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Lifetime of Meteor Streams Associated with Comet Halley
Published online by Cambridge University Press: 12 April 2016
Abstract
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Critical examination of the orbital parameters of particles ejected from comet Halley rejects the low age hypotheses for meteor showers associ- ated with the comet. The diffusion of the orbits of large particles is too slow for explaining the observed structural features of the stream. The mass-loss process as derived from space observations compared with the mass of the stream of particles deduced from flux data lead to comet lifetimes of the order of 105 years.
- Type
- Meteoroids and Meteor Streams
- Information
- International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 323 - 326
- Copyright
- Copyright © Kluwer 1991
References
Carusi, A., Kresák, L., Perozzi, E., and Valsecchi, G.B. (1987). Long-term resonances and orbital evolution of Halley-type comets. 10th Europ. Reg. Astron. Meeting
2, 29–32.Google Scholar
Chirikov, B.V. and Vecheslavov, V.V. (1989). Chaotic dynamics of comet Halley. Astron. Astrophys. 221, 146–154.Google Scholar
Crifo, J.F. (1987). Are cometary dust mass loss rates deduced from optical emissions reliable? 10th Europ. Reg. Astron. Meeting
2, 59–66.Google Scholar
Hajduk, A. (1982). The total mass and structure of the meteor stream associated with comet Halley, Sun and Planetary System (eds. Fricke, W. and Teleki, G.), D. Reidel; 335–336.Google Scholar
Hajduk, A. (1985). The past orbit of comet Halley and its meteor stream. IAU Coll. No. 83, 399–404, Reidel, Dordrecht.Google Scholar
Hajduk, A. (1987). Dust production of comet Halley with account of large particles contribution. 10th Europ. Reg. Astron. Meeting
2, 177–178.Google Scholar
Hajduk, A. and Hajduková, M. (1989). From the formation of meteor streams up to their decay. Asteroids, Comets, Meteors III, Uppsala Univ., pp. 531–534.Google Scholar
Hughes, D.W. (1985). The size, mass, mass-loss and age of Halley’s comet. Mon. Not. R. Astron. Soc.
213, 103–109.Google Scholar
Hughes, D.W. (1988). Cometary magnitude distribution and the ratio between the numbers of long- and short-period comets. Icarus
73, 149–162.CrossRefGoogle Scholar
Jones, J., McIntosh, B.A. and Hawkes, R.L. (1989). Mon. Not. R. Astron. Soc.
238, 179–
CrossRefGoogle Scholar
Kozai, Y. (1979). Secular perturbations of asteroids and comets. In: Dynamic of the Solar System, IAU Symp. No.
81, 231–237, Reidel, Dordrecht..CrossRefGoogle Scholar
Kresák, L. (1985). The aging and lifetimes of comets. In: Dynamics of Comets: Their Origin and Evolution, IAU Coll. No.
83, 279–302, Reidel, Dordrecht.CrossRefGoogle Scholar
McIntosh, B.A. and Jones, J. (1988). The Halley comet meteor stream. Mon. Not. R. Astron. Soc.
235, 673–694.CrossRefGoogle Scholar
Olsson-Steel, D. (1987). The dynamical lifetime of comet P/Halley. Astron. Astrophys. 187, 909–912.Google Scholar
Whipple, F.L. (1986). The cometary nucleus: current concepts. ESA SP-250, II, 281–288.Google Scholar
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