2003
DOI: 10.1119/1.1561272
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Tracing a planet’s orbit with a straight edge and a compass with the help of the hodograph and the Hamilton vector

Abstract: We describe a geometrical method for tracing a planet's orbit using its velocity hodograph, that is, the path of the planet's velocity. The method requires only a straight edge, a compass, and the help of the hodograph. We also obtain analitically the hodograph and some of the features of the motion that can be obtained from it.

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Cited by 4 publications
(5 citation statements)
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References 14 publications
(18 reference statements)
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“…He found a replica of vector e with different interesting properties (see [2]). This result was found again identically by various authors 35 years after (see [6], [9]- [11], [17]- [19]). This vector e can be computed only from the initial conditions and gives a complete overview to the entire motion, containing all the informations about it.…”
Section: Discussionsupporting
confidence: 88%
See 1 more Smart Citation
“…He found a replica of vector e with different interesting properties (see [2]). This result was found again identically by various authors 35 years after (see [6], [9]- [11], [17]- [19]). This vector e can be computed only from the initial conditions and gives a complete overview to the entire motion, containing all the informations about it.…”
Section: Discussionsupporting
confidence: 88%
“…Using complex numbers, professor A. Braier found in 1965 a replica of vector e with specific consequences (see [1,2,3]). He deduced a vectorial eccentricity (see [1]) that was again discovered by various authors in the same way between 1996-2004 (see [6], [9]- [11], [17]- [19]).…”
Section: Kepler's Problem: a Vectorial Solutionmentioning
confidence: 89%
“…It reflects a special property-often referred to as a dynamical symmetry-of a radial inverse-square-law force within the context of non-relativistic mechanics and allows for a rather straightforward derivation of the orbit of a particle moving under the influence of such a force. An alternative [6][7][8] is to use the Hamilton vector, a quantity related in a simple manner to the Laplace-Runge-Lenz vector whose conservation was first discovered by W R Hamilton in 1845 [9].…”
Section: Introductionmentioning
confidence: 99%
“…Given the remarkable efficiency introduced by the Hamilton vector into the derivation of the orbit of the particle [6][7][8], it is only natural to ask whether the relativistic problem might not also benefit from a similar development. At first sight, the answer seems rather trivially no, since special-relativistic effects break the degeneracy that ensures conservation of the Hamilton and Laplace-Runge-Lenz vectors.…”
Section: Introductionmentioning
confidence: 99%
“…A completely different way of tracing all three kinds of orbits with the help of hodographs has been successfully developed by Salas-Brito and co-workers in a series of publications culminating in Ref. 10.…”
mentioning
confidence: 99%