Skip to main content
Log in

On the integrability of the Roche coordinates

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

The aim of the present paper is to prove that the system of partial differential equations, which define a set of curvilinear coordinates ξ, η, ζ that are orthogonal to the Roche equipotentials ξ(r, θ, ϕ) incorporating the effects of both rotationaland tidal distortion, does not admit of any formal integrals; and can be solved only numerically in an asymptotic manner. This fact is related with analytic properties of the problem of three bodies, in which ξ represents the potential.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Charlier, C. V. L.: 1902,Die Mechanik des Himmels, Viet und Co., Leipzig, Vol.II, Chapter 8.

    Google Scholar 

  • Darboux, G.: 1910,Leçons sur les systèmes orthogonaux et les coordonnées curviliques, Gauthier-Villars, Paris, Sections 9–12.

    Google Scholar 

  • Kitamura, M.: 1970,Astrophys. Space Sci. 7, 272–358.

    Google Scholar 

  • Kopal, Z.: 1970,Astrophys. Space Sci. 8, 149–171.

    Google Scholar 

  • Kopal, Z.: 1971,Astrophys. Space Sci. 10, 328–331.

    Google Scholar 

  • Poincaré, H.: 1892,Méthodes nouvelles de la mécanique céleste, Gauthier-Villars, Paris, Vol.I, Chapter V.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Kopal, Z., Sekender Ali, A.K.M. On the integrability of the Roche coordinates. Astrophys Space Sci 11, 423–429 (1971). https://doi.org/10.1007/BF00649635

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00649635

Keywords

Navigation