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Possible Thermal History of the Moon

Published online by Cambridge University Press:  07 February 2017

Peter E. Fricker ,
Ray T. Reynolds  and
Audrey L. Summers
Peter E. Fricker
Affiliation:
Ames Research Center, NASA, Moffett Field, California, U.S.A.
Ray T. Reynolds
Affiliation:
Ames Research Center, NASA, Moffett Field, California, U.S.A.
Audrey L. Summers
Affiliation:
Ames Research Center, NASA, Moffett Field, California, U.S.A.

Abstract

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The possible thermal history of the Moon is investigated by means of theoretical models. The calculations include the effects of melting and time-dependent redistribution of radioactive heat sources. The known constraints can best be satisfied by a model which is characterized by relatively high initial temperatures close to the melting range; melting and, consequently, fractionation and redistribution of radionuclides would occur during the first 1.5 × 109 yr and would then be followed by an effective cooling process. Heat flow measurements on the lunar surface should permit a distinction between such a completely fractionated model and a non-fractionated model or a model with restricted fractionation in the outer few hundred kilometers.

Type
Part II: Scientific Papers
Information
Symposium - International Astronomical Union , Volume 47: The Moon , 1972 , pp. 384 - 391
Copyright
Copyright © Reidel 1972 

References

Akimoto, S. I., Nishikawa, M., Nakamura, Y., Kushiro, I., and Katsura, T.: 1970, Geochim. Cosmochim. Acta, Suppl. 1, Proceedings of the Apollo 11 Lunar Science Conference, 129.Google Scholar
Albee, A., Burnett, D. S., Chodos, A. A., Eugster, O. J., Huneke, J. C., Papanastassiou, D. A., Podosek, F. A., Price Russ, G. II, Sanz, H. G., Tera, F., and Wasserburg, G. W.: 1970, Science 167, 463.Google Scholar
Albee, A., Burnett, D. S., Chodos, A. A., Haines, E., Huneke, J. C., Papanastassiou, D. A., Podosek, F. A., Price Russ, G. II, Tera, F., and Wasserburg, G. W.: 1971, 1971 Lunar Science Conference Abstracts, Houston, Texas, 56.Google Scholar
Cohen, L. H., Ito, K., and Kennedy, G. C.: 1967, Am. J. Sci. 265, 475.CrossRefGoogle Scholar
Compston, W., Chappell, B. W., Arriens, P. A., and Vernon, M. J.: 1970, Geochim. Cosmochim. Acta, Suppl. 1, Proceedings of the Apollo 11 Lunar Science Conference, 1007.Google Scholar
Fricker, P. E., Reynolds, R. T., and Summers, A. L.: 1967, J. Geophys. Res. 72, 2649.Google Scholar
Fricker, P. E., Goldstein, J. I., and Summers, A. L.: 1970, Geochim. Cosmochim. Acta 34, 475.Google Scholar
Goldschmidt, V. M.: 1954, Geochemistry, Oxford at the Clarendon Press, p. 730.Google Scholar
Kopal, Z.: 1962, ‘Thermal History of the Moon and of the Terrestrial Planets: Numerical Results’, TR 32-225, Jet Propulsion Laboratory, California Institute of Technology.Google Scholar
Kushiro, I., Yoder, H. S. Jr., and Nichikawa, M.: 1968, Geol. Soc. Am. Bull. 79, 1685.Google Scholar
Levin, B. J.: 1962, in Kopal, Z. and Mikhailov, Z. K. (eds.), The Moon, Academic Press, New York, p. 157.Google Scholar
LSPET (Lunar Sample Preliminary Examination Team): 1969, Science 165, 1222.Google Scholar
LSPET (Lunar Sample Preliminary Examination Team): 1970, Science 167, 1325.Google Scholar
MacDonald, G. J. F.: 1959, J. Geophys. Res. 64, 1967.Google Scholar
MacDonald, G. J. F.: 1962, J. Geophys. Res. 67, 2945.Google Scholar
Maeva, S. V.: 1965, Soviet Phys. Dokl. 9, 945.Google Scholar
McConnell, R. K., McClaine, L., Lee, D., Aaronson, J., and Allen, J.: 1967, Rev. Geophys. 5, 121.Google Scholar
Phinney, R. A. and Anderson, D. L.: 1965, ‘Internal Temperatures of the Moon’, Minnesota University Rept., Tycho Meeting.Google Scholar
Reynolds, R. T. and Summers, A. L.: 1969, J. Geophys. Res. 74, 2494.CrossRefGoogle Scholar
Reynolds, R. T., Fricker, P. E., and Summers, A. L.: 1966, J. Geophys. Res. 71, 573.Google Scholar
Reynolds, R. T., Fricker, P. E., and Summers, A. L.: in Lucas, J. (ed.), Lunar Thermal Characteristics, AIAA Progress Series (in press).Google Scholar
Ringwood, A. E. and Essene, E.: 1970, Geochim. Cosmochim. Acta, Suppl. 1, Proceedings of the Apollo 11 Lunar Science Conference, 769.Google Scholar
Runcorn, S. K.: 1962, Nature 195, 1150.Google Scholar
Sonett, C. P. and Colburn, D. S.: 1968, Nature 219, 924.Google Scholar
Tatsumoto, M.: 1970, Geochim. et Cosmochim. Acta, Suppl., Proceedings of the Apollo 11 Lunar Science Conference, 1595.Google Scholar
Turner, G.: 1970, Geochim. Cosmochim. Acta, Suppl. 1, Proceedings of the Apollo 11 Lunar Science Conference, 1665.Google Scholar
Turner, G.: 1971, 1971 Lunar Science Conference Abstracts, Houston, Texas, p. 63.Google Scholar
Urey, H. C.: 1952, The Planets: Their Origin and Development, Yale University Press, New Haven, Conn.Google Scholar
Urey, H. C.: 1962, in Kopal, Z. (ed.), Physics and Astronomy of the Moon, Academic Press, New York, p. 481.Google Scholar
Urey, H. C. and MacDonald, G. J. F.: in Kopal, Z. (ed.), Physics and Astronomy of the Moon, 2nd ed., Academic Press, New York (to be published).Google Scholar
Wakita, H., Schmitt, R. A., and Rey, P.: 1970, Geochim. Cosmochim. Acta. Suppl. 1, Proceedings of the Apollo 11 Lunar Science Conference, 1685.Google Scholar
Wasserburg, G. J., MacDonald, G. J. F., Hoyle, F., and Fowler, W. A.: 1964, Science 143, 465.Google Scholar
Wood, J. A.: in Simmons, G. (ed.), The Geophysical Interpretation of the Moon, preprint Sept. 1970 (to be published).Google Scholar