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Thermal Gradients in the Outer Lunar Layers

Published online by Cambridge University Press:  07 February 2017

J. A. Bastin ,
S. J. Pandya  and
D. A. Upson
J. A. Bastin
Affiliation:
Queen Mary College, University of London, England
S. J. Pandya
Affiliation:
Queen Mary College, University of London, England
D. A. Upson
Affiliation:
Queen Mary College, University of London, England

Abstract

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During the next Apollo mission Apollo 15, it is planned to fix thermocouples at various depths up to 3 m below the lunar surface. It seems likely that the resulting temperature measurements will show a positive temperature differential with depth resulting from a net outward heat flux. It is the purpose of this paper to examine experiments already carried out which indicate a temperature gradient. Since the thermal flux is of direct importance in fundamental problems of lunar origin and the nature of the lunar interior, the relation between this quantity and the temperature gradient will be examined.

Type
Part II: Scientific Papers
Information
Symposium - International Astronomical Union , Volume 47: The Moon , 1972 , pp. 372 - 376
Copyright
Copyright © Reidel 1972 

References

Ade, P. A., Bastin, J. A., Marston, A. C., Pandya, S. J., and Puplett, E.: 1971, Proc. Second Lunar Science Conference 3, 2203.Google Scholar
Bastin, J. A., Clegg, P. E., and Fielder, G.: 1970, Proc. Apollo XI Lunar Science Conference 3, 1987.Google Scholar
Clegg, P. E., Pandya, S. J., Bastin, J. A., and Foster, S.: 1972, ‘Far Infrared Properties of Lunar Rock’, Proc. Third Lunar Science Conference, to be published.Google Scholar
Cremers, C. J., Birkebak, R. C., and Dawson, J. P.: 1970, Proc. Apollo XI Lunar Science Conference 3, 2045.Google Scholar
Cremers, C. J. and Birkebak, R. C.: 1971, Proc. Second Lunar Science Conference 3, 2311.Google Scholar
Gough, G. O., Pandya, S. J., and Bastin, J. A.: 1969, Private Communication.Google Scholar
Horai, K., Simmons, G., Kanamori, H., and Wones, D.: 1970, Proc. Apollo XI Lunar Science Conference 3, 2243.Google Scholar
Hoyt, H. Jr., Miyajima, M., Walker, R., Zimmerman, D., Zimmerman, J., Britton, D., and Kardos, J. L.: 1971, ‘Radiation Dose Rates and Thermal Gradients in the Lunar Regolith: Thermoluminescence and DTA of Apollo XII Samples’ 3, 2245.Google Scholar
Krotikov, V. D. and Troitskii, V. S.: 1963, Soviet Phys. Uspekhi 6, 841.Google Scholar
Langseth, M. G. Jr.: 1972, Third Lunar Science Conference 3, 475.Google Scholar
Linsky, J. L.: 1966, Icarus 5, 606.Google Scholar
MacDonald, G. J. F.: 1959, J. Geophys. Res. 64, 1967.Google Scholar
Sonett, C. P., Colburn, D. S., Dyal, P., Parkin, C. W., Smith, B. F., Schubert, G., and Schwartz, K.: 1971, Nature 230, 359.CrossRefGoogle Scholar