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  2. Free-return trajectory - Wikipedia

    en.wikipedia.org/wiki/Free-return_trajectory

    Sketch of a circumlunar free return trajectory (not to scale), plotted on the rotating reference frame rotating with the moon. (Moon's motion only shown for clarity) In orbital mechanics, a free-return trajectory is a trajectory of a spacecraft traveling away from a primary body (for example, the Earth) where gravity due to a secondary body (for example, the Moon) causes the spacecraft to ...

  3. File:Orbits around earth scale diagram.svg - Wikipedia

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

    Distance above earth (km) Distance from center of earth (km) Earth Erde Terre భూమి: Blue/brown image: 0: 6370 Low Earth Orbit (LEO) Low Earth Orbit Orbite terrestre basse భూ నిమ్న కక్ష్య: Cyan area: 160 to 2,000: 6,530 to 8,370 Medium Earth Orbit (MEO) Medium Earth Orbit Orbite moyenne de la terre

  4. Saturn - Wikipedia

    en.wikipedia.org/wiki/Saturn

    With an average orbital speed of 9.68 km/s, [6] it takes Saturn 10,759 Earth days (or about 29 + 1 ⁄ 2 years) [86] to finish one revolution around the Sun. [6] As a consequence, it forms a near 5:2 mean-motion resonance with Jupiter. [87] The elliptical orbit of Saturn is inclined 2.48° relative to the orbital plane of the Earth. [6]

  5. File:Saturn diagram.svg - Wikipedia

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

    This W3C-invalid diagram was created with Inkscape …important. This diagram uses embedded text that can be easily translated using a text editor. This is a featured picture on Wikimedia Commons ( Featured pictures ) and is considered one of the finest images.

  6. NASA spacecraft captures beautiful photos of Saturn orbit change

    www.aol.com/article/news/2016/12/08/nasa...

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  7. List of objects at Lagrange points - Wikipedia

    en.wikipedia.org/wiki/List_of_objects_at...

    Mission consists of two spacecraft, which were the first spacecraft to reach Earth–Moon Lagrangian points. Both moved through Earth–Moon Lagrangian points, and are now in lunar orbit. [34] [35] WIND: Sun–Earth L 2: NASA: Arrived at L 2 in November 2003 and departed April 2004. Gaia Space Observatory: Sun–Earth L 2: ESA: Launched 19 ...

  8. Rings of Saturn - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Saturn

    Earth appears as a dot at 4 o'clock, between the G and E rings – with its brightness artificially exaggerated in this photograph. Saturn has the most extensive and complex ring system of any planet in the Solar System. The rings consist of particles in orbit around the planet made almost entirely of water ice, with a trace component of rocky ...

  9. Great conjunction - Wikipedia

    en.wikipedia.org/wiki/Great_conjunction

    Saturn's orbit plane is inclined 2.485 degrees relative to Earth's, and Jupiter's is inclined 1.303 degrees. The ascending nodes of both planets are similar (100.6 degrees for Jupiter and 113.7 degrees for Saturn), meaning if Saturn is above or below Earth's orbital plane Jupiter usually is too. Because these nodes align so well it would be ...