Image:Kepler hodograph family.png

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Family of circular hodographs sharing the same total energy E for the Kepler problem of determining the motion of two particles interacting by force that varies as the inverse-square of the distance between them. In the sense taken here, hodographs are plots of the path of the momentum vector over the orbit; the coordinate system is chosen so that the orbit lies in the x-y plane. Such a family is geometrically equivalent to a family of Apollonian circles or the σ isosurfaces of bipolar coordinates. The dotted circle is not a hodograph; rather, inversion in the dotted circle transforms the Keplerian hodographs into a family of straight lines passing through a common point (see Image:Kepler_hodograph_family_trasformed.png). This figure was made by me on 22 November 2006 using Xfig and is hereby released under the GFDL.

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GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation license, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled "GNU Free Documentation license".

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Historique du fichier

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Date et heureDimensionsUtilisateurCommentaire
actuel29 novembre 2006 à 01:33323×643 (12 Kio)WillowW (Revised version in which I eliminate the circle of inversion. Made by me on 28 November 2006 using Xfig and released under the GFDL.)
22 novembre 2006 à 18:48383×643 (13 Kio)WillowW (Family of circular hodographs sharing the same total energy ''E'' for the Kepler problem of determining the motion of two particles interacting by force that varies as the inverse-square of the distance between them. In the sense taken here, hodographs a)

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