Hostname: page-component-77c89778f8-vpsfw Total loading time: 0 Render date: 2024-07-20T23:08:53.548Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Production of Meteor Streams by Cometary Nuclei

Published online by Cambridge University Press:  14 August 2015

L. A. Katasev  and
N. V. Kulikova
L. A. Katasev
Affiliation:
Institute for Experimental Meteorology, Obninsk, U.S.S.R.
N. V. Kulikova
Affiliation:
Institute for Experimental Meteorology, Obninsk, U.S.S.R.

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.

An attempt is made to use Monte-Carlo techniques to model the process of formation of meteor streams. It is supposed that meteor streams are formed as the result of ejection of meteoroids from a cometary nucleus at perihelion. Possible ejection velocities are determined for the Draconids, Perseids, Leonids, and Taurids. In general the values do not exceed 100 m s-1. The data obtained can also be used to estimate the ages of the streams.

Type
Part VI/Relationship With Meteors and Minor Planets
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 498 - 502
Copyright
Copyright © Reidel 1972 

References

Astapovich, I. S.: 1968, Probl. Kosmich. Fiz. No. 3, 103.Google Scholar
Hamid, S. E.: 1950, Ph.D. dissertation, Harvard University.Google Scholar
Lovell, B.: 1954, Meteor Astronomy , Clarendon Press, Oxford.Google Scholar
Murakami, T.: 1961, Publ. Astron. Soc. Japan 13, 51, 212.Google Scholar
Neumann, J.: 1951, Natl. Bur. Sci. Appl. Math. Sci. 12, 36.Google Scholar
Orlov, S. V.: 1960, O Prirode Komet , Akad. Nauk SSSR.Google Scholar
Plavec, M.: 1955, Bull. Astron. Inst. Czech. 6, 20.Google Scholar
Southworth, R. B.: 1963, Smithsonian Contr. Astrophys. 7, 299.Google Scholar
Vsekhsvyatskij, S. K.: 1966, Fizika Komet i Meteorov , Kiev, p. 32.Google Scholar
Whipple, F. L. and Hamid, S. E.: 1952, Bull. Roy. Obs. Helwan No. 41.Google Scholar
Wright, F. W. and Whipple, F. L.: 1950, Harvard Repr. Ser. 2 No. 35.Google Scholar