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  2. Newton's theorem of revolving orbits - Wikipedia

    en.wikipedia.org/wiki/Newton's_theorem_of...

    Newton's theorem of revolving orbits was his first attempt to understand apsidal precession quantitatively. According to this theorem, the addition of a particular type of central force—the inverse-cube force—can produce a rotating orbit; the angular speed is multiplied by a factor k , whereas the radial motion is left unchanged.

  3. De motu corporum in gyrum - Wikipedia

    en.wikipedia.org/wiki/De_motu_corporum_in_gyrum

    Newton's style of demonstration in all his writings was rather brief in places; he appeared to assume that certain steps would be found self-evident or obvious. In 'De Motu', as in the first edition of the Principia , Newton did not specifically state a basis for extending the proofs to the converse.

  4. Circular orbit - Wikipedia

    en.wikipedia.org/wiki/Circular_orbit

    At the top of the diagram, a satellite in a clockwise circular orbit (yellow spot) launches objects of negligible mass: (1 - blue) towards Earth, (2 - red) away from Earth, (3 - grey) in the direction of travel, and (4 - black) backwards in the direction of travel. Dashed ellipses are orbits relative to Earth.

  5. File:Newton revolving orbit diagram.svg - Wikipedia

    en.wikipedia.org/wiki/File:Newton_revolving...

    English: Diagram illustrating Newton's derivation of his theorem of revolving orbits. Date: 23 August 2008: Source: Own work: ... Newton's theorem of revolving orbits;

  6. File:Newton revolving orbit e0.6 precession.ogv - Wikipedia

    en.wikipedia.org/wiki/File:Newton_revolving...

    English: According the Newton's theorem of revolving orbits the planets revolving the Sun follow elliptical (oval) orbits that rotate gradually over time (apsidal precession). The eccentricity of this ellipse is exaggerated for visualization. Most orbits in the Solar System have a much smaller eccentricity, making them nearly circular.

  7. Orbital mechanics - Wikipedia

    en.wikipedia.org/wiki/Orbital_mechanics

    The fundamental laws of astrodynamics are Newton's law of universal gravitation and Newton's laws of motion, while the fundamental mathematical tool is differential calculus. In a Newtonian framework, the laws governing orbits and trajectories are in principle time-symmetric .

  8. Newton's theorem - Wikipedia

    en.wikipedia.org/wiki/Newton's_theorem

    Newton's theorem of revolving orbits; Newton's shell theorem This page was last edited on 28 June 2021, at 14:38 (UTC). Text is available under the Creative ...

  9. Three-body problem - Wikipedia

    en.wikipedia.org/wiki/Three-body_problem

    The circular restricted three-body problem [clarification needed] is a valid approximation of elliptical orbits found in the Solar System, [citation needed] and this can be visualized as a combination of the potentials due to the gravity of the two primary bodies along with the centrifugal effect from their rotation (Coriolis effects are ...