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  2. 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.

  3. File:HD10180Orbits.svg - Wikipedia

    en.wikipedia.org/wiki/File:HD10180Orbits.svg

    Date/Time Thumbnail Dimensions User Comment; current: 16:42, 25 August 2010: 672 × 1,328 (8 KB): Icalanise: Fixed description: should say HD 10180, not Gliese 876

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Animations of the Solar System's inner planets orbiting. Each frame represents 2 days of motion. Animations of the Solar System's outer planets orbiting. This animation is 100 times faster than the inner planet animation. The planets and other large objects in orbit around the Sun lie near the plane of Earth's orbit, known as the ecliptic ...

  5. File:Comparison satellite navigation orbits.svg - Wikipedia

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

    To see the animation, open media:Comparison satellite navigation orbits.svg. It should run in any modern browser or viewer. Recent versions of Chrome, Firefox, Microsoft Edge, Safari, and Opera all support SVG animated with SMIL. Other SVG animations can be found at Category:Animated SVG files.

  6. File:ThePlanets Orbits Mercury PolarView.svg - Wikipedia

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

    Orbits Mercury in yellow; For reference a circular orbit with the same semi-major axis in grey; The orbit plotted in brighter colours above the ecliptic and darker below. Major axis drawn showing perihelion (q) and aphelion (Q) Mercury Positions show every 5 days before and after the perihelion on May 20, 2006

  7. File:ThePlanets Orbits Ceres Mars PolarView.svg - Wikipedia

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

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  8. File:ThePlanets Orbits Ceres Mars.svg - Wikipedia

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

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  9. Orbital eccentricity - Wikipedia

    en.wikipedia.org/wiki/Orbital_eccentricity

    The table lists the values for all planets and dwarf planets, and selected asteroids, comets, and moons. Mercury has the greatest orbital eccentricity of any planet in the Solar System (e = 0.2056), followed by Mars of 0.093 4. Such eccentricity is sufficient for Mercury to receive twice as much solar irradiation at perihelion compared to aphelion.

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