Abstract
Curvilinear coordinates in three dimensions associated with the Roche model distorted by centrifugal force alone constitute a Lamé family, of which one (ξ-) coordinate can be defined by equipotential surfaces which are known in closed algebraic form; the other (η) becomes identical with the meridional planes of the rotationally distorted Roche model; while the third (ζ) then follows from the requirements of orthogonality to the others. The explicit form of such coordinates in terms of the polar or cartesian systems has already been established by the author (Kopal, 1970) correctly to quantities of the first order in superficial distortion of the respective Roche model. In the present paper this latter restriction on accuracy will be removed, and expressions constructed for the ζ-coordinate in the form of infinite series which are exact and converge rapidly for any distortion below that which entails equatorial break-up.
Similar content being viewed by others
References
Darboux, G.: 1910,Leçons sur les systèmes orthogonaux et les coordonnées curvilignes, Gauthier-Villars. Paris, Chapter II.
Kopal, Z.: 1970,Astrophys. Space Sci. 8, 149–171.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kopal, Z. The Roche coordinates for the rotational problem. Astrophys Space Sci 10, 328–331 (1971). https://doi.org/10.1007/BF00704090
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00704090