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The past and future of 1983 TB and its relationship to the geminid meteor stream

Published online by Cambridge University Press:  12 April 2016

Ken Fox
Affiliation:
Theoretical Astronomy Unit, School of Mathematical Sciences, Queen Mary College, Mile End Road, London. El 4NS, U.K.
Iwan P. Williams
Affiliation:
Theoretical Astronomy Unit, School of Mathematical Sciences, Queen Mary College, Mile End Road, London. El 4NS, U.K.
J. Hunt
Affiliation:
Theoretical Astronomy Unit, School of Mathematical Sciences, Queen Mary College, Mile End Road, London. El 4NS, U.K.

Abstract

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It is now well known that object 1983 TB, discovered by IRAS, has an orbit very similar to that of the Geminid meteor stream. Calculations show that this orbit crossed over the orbit of Venus about 500 years ago. We will describe calculations tracing the history of both the object and the stream through this interaction with Venus and the present interaction with the Earth.

Type
Section III. Meteor Streams and Interrelations with Minor Planets
Copyright
Copyright © Cambridge University Press 1985

References

Babadzhanov, P.B. and Obrubov, Y.V.: 1980, in ‘Solid Particles in the Solar System’, p. 157, ed. Halliday, I. and McIntosch, B.A., D. Reidel.Google Scholar
Dormand, J.R. and Prince, P.J.: 1978, Celest. Mech., 18, 223.CrossRefGoogle Scholar
Fox, K.: 1984, Celest. Mech., 33, 127.CrossRefGoogle Scholar
Fox, K., Williams, I.P. and Hughes, D.W.: 1982, Mon. Not. R. astr. Soc., 200, 313.Google Scholar
Fox, K., Williams, I.P. and Hughes, D.W: 1983, Mon. Not. R. astr. Soc., 205, 1155.Google Scholar
Fox, K., Williams, I.P. and Hughes, D.W.: 1984, Mon. Not. R. astr. Soc., 208, Short Communication, 11P.Google Scholar
Jacchia, L.G. and Whipple, F.L.: 1961, Smithson. Contrib. Astrophys., 4, 97.Google Scholar
Spalding, G.H.: 1984, J. Brit. astron. Assoc., 94, 3.Google Scholar
Weissman, P.R.: 1979, Astr. J., 84, 580.Google Scholar