)
External Source(s)
doi:10.1016/0016-7037(93)90201-7
Authors
Korotev, Randy T. (Washington Univ. Saint Louis, MO United States)
Morris, Richard V. (Washington Univ. Saint Louis, MO United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Geochimica et Cosmochimica Acta
Publisher: Pergamon Press, Ltd.
Volume: 57
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
NAS 1.26:207235
NASA/CR-93-207235
Funding Number(s)
PROJECT: RTOP 152-17-40-21
CONTRACT_GRANT: NAG9-56
Distribution Limits
Public
Copyright
Public Use Permitted.

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