NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Thorium concentrations in the lunar surface. III - Deconvolution of the Apenninus regionA technique of deconvoluting orbital-gamma ray data which improves spatial resolution and contrast has been applied to Th concentrations in the Apenninus region of the moon. The highest concentration seen from orbit has been found along the northern edge of the data track at Archimedes, requiring a component more highly fractionated in KREEP than the Apollo 15 medium-K Fra Mauro basalt. The results show generally diminishing Th levels extending outward from the Imbrium Basin, and impact penetration of basalt flows in Mare Imbrium to eject sub-mare Th-rich material. The results reinforce the hypothesis that the highlands which border and underlie the western maria contain a pre-mare layer of volcanically-derived KREEP material.
Document ID
19800039482
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Metzger, A. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Haines, E. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Etchegaray-Ramirez, M. I.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Hawke, B. R.
(Hawaii, University Honolulu, Hawaii, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 19, 1979
End Date: March 23, 1979
Accession Number
80A23652
Funding Number(s)
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NSG-7312
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available