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Induced and Permanent Magnetism on the Moon: Structural and Evolutionary Implications

Published online by Cambridge University Press:  30 March 2016

C. P. Sonett
Affiliation:
Ames Research Center, NASA, Moffett Field, Calif., U.S.A.
P. Dyal
Affiliation:
Ames Research Center, NASA, Moffett Field, Calif., U.S.A.
D. S. Colburn
Affiliation:
Ames Research Center, NASA, Moffett Field, Calif., U.S.A.
B. F. Smith
Affiliation:
Space Sciences Department, University of California at Los Angeles, Calif., U.S.A.
G. Schubert
Affiliation:
Space Sciences Department, University of California at Los Angeles, Calif., U.S.A.
K. Schwartz
Affiliation:
American Nucleonics Corporation, Woodland Hills, Calif., U.S.A.
J. D. Mihalov
Affiliation:
Ames Research Center, NASA, Moffett Field, Calif, U.S.A.
C. W. Parkin
Affiliation:
Ames Research Center, NASA, Moffett Field, Calif, U.S.A.

Abstract

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It is shown that the Moon possesses an extraordinary response to induction from the solar wind due to a combination of a high interior electrical conductivity together with a relatively resistive crustal layer into which the solar wind dynamic pressure forces back the induced field. The dark side response, devoid of solar wind pressure, is approximately that expected for the vacuum case. These data permit an assessment of the interior conductivity and an estimate of the thermal gradient in the crustal region. The discovery of a large permanent magnetic field at the Apollo 12 site corresponds approximately to the paleomagnetic residues discovered in both Apollo 11 and 12 rock samples The implications regarding an early lunar magnetic field are discussed and it is shown that among the various conjectures regarding the early field the most prominent are either an interior dynamo or an early approach to the Earth though no extant model is free of difficulties.

Type
II. Special Meeting on Direct Exploration of the Moon
Copyright
Copyright © Reidel 1971

References

Bibliography

[1] Gold, T.: 1966, ‘The Magnetosphere of the Moon’, in The Solar Wind (ed. by Mackin, R. J. and Neugebauer, M.), Pergamon Press, New York.Google Scholar
[2] Dolginov, Sh.Sh., Eroshenko, E. G., Zhozov, L. N., and Pushkov, N. V.: 1966, ‘Measurements of the Magnetic Field in the Vicinity of the Moon by the Artificial Satellite Luna 10’, Dokl. Akad. Nauk U.S.S.R. 170, 574.Google Scholar
[3] Colburn, D. S., Currie, R. G., Mihalov, J. D., and Sonett, C. P.: 1967, ‘Diamagnetic Solar Wind Cavity Discovered Behind the Moon’, Science 158, 1040.CrossRefGoogle Scholar
[4] Sonett, C. P., Colburn, D. S., and Currie, R. G.: 1967, ‘The Intrinsic Magnetic Field of the Moon’, J. Geophys. Res. 72, 5503.CrossRefGoogle Scholar
[5] Ness, N. F., Behannon, K. W., Scearce, C. S., and Cantarano, S. C.: 1969, ‘Early Results of the Magnetic Field Experiment on Lunar Explorer 35’, J. Geophys. Res. 72, 5769.CrossRefGoogle Scholar
[6] Ness, N. F.: 1971, ‘Interaction of the Solar Wind with the Moon’, NASA/GSFC preprint X692-70-141, Proc. STP Leningrad Symposium, Reidel, D., Dordrecht, in press.Google Scholar
[7] Apollo 12 Preliminary Science report NASA SP-235 (1970).Google Scholar
[8] Sonett, C. P. and Dyal, P.: 1970, ‘The Moon: Global Electromagnetic Sounding Using the Solar Wind’, Comments Astrophys. Space Phys. 2, 5.Google Scholar
[9] Sonett, C. P. and Colburn, D. S.: 1967, ‘Establishment of a Lunar Unipolar Generator and Associated Shock and Wake by the Solar Wind’, Nature 216, 340.CrossRefGoogle Scholar
[10] Sonett, C. P. and Colburn, D. S.: 1968, ‘The Principle of Solar Wind Induced Dynamos’, Earth Planetary Interiors 1, 326.CrossRefGoogle Scholar
[11] Schubert, J. and Schwartz, K.: 1969, ‘A Theory for the Interpretation of Lunar Surface Magnetometer Data’, The Moon 1, 106.CrossRefGoogle Scholar
[12] Sill, W. R. and Blank, J. L.: 1970, ‘Method for Estimating the Electrical Conductivity of the Lunar Interior’, J. Geophys. Res. 75, 201.CrossRefGoogle Scholar
[13] Ness, N. F.: ‘Interaction of the Moon with the Solar Wind’, Proc. STP Leningrad Symposium, Reidel, D., Dordrecht, in press. Also, Proc. Kiev Conference on the Moon and Planets, October 1968, in press.Google Scholar
[14] Behannon, K. E.: 1968, ‘Intrinsic Magnetic Properties of the Lunar Body’, J. Geophys. Res. 73, 7257.CrossRefGoogle Scholar
[15] Buhler, F., Eberhardt, P., Geiss, J., Meister, J., and Signer, P.: 1969, ‘Apollo U Solar Wind Composition Experiment: First Results’, Science 166, 1502.CrossRefGoogle Scholar
[16] Ogilvie, K. W. and Ness, N. F.: 1969, ‘Dependence of the Lunar Wake on Solar Wind Plasma Characteristics’, J. Geophys. Res. 74, 4123.CrossRefGoogle Scholar
[17] Sonett, C. P., Dyal, P., Parkin, C. W., Colburn, D. S., Mihalov, J. D., and Smith, B. F.: ‘On the Whole Body Response of the Moon to Electromagnetic Induction by the Solar Wind’, Science, in press.Google Scholar
[18] Nagata, T., Rikitake, T., and Kono, M.: 1900, ‘Electrical Conductivity and the Age of the Moon’, preprint.Google Scholar
[19] England, A. W., Simmons, G., and Strangway, D.: 1968, ‘Electrical Conductivity of the MoonJ. Geophys. Res. 73, 3219.CrossRefGoogle Scholar
[20] Dyal, P., Parkin, C. W., and Sonett, C. P.: 1970, ‘Apollo 12 Magnetometer: Measurement of a Steady Magnetic Field on the Surface of the Moon’, Science 169, 762.CrossRefGoogle ScholarPubMed
[21] Strangway, D. W., Larson, E. E., and Pearce, G. W.: ‘Magnetic Studies of Lunar Samples-Breccia and Fines’, pp. 2435-2451.Google Scholar
Runcorn, S. K., Collinson, D. W., O’Reilly, W., Battey, M. H., Stephenson, A., Jones, J. M., Manson, A. J., and Readman, P. W.: ‘Magnetic Properties of Apollo 11 Lunar Samples’, pp. 2369-2387.Google Scholar
Nagata, T., Ishikawa, Y., Kinoshita, H., Kono, M., Syono, Y., and Fisher, R. M.: ‘Magnetic Properties and Natural Remanent Magnetism of Lunar Materials’, pp. 2325-2340.Google Scholar
Larochelle, A. and Schwartz, E. J.: ‘Magnetic Properties of Apollo 11 Sample 10048-22’, pp. 2305-2308.Google Scholar
Helseley, C. E.: ‘Magnetic Properties of Lunar Samples 10022, 10069, 10084, and 10085’ pp. 2213-2219.Google Scholar
Doell, R. R. and Grommé, C. S.: ‘Survey of Magnetic Properties of Apollo 11 Samples at the Lunar Receiving Laboratory’, pp. 2093-2096.Google Scholar
Doell, R. R., Grommé, C. S., Thorpe, A. N., and Senftle, F. E.: ‘Magnetic Studies of Apollo 11 Lunar Samples’, pp. 2097-2102.Google Scholar
All in Proceedings of the Apollo 11 Lunar Science Conference, Vol. 3, Physical Properties (ed. by Levinson, A. A.), Pergamon Press, 1970.Google Scholar
[22] Singer, S. F.: 1969, Trans. AGU, Natl. Fall Mtg.Google Scholar
Barnes, A., Cassen, P., Mihalov, J. D., and Eviatar, A.: ‘Permanent Lunar Surface Magnetism and Its Deflection of the Solar Wind’ (Submitted to Science).Google Scholar
Dyal, P., Parkin, C. W., Sonett, C. P., and Colburn, D. S.: ‘Electrical Conductivity and Temperature of the Lunar Interior From Magnetic Transient Response Measurements’, NASA TMX-62, 012. (Also submitted to J. Geophys. Res.).Google Scholar
Mihalov, J. H., Sonett, C. P., Binsack, J. H., and Mitsoulas, M. D.: ‘Possible Fossil Lunar Magnetism Inferred From Satellite Data’. (Science - In press).Google Scholar
Sonett, C. P., Smith, B. F., Colburn, D. S., Schubert, G., Schwartz, K., Dyal, P., and Parkin, C. W.: ‘The Lunar Electrical Conductivity Profile: Mantle-Core Stratification, Near Surface Thermal Gradient, Heat Flux, and Composition’. (Submitted to Nature).Google Scholar
Sonett, C. P., Dyal, P., Parkin, C. W., Colburn, D. S., Mihalov, J. H., and Smith, B. F.: ‘Whole Body Response of the Moon to Electromagnetic Induction by the Solar Wind’. (Science - In press).Google Scholar