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Thermal diffusivity of four Apollo 17 rock samplesThe modified Angstrom technique was used to measure the thermal diffusivity of four Apollo 17 rock samples in air at pressures of 1 atm and one-millionth torr in the temperature range 80-460 K, and in CO2 at different pressures for various temperature ranges and at different temperatures for the range of interstitial CO2 gas pressure 1 atm to 0.0001 torr. The experiments with CO2 were intended to simulate Martian conditions, and it was found that the thermal diffusivity of lunar crystalline basalt and breccia varies very little with temperature in a simulated Martian environment, which indicates that the thermal processes in the Martian regolith could be more straightforward than in the lunar regolith.
Document ID
19770051979
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Horai, K.-I.
(NASA Johnson Space Center Geochemistry Branch, Houston, Tex.; Lamont-Doherty Geological Observatory, Palisades, N.Y., United States)
Winkler, J. L., Jr.
(Lockheed Electronics Co., Inc. Houston, Tex., 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
77A34831
Funding Number(s)
CONTRACT_GRANT: NGR-33-008-177
Distribution Limits
Public
Copyright
Other

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