Hostname: page-component-5cf477f64f-zrtmk Total loading time: 0 Render date: 2025-04-04T14:48:06.679Z Has data issue: false hasContentIssue false
  • English
  • Français

Recent Progress in the Theory of Trojan Asteroids

Published online by Cambridge University Press:  14 August 2015

Boris Garfinkel
Boris Garfinkel*
Affiliation:
Yale University Observatory New Haven, Connecticut, U.S.A.

Extract

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.

In order to provide the necessary background for this report, this section summarizes the previously published “Theory of the Trojan Asteroids, Part I”. Treating the system as the case of 1:1 resonance in the restricted problem of three bodies, the author constructs a formal long-periodic solution of 0(m), where m is the mass-parameter of the system, assumed to be sufficiently small.

Type
Part V: Minor Planets
Information
Symposium - International Astronomical Union , Volume 81: Dynamics of the Solar System , 1979 , pp. 251 - 256
Copyright
Copyright © Reidel 1979 

References

1. Deprit, A. and Delie, A., 1965, Icarus 4, 242.Google Scholar
2. Deprit, A., Henrard, J., and Rom, A., 1967, Icarus 6, 381.Google Scholar
3. Deprit, A. and Henrard, J. 1970, “Periodic Orbits, Stability and Resonance”, Ed. Giacaglia, G.E.O., p.1 (Reidel).CrossRefGoogle Scholar
4. Garfinkel, B. 1976, Cel. Mech. 13, 229.Google Scholar
5. Garfinkel, B. 1977, Astron. Jr. 82, 368.CrossRefGoogle Scholar
6. Hagihara, Y. 1944, Japanese Jr. Astron. Geophys. 21, 29.Google Scholar
7. Hagihara, Y. 1972, “Celestial Mechanics” Vol. II, 299–307 (MIT Press).Google Scholar
8. Hori, G. 1966, Publ. Astron. Soc. Japan, 18, 287.Google Scholar
9. Szebehely, V. 1967, “Theory of Orbits”, 250 (Academic Press).Google Scholar