Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-20T13:06:43.681Z Has data issue: false hasContentIssue false
  • English
  • Français

Capture of the Comet P/Boethin by Jupiter

Published online by Cambridge University Press:  12 April 2016

Benest Daniel ,
Bien Reinhold  and
Rickman Hans
Benest Daniel
Affiliation:
Observatoire de Nice, France
Bien Reinhold
Affiliation:
Astronomisches Rechen InstitutHeidelberg, Fed. Rep. Germany
Rickman Hans
Affiliation:
Astronomiska Observatoriet, Uppsala, Sweden

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 possible effects of non-gravitationnal forces on the motion of the comet P/Boethin are investigated for various values of the orbital period. A time interval of 2000 years backward and forward is treated. The authors find in all cases that the comet librates temporarily around the 1/1 resonance with Jupiter as a remote jovian satellite during at least two centuries.

Type
Part II - Comets and Meteor Streams
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 107 - 114
Copyright
Copyright © Reidel 1983

References

Benest, D., Bien, R., Rickman, H.: 1980, Astron. Astrophys. 84, pp.L11–L12.Google Scholar
Benest, D., Bien, R., Rickman, H.: 1981, Astr. Ges. Mitt. 52, pp.27–28.Google Scholar
Benest, D., Bien, R., Rickman, H.: 1982, in “Sun and Planetary System”,eds. Fricke, W. and Teleki, G. Reidel pp.397–400. Google Scholar
Marsden, B.G.: 1974, Ann. Rev. Astron. Astrophys. 12, pp.1–21.Google Scholar
Marsden, B.G.: 1979, “Catalogue of Cemetery Orbits”, third edition, I.A.U. Central Bureau for Astronomical Telegrams, Cambridge (Mass.).Google Scholar