Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-19T03:27:11.782Z Has data issue: false hasContentIssue false

The Quadrantid Stream, Chaos or Not?

Published online by Cambridge University Press:  07 August 2017

Zidian Wu
Affiliation:
Astronomy Unit, Queen Mary & Westfield College, Mile End Rd, London E1 4NS
Iwan P Williams
Affiliation:
Astronomy Unit, Queen Mary & Westfield College, Mile End Rd, London E1 4NS

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.

The Quadrantid stream covers a region of space which contains many strong resonances and commensurabilities with the Jovian orbit. We have numerically integrated the orbital evolution of over one hundred actual meteoroids backwards to BC 5000. The evolution is quit complex, but most of the meteoroids are quite well behaved with rapid but smooth changes in the orbital elements. One meteoroid however shows sharp sudden changes in its orbital parameters and these changes are generally indicative of the presence of chaos.

Type
Part VI - Meteors. Zodiacal Cloud. Nebulae
Copyright
Copyright © Kluwer 1992 

References

Dormand, J.R. El-Mikkai, M.E.A. and Prince, P.J. (1987) J. Numer. Anal. , 7, 423.Google Scholar
Drummond, J.D., (1981) Icarus , 45, 545.CrossRefGoogle Scholar
Froeschlé, Cl. and Scholl, H., (1981) Astron. Astroph. , 93, 62.Google Scholar
Hughes, D.W, Williams, I.P. and Fox, K. (1981) Mon. Not. R. astr. Soc. , 195, 625.CrossRefGoogle Scholar
Murray, C.D. Hughes, D.W. and Williams, I.P.(1979) Mon. Not. R. astr. Soc. , 190, 733.Google Scholar
Williams, I.P., Murray, C.D. and Hughes, D.W.(1979) Mon. Not. R. astr. Soc. , 189, 483.Google Scholar