Conic Section Trajectories
Conic Section Trajectories is a mathematical model in celestial mechanics that describes the possible paths of two bodies under mutual gravitational attraction as conic sections—ellipses, parabolas, or hyperbolas—distinguished by their orbital energy and eccentricity.
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Publications
1.2K
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33
Authors
27
Institutions
Publications per year
2017–2026
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1 publications · 116 citations
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University of Colorado Boulder
Boulder, United States
2 h-index
3 publications
53 citations
Oberlin College
Oberlin, United States
1 h-index
1 publications
27 citations

Centre National de la Recherche Scientifique
Paris, France
1 h-index
1 publications
18 citations
Wayne State University
Detroit, United States
1 h-index
1 publications
27 citations
Centre for Alternative Technology
Newtown, United Kingdom
1 h-index
1 publications
106 citations
Microsoft (United States)
Redmond, United States
1 h-index
1 publications
193 citations
Rensselaer Polytechnic Institute
Troy, United States
1 h-index
1 publications
13 citations
The University of Texas at Austin
Austin, United States
1 h-index
1 publications
48 citations
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2 publications · 40 citations
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2 publications · 41 citations
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2 publications · 65 citations
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1 publications · 18 citations
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1 publications · 27 citations
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