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Evolution of Orbits and Intersection Conditions with the Earth of the Geminid and Quadrantid Meteor Streams

Published online by Cambridge University Press:  14 August 2015

P. B. Babadzhanov
Affiliation:
Astrophysical Institute, Dushanbe, USSR
Yu.V. Obrubov
Affiliation:
Astrophysical Institute, Dushanbe, USSR

Extract

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The Geminids and Quadrantids belong to the most active annual meteor showers. The distinct difference between the orbit sizes of large and small meteoroids in these streams has been shown. From this, the estimated age of the streams greatly exceeds the time since their discovery in the XIX century (Geminids in 1862, Quadrantids in 1830) (Lovell 1954, Hindley 1972).

Type
II: Meteors and Meteorites
Copyright
Copyright © Reidel 1980 

References

Cook, A.F.: 1973, NASA SP – 319, 183.Google Scholar
Dobrovolsky, O.V., Jegibekov, P., Zausaev, A.F.: 1973, Sov. Astron. J., 50, 832.Google Scholar
Gorjachev, N.N.: 1937, Halphen's method of calculation of secular perturbations and its application to Cerere, Tomsk.Google Scholar
Hajduk, A., McIntosh, B.A., Simek, M.: 1974, Bull. Astron. Inst. Czech. 25, 305.Google Scholar
Hindley, K.B.: 1972, Sky and Telescope 43, 162.Google Scholar
Huebner, W.F.: 1970, Astron. and Astrophys. 5, 286.Google Scholar
Imoto, S., Hasegawa, I.: 1958, Smith. Contr. Astrophys. 2, 131.Google Scholar
Jones, J.: 1978, Mon. Not. Roy. Astron. Soc. 183, 539.CrossRefGoogle Scholar
Lovell, A.C.B.: 1954, Meteor Astronomy, Clarendon Press, Oxford.Google Scholar
Whipple, F.L.: 1955, Astrophys. J. 121, 750.CrossRefGoogle Scholar
Whipple, F.L. and Wright, F.W.: 1954, Mon. Not. Roy. Astron. Soc. 114, 229.Google Scholar