Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-18T06:36:26.097Z Has data issue: false hasContentIssue false
  • English
  • Français

3. Pre-Main Sequence Heating of Planetoids

Published online by Cambridge University Press:  12 April 2016

C. P. Sonett  and
F. L. Herbert

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The problem of thermal metamorphosis of meteorites, possibly the Moon and Mercury, and perhaps other planetary objects is reviewed. Classical mechanisms of heating include fossil nuclides (especially 26Al), accretional heating, tidal heating, chemical reaction heat, and electrical induction. These various mechanisms involve constraints on the early thermal profiles of the Moon or Mercury. In the case of the meteorites, the primary contenders for a viable mechanism currently are fossil nuclides and electromaqnetic induction, or some combination of these. But the issue of energetic mechanisms in the early solar system remains enigmatic. The fossil nuclide hypothesis leads to constraints upon nucleosynthesis while electromagnetic induction places significant constraints upon electrodynamic effects such as solar spin damping.

Type
Part VII. Differentiated Meteorites
Information
International Astronomical Union Colloquium , Volume 39: Comets, Asteroids, Meteorites: Interrelations, Evolution and Origins , December 1977 , pp. 429 - 437
Copyright
Copyright © A.H. Delsemme 1977

References

Alexander, E. C., Lewis, R. S., and Reynolds, J. H. 1971, Science, 172, 837.Google Scholar
Alfven, H. 1954, The Origin of the Solar System, Oxford Press.Google Scholar
Bainbridge, J. J. 1962, Ap.J., 136, 202.Google Scholar
Brecher, A. 1972, in Proc. Symp. Origin of the Solar System, CNRS, p. 270.Google Scholar
Briggs, P. L. 1976, M.S. Thesis, preprint, MIT Cambridge, Massachusetts.Google Scholar
Brown, H. 1974, Phys. Rev. 72, 348.CrossRefGoogle Scholar
Butler, R. F. 1972, Earth and Planet. Sci. Letts., 17, 120.CrossRefGoogle Scholar
Cameron, A.G.W. 1973, Icarus, 18, 407.Google Scholar
Essene, E. J., Ringwood, A. E., and Ware, N. G. 1970, Proc. Apollo ll Sci. Conf., 1, 385.Google Scholar
Fish, R. A., Goles, G. G., and Anders, E. 1960, Astrophys. J., 132, 243.CrossRefGoogle Scholar
Fleischer, R. L., Price, P. B., and Walker, R. M. 1965, J. Geophys. Res., 70, 2703.CrossRefGoogle Scholar
Goldstein, J. I., and Ogilvie, R. E. 1965, Geochim. Cosmochim. Acta, 29, p. 893.Google Scholar
Goldstein, B. E., Phillips, R. J., Russell, C. T., and Tsay, F. D. 1976, submitted to Proc. Seventh Lun. Sci. Conf., in press.Google Scholar
Hayashi, C., and Nakano, T. 1965, Prog. Theor. Phys., 34, 754.Google Scholar
Herbert, F., Sonett, C. P., and Wiskerchen, M. J. (1976a), submitted to J. Geophys. Res.Google Scholar
Herbert, F., Wiskerchen, M. J., Sonett, C. P., and Chao, J. K. 1976, Icarus, 28, 489.Google Scholar
Herbig, G. H. 1970, Mem. Soc. Roy. Sci. Liege, 19, 13.Google Scholar
Hoyle, F. 1960, Q.J.R.A.S., 1, 28.Google Scholar
Kaula, W. M. 1963, J. Geophys. Res., 68, 4945.Google Scholar
Kraft, R. P. 1967, Ap.J., 150, 551.Google Scholar
Kraft, R. P. 1972, in Solar Wind, ed. Sonett, C. P., Wilcox, J. M. and Coleman, P. J. Jr., NASA SP-308, p. 276.Google Scholar
Kuhi, I. V. 1964, Ap.J., 140, 1409.Google Scholar
Larson, R. B. 1973, Fund, of Cosmic Phys., 1, 1.Google Scholar
Lee, T., Papanastassiou, D. A., and Wasserburg, G. J. 1976, Geophys. Res. Lett., 3, 109.Google Scholar
McCrea, W. H. 1973, Q.J.R.A.S., 4, 192.Google Scholar
Murray, B. C., Belton, M.J.S., Danielson, G. E., Davis, M. E., Gault, D. E., Hapke, B., O’Leary, B., Strom, R. G., Suomi, V., and Trask, N. 1974, Science, 185, 169.Google Scholar
Nakamura, Y., Lammlein, D., Latham, G., Ewing, M., Dorman, J., Press, F., and Toksoz, N. 1973, Science, 181, 49.Google Scholar
Ostriker, J. P. 1964, Ap.J., 140, 1056.CrossRefGoogle Scholar
Pochtarev, V. I., Guskove, Ye. G. 1962, Geomag. and Aeronomy, 2, 626.Google Scholar
Reeves, H., and Audouze, J. 1968, Earth and Planet. Sci. Lett., 4, 135.Google Scholar
Reynolds, J. A. 1960, Phys. Rev. Lett., 4, 8.CrossRefGoogle Scholar
Safronov, V. S. 1972, Evolution of the Protoplanetary Cloud and Formation of the Earth and the Planets, NASA TT F-677.Google Scholar
Siegfried, R. W., and Solomon, S. C. 1974, Icarus, 23, 192.Google Scholar
Sonett, C. P. 1971, in Physical Studies of Minor Planets, ed. Gehrels, T., NASA SP-267, p. 239.Google Scholar
Sonett, C. P. 1974, in Solar Wind Three, ed. Sonett, C. P., Wilcox, J. M., and Coleman, P. J. Jr., NASA SP-308.Google Scholar
Sonett, C. P., and Colburn, D. S. 1970, The Moon, 1, 483.Google Scholar
Sonett, C. P., Colburn, D. S., and Schwartz, K. 1968, Nature, 219, 924.Google Scholar
Sonett, C. P., Smith, B. F., Colburn, D. S., Schubert, G., and Schwartz, K. 1972, in Proc. Third Lunar Sci. Conf., 3, 2309 (Geochim. Cosmochim. Acta, Suppl. 3).Google Scholar
Srnka, L. J. 1976, J. Geophys. Res., 31, 2015.Google Scholar
Stacey, F. D., Lovering, J. F., and Parry, L. G. 1961, J. Geophys. Res., 66, 1523.Google Scholar
Struve, 0. 1930, Ap.J., 72, 1.CrossRefGoogle Scholar
THksoz, M. N., Solomon, S. C., Minear, J. W., and Johnson, D. H. 1972, The Moon, 4, 190.Google Scholar
Urey, H. C. 1961, in The Moon, ed. Kopal, Z., IAU Symp. 14, Academic Press, p. 133.Google Scholar
Urey, H. C., and Donn, B. 1956, Ap.J., 124, 307.Google Scholar
Wasson, J. T. 1974, Meteorites, Springer-Verlag.Google Scholar
Weaving, B. 1962, Geophys. J., 7, 203.Google Scholar
Wetherill, G. W. 1975, in Papers Presented to the Conf. on Origins of Mare Basalts and their Implications for Lunar Evolution, Lunar Sci., Inst., Houston, p. 184.Google Scholar
Wetherill, G. W. 1976, in Lunar Science VII, part II, p. 930.Google Scholar
Wiskerchen, M. J., Parker, G. D., Sonett, C. P., Schubert, G., and Schwartz, K. 1976, in Lunar Science VII, part II, p. 944.Google Scholar
Wood, J. A. 1968, Meteorites and the Origin of Planets, McGraw-Hill.Google Scholar
Wood, J. A. 1972 Icarus, 16, 229.Google Scholar
Wood, J. A., Dickey, J. S., Marvin, U. B., and Powell, B. N. 1970, Science, 167, 602.Google Scholar
Wones, D. R., and Shaw, H. R. 1975, Tidal dissipation: a possible heat source for mare basalt magmas, in Lunar Science VI, part II, Lunar Sci. Inst., Houston, p. 878.Google Scholar