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Luna 24 origins - Some trace element constraintsLuna 24 basaltic material originated in the particular volume of the lunar crust that produced Apollo 11 and Luna 16 basaltic material; it has the same Clr/P2O5 (r = residual) signature. Ru-Os contents (Barsukov et al., 1977) and a number of radiogenic age measurements place Luna 24 basalt origins stratigraphically in a layer between those from which Apollo 15 and Apollo 11 and 17 basalts were derived.
Document ID
19790048532
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Jovanovic, S.
(Argonne National Lab. IL, United States)
Jensen, K. J.
(Argonne National Lab. IL, United States)
Reed, G. W., Jr.
(Argonne National Laboratory Argonne, Ill., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Mare Crisium: The view from Luna 24; Conference
Location: Houston, TX
Start Date: December 1, 1977
End Date: December 3, 1977
Sponsors: NSF
Accession Number
79A32545
Distribution Limits
Public
Copyright
Other

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