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About: Newton's theorem of revolving orbits     Goto   Sponge   NotDistinct   Permalink

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Type: yago:WikicatConceptsInPhysicsyago:WikicatTheoremsyago:Abstraction100002137yago:Cognition100023271yago:Communication100033020yago:Concept105835747yago:Content105809192yago:Idea105833840yago:Message106598915yago:Proposition106750804yago:PsychologicalFeature100023100yago:Statement106722453yago:Theorem106752293 New Facet based on Instances of this Class

In classical mechanics, Newton's theorem of revolving orbits identifies the type of central force needed to multiply the angular speed of a particle by a factor k without affecting its radial motion (Figures 1 and 2). Newton applied his theorem to understanding the overall rotation of orbits (apsidal precession, Figure 3) that is observed for the Moon and planets. The term "radial motion" signifies the motion towards or away from the center of force, whereas the angular motion is perpendicular to the radial motion.