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  2. File:Animation of the planetary system around Sun-like star ...

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

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  3. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    Despite being correct in saying that the planets revolved around the Sun, Copernicus was incorrect in defining their orbits. Introducing physical explanations for movement in space beyond just geometry, Kepler correctly defined the orbit of planets as follows: [1] [2] [5]: 53–54 The planetary orbit is not a circle with epicycles, but an ellipse.

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    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. Smaller icy objects such as comets frequently orbit at significantly greater angles to this plane.

  5. Ecliptic - Wikipedia

    en.wikipedia.org/wiki/Ecliptic

    Most of the planets orbit the Sun very nearly in the same plane in which Earth orbits, the ecliptic. Five planets (Earth included) lined up along the ecliptic in July 2010, illustrating how the planets orbit the Sun in nearly the same plane. Photo taken at sunset, looking west over Surakarta, Java, Indonesia.

  6. Copernican Revolution - Wikipedia

    en.wikipedia.org/wiki/Copernican_Revolution

    2. The Law of Equal Areas in Equal Time: A line that connects a planet to the Sun sweeps out equal areas in equal times. 3. The Law of Harmony: The time required for a planet to orbit the Sun, called its period, is proportional to long axis of the ellipse raised to the 3/2 power. The constant of proportionality is the same for all the planets.

  7. List of Solar System probes - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System_probes

    Lissajous orbit around Sun-Earth L2 point success study of formation and evolution of galaxies and stars 2009-026A: Planck: ESA: 14 May 2009 (launch) - 2013 Lissajous orbit around Sun-Earth L2 point success cosmic microwave background observations 2009-026B: IKAROS: JAXA: 20 May 2010 (launch) Earth-Venus transfer heliocentric orbit operational

  8. Newton's theorem of revolving orbits - Wikipedia

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

    The green planet moves angularly three times as fast as the blue planet (k = 3); it completes three orbits for every orbit of the blue planet. The red planet illustrates purely radial motion with no angular motion (k = 0). The paths followed by the green and blue planets are shown in Figure 9.

  9. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    All five known planets orbit around star A (none are circumbinary or orbit around star B). Closest system with exactly five confirmed planets. Gliese 180: Eridanus: 04 h 53 m 49.9798 s: −17° 46′ 24.294″ 10.894: 40.3: M2V [41] or M3V [42] 0.39: 3562: unknown: 3: The habitability of planets b and c is disputed. [43] [44] HD 69830: Puppis ...