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Sources of Interplanetary Dust

Published online by Cambridge University Press:  14 August 2015

Ľubor Kresák
Ľubor Kresák*
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Bratislava, Czechoslovakia

Abstract

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It is generally assumed that ejections from active cometary nuclei are the major source of replenishment of the interplanetary dust complex. Conjectures against this concept are usually based on comparison of the quantitative efficiency of the dust production by comets with the efficiency of all the dissipative processes involved. The present paper discusses this problem from the dynamical point of view, tracing the evolution of swarms of cometary ejecta as they pass through different evolutionary stages. It is concluded that the contribution of the present population of active comets, of all revolution periods, is not only inadequate to explain the abundance of interplanetary particles, but also inconsistent with the distribution of their orbits. Other potential sources and their implications for the equilibrium problem are reviewed.

Type
III: The Interplanetary Dust Complex 1. Sources, Evolution, and Dynamics
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 211 - 222
Copyright
Copyright © Reidel 1980 

References

Chapman, C.R.: 1979, in Gehrels, T. (ed.), “Asteroids”, Univ.Ariz.Tucson, (in press).Google Scholar
Davies, J.G. and Gill, J.C.: 1960, Mon.Not.Roy.Astron.Soc. 121, pp.437–462.CrossRefGoogle Scholar
Delsemme, A.H.: 1976, Lecture Notes in Phys. 48, pp.314–318 and 481–484.Google Scholar
Dohnanyi, J.S.: 1976, Lecture Notes in Phys. 48, pp.187–205.Google Scholar
Everhart, E.: 1972, Astrophys.Lett. 10, pp.131–135.Google Scholar
Fechtig, H., Grün, E., Morfill, C.: 1979, Planet.Space Sci. 27, pp.511–531.Google Scholar
Galibina, I.V.: 1979, “Secular Perturbations of Minor Meteor Streams”, Moscow.Google Scholar
Giese, R.H., Weiss, K., Zerull, R.H., Ono, T.: 1978, Astron.Astrophys. 65, pp.265–272.Google Scholar
Hughes, D.W., Williams, I.P., Murray, C.D.: 1979, Mon.Not.Roy.Astron.Soc., (in press).Google Scholar
Humes, D.H.: 1976, in Gehrels, T. (ed.), “Jupiter”, Univ.Ariz.Tucson, pp.1052–1067.Google Scholar
Imoto, S. and Hasegawa, I.: 1958, Smithson.Contr.Astrophys. 2, pp. 131–144.Google Scholar
Jacchia, L.G., Verniani, F., Briggs, R.E.: 1967, Smithson.Contr.Astroph. 10, pp.1–139.CrossRefGoogle Scholar
Kashcheev, B.L. and Lebedinets, V.N.: 1967, NASA SP-150, pp.189–199.Google Scholar
Kashcheev, B.L., Lebedinets, V.N., Lagutin, M.F.: 1967, IGP Results, Ser.Meteors 2.Google Scholar
Kresák, L.: 1964, Bull.Astron.Inst.Czechosl. 15, pp.190–201.Google Scholar
Kresák, L.: 1976, Bull.Astron. Inst.Czechosl. 27, pp.35–46.Google Scholar
Kresák, L.: 1977, Bull.Astron.Inst.Czechosl. 28, pp.65–82.Google Scholar
Kresák, L.: 1978, Bull.Astron.Inst.Czechosl. 29, pp.114–125 and 135–149.Google Scholar
Kresák, L.: 1979, in Gehrels, T. (ed.), “Asteroids”, Univ.Ariz.Tucson, (in press).Google Scholar
LeSergeant, L.B. and Lamy, P.L.: 1978, Nature 276, pp.800–802.Google Scholar
Marsden, B.G.: 1973, Astron.J. 78, pp.654–662.Google Scholar
Marsden, B.G. and Sekanina, Z.: 1971, Astron.J. 76, pp.1135–1151.CrossRefGoogle Scholar
McCrosky, R.E. and Posen, A.: 1961, Smithson.Contr.Astrophys. 4, pp.15–84.Google Scholar
McIntosh, B.A.: 1973, NASA SP-319, pp.193–198.Google Scholar
Millman, P.M.: 1979, Naturwissenschaften 66, pp.134–139.Google Scholar
Millman, P.M. and McIntosh, B.A.: 1966, Canad.J.Phys. 44, pp.1593–1602.CrossRefGoogle Scholar
Oikawa, S. and Everhart, E.: 1979, Astron.J. 84, pp.134–139.CrossRefGoogle Scholar
Öpik, E.J.: 1973, Astrophys.Space Sci. 21, pp.307–398.Google Scholar
Paddack, S.J. and Rhee, J.W.: 1976, Lecture Notes in Phys. 48, pp.453–457.Google Scholar
Röser, S.: 1976, Lecture Notes in Phys. 48, pp.319–322.CrossRefGoogle Scholar
Sekanina, Z.: 1972, IAU Symposium 45, pp.301–307.Google Scholar
Sekanina, Z.: 1973, Icarus 18, pp.253–284.CrossRefGoogle Scholar
Stohl, J.: 1969, Contr.Astron.Obs.Skalnaté Pleso 4, pp.46–62.Google Scholar
Whipple, F.L.: 1951, Astrophys.J. 113, pp.464–474.CrossRefGoogle Scholar
Whipple, F.L.: 1967, NASA SP-150, pp.409–426.Google Scholar