Realizing Keplerian orbits as geodesics on a surface of revolution

dc.contributor.advisorSmith, Alex
dc.contributor.authorBarrette, Brandon
dc.date.accessioned2008-02-04T21:04:42Z
dc.date.available2008-02-04T21:04:42Z
dc.date.issued2007-05-01T21:04:42Z
dc.descriptionColor poster with text and graphs describing research conducted by Brandon Barrette advised by Alex Smith.en
dc.description.abstractIt is well known that in Newtonian physics, the gravitational trajectories in a central gravitational field are conic sections with one focus at the central mass. This is known as Kepler's First Law. We consider those gravitational trajectories that lie in a fixed plane P (perhaps thought of as an ecliptic plane), and investigate this question: to what extent can P be embedded as a surface of revolution S inside an abstract three-dimensional Euclidean space E in such a way that gravitational trajectories are mapped to geodesics on S, subset of E?en
dc.description.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programs.en
dc.format.extent374777 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.urihttp://digital.library.wisc.edu/1793/23192
dc.language.isoen_USen
dc.relation.ispartofseriesUSGZE AS589en
dc.subjectKepler's lawsen
dc.subjectOrbitsen
dc.subjectGravitationen
dc.subjectPostersen
dc.titleRealizing Keplerian orbits as geodesics on a surface of revolutionen
dc.typePresentationen

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