Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-28T03:41:40.193Z Has data issue: false hasContentIssue false

The Stability of the Planetary Triangular Lagrange Points

Published online by Cambridge University Press:  12 April 2016

Seppo Mikkola
Affiliation:
Turku University Observatory, Turku, Finland
K.A. Innanen
Affiliation:
Physics Department, York University, Toronto, Canada

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.

Numerical, self-consistent, n-body integrations of the solar system show significant indications of medium-term (i.e. several million-year) stability for the various planet-Sun L4,L5 configurations. A progress report of our computations, emphasizing the inner solar system, will be given. There exist interesting possibilities for these locations (including the Earth) as the sites for longer term scientific applications, both pure and applied.

Type
V. Long Term Future Issues
Copyright
Copyright © Kluwer 1990

References

Innanen, K.A. and Mikkola, S.: 1989, Astron. J. 97, 900 Google Scholar
Mikkola, S. and Innanen, K.A.: 1990, Astron. J., in press (July)Google Scholar
Weissman, P.R. and Wetherill, G.W.: 1974, Astron. J. 79, 404 Google Scholar
Zhang, S-P. and Innanen, K.A.: 1988, Astron. J. 96, 1983 Google Scholar
Zhang, S-P. and Innanen, K.A.: 1988, Astron. J. 96, 1989 Google Scholar
Zhang, S-P. and Innanen, K.A.: 1988, Astron. J. 96, 1995 Google Scholar