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Revised lunar heat-flow valuesThe 3.5- and 2-year subsurface temperature histories at the Apollo 15 and 17 heat-flow sites have been analyzed, and the results yield significantly lower thermal conductivity determinations than the results of previous short-term experiments. The thermal conductivity determined by probes at a depth of about 150 cm and 250 cm lies in the range 0.9-1.3 times 10 to the -4th W/cm K. On the basis of measurements of variations of surface thorium abundance and inferred crustal thicknesses, the average global heat flux is estimated to be about 1.8 microwatts/sq cm. This requires a uranium concentration of 46 ppb.
Document ID
19770051977
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Langseth, M. G.
(Lamont-Doherty Geological Observatory Palisades, NY, United States)
Keihm, S. J.
(Lamont-Doherty Geological Observatory Palisades, NY, United States)
Peters, K.
(Lamont-Doherty Geological Observatory Palisades, N.Y., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1976
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 15, 1976
End Date: March 19, 1976
Accession Number
77A34829
Funding Number(s)
CONTRACT_GRANT: NAS9-6037
CONTRACT_GRANT: NSG-7194
Distribution Limits
Public
Copyright
Other

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