Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-30T02:39:55.730Z Has data issue: false hasContentIssue false
  • English
  • Français

From Interstellar Dust to Comets to the Zodiacal Light

Published online by Cambridge University Press:  14 August 2015

J. M. Greenberg
J. M. Greenberg*
Affiliation:
Laboratory Astrophysics, Leiden University, Leiden, Holland

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.

We consider the consequences of the assumption that the interplanetary particles which produce the zodiacal light have evolved from interstellar dust via comets. The chemical evolution of interstellar dust followed by the process of aggregation into the cometary nucleus and the subsequent ejection of cometary debris provide the basis for a model for the interplanetary particles. The scattering properties of these particles are reasonably consistent with current observations of the variation with elongation angle of the brightness and polarization of the zodiacal light. The major chemical constituents of the model are in the form of a matrix of volatile ices and complex nonvolatile molecules containing C, N and O in which are imbedded silicate and metallic inclusions.

Type
IV: The Interplanetary Dust Complex 2. Physical Properties
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 343 - 350
Copyright
Copyright © Reidel 1980 

References

Allamandola, L.J., Greenberg, J.M., and Norman, C.A.: 1979a, Astron. Astrophys. 77, pp. 66.Google Scholar
Allamandola, L.J., Greenberg, J.M., and Norman, C.A.: 1979b, Proc. IAU Symposium no. 87, ed. Andrew, B., Reidel.Google Scholar
Bierman, L., and Michel, K.W.: 1978, The Moon and the Planets 18, pp. 447.CrossRefGoogle Scholar
Brownlee, D.E.: 1978, Chapter 5 in Cosmic Dust, ed. McDonnell, J.A.M., J. Wiley Publ., pp. 295.Google Scholar
Cameron, A.G.W.: 1973, Icarus 18, pp. 407.CrossRefGoogle Scholar
Donn, B.: 1963, Icarus 2, pp. 396.Google Scholar
Fechtig, H.: 1976, in Interplanetary Dust and Zodiacal Light (Elsässer, H. and Fechtig, H., eds.), Springer-Verlag, Heidelberg, pp. 143.Google Scholar
Giese, R.H., and Grün, E.: 1976, in Interplanetary Dust and Zodiacal Light (Elsässer, H. and Fechtig, H., eds.), Springer-Verlag, Heidelberg, pp. 135.CrossRefGoogle Scholar
Giese, R.H., Weiss, R., Zerull, R.H., and Ono, T.: 1978, Astron. Astrophys. 65, pp. 265.Google Scholar
Goldreich, P., and Ward, W.R.: 1973, Astrophys. J. 183, pp. 1051.Google Scholar
Greenberg, J.M.: 1974a, Astrophys. J. 189, pp. L81.Google Scholar
Greenberg, J.M.: 1974b, in Planets, Stars and Nebulae Studied with Photopolarimetry (ed. Gehrels, T.), The Univ. of Arizona Press, pp. 107.Google Scholar
Greenberg, J.M.: 1977, Comets, Asteroids, Meteorites, ed. Delsemme, A.H. (Univ. of Toledo) pp. 491.Google Scholar
Greenberg, J.M.: 1978, Chapter 4 in Cosmic Dust, ed. McDonnell, J.A.M., J. Wiley Publ., pp. 187.Google Scholar
Greenberg, J.M.: 1979a, in Stars and Stars Systems, ed. Westerlund, B.E., D. Reidel, pp. 173.CrossRefGoogle Scholar
Greenberg, J.M.: 1979b, The Moon and the Planets 20, pp. 15.Google Scholar
Greenberg, J.M., and Gustafson, B.A.S.: 1978, preprint.Google Scholar
Hagen, W., Allamandola, L.J., and Greenberg, J.M.: 1979, Astrophys. Spaces Sci. 65, pp. 215.CrossRefGoogle Scholar
Lanzerotti, L.J., Brown, W.L., Poate, J.M., and Augustyniak, W.M.: 1979, Nature 272, pp. 431.CrossRefGoogle Scholar
Lewis, J.S.: 1971, Icarus 15, pp. 174.Google Scholar
Oort, J.H.: 1950, Bull.Ast.Inst.Ned. 11, pp. 91.Google Scholar
Safronov, V.S.: 1972, in Evolution of the Protoplanetary Cloud and the Formation of the Earth and the Planets, Israel Program for Scientific Translations, Jerusalem.Google Scholar
Le Sergeant, L.B., and Lamy, Ph.L.: 1978, Nature 276, pp. 800.CrossRefGoogle Scholar
Weinberg, J., and Sparrow, J.G.: 1978, Review of Zodiacal Light in “Cosmic Dust” (ed. McDonnell, J.A.M.), J. Wiley Publ., pp. 75.Google Scholar