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  2. File:PIA02863 - Jupiter surface motion animation 10fps.ogv

    en.wikipedia.org/wiki/File:PIA02863_-_Jupiter...

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  3. Wikipedia : Featured picture candidates/PIA02863 - Jupiter ...

    en.wikipedia.org/.../Cloud_motion_on_Jupiter

    1 Cloud motion on Jupiter. Toggle the table of contents. Wikipedia: Featured picture candidates/PIA02863 - Jupiter surface motion animation.gif. Add languages. Add links.

  4. File:PIA02863 - Jupiter surface motion animation thumbnail ...

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  5. Retrograde and prograde motion - Wikipedia

    en.wikipedia.org/wiki/Retrograde_and_prograde_motion

    Retrograde motion in astronomy is, in general, orbital or rotational motion of an object in the direction opposite the rotation of its primary, that is, the central object (right figure). It may also describe other motions such as precession or nutation of an object's rotational axis .

  6. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    3-hour timelapse showing rotation of Jupiter and orbital motion of the moons. Jupiter is the only planet whose barycentre with the Sun lies outside the volume of the Sun, though by 7% of the Sun's radius. [130] [131] The average distance between Jupiter and the Sun is 778 million km (5.20 AU) and it completes an orbit every 11.86 years.

  7. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    In the asteroid belt within 3.5 AU from the Sun, the major mean-motion resonances with Jupiter are locations of gaps in the asteroid distribution, the Kirkwood gaps (most notably at the 4:1, 3:1, 5:2, 7:3 and 2:1 resonances). Asteroids have been ejected from these almost empty lanes by repeated perturbations. However, there are still ...

  8. Solar rotation - Wikipedia

    en.wikipedia.org/wiki/Solar_rotation

    At the equator, the solar rotation period is 24.47 days. This is called the sidereal rotation period, and should not be confused with the synodic rotation period of 26.24 days, which is the time for a fixed feature on the Sun to rotate to the same apparent position as viewed from Earth (the Earth's orbital rotation is in the same direction as the Sun's rotation).

  9. Rømer's determination of the speed of light - Wikipedia

    en.wikipedia.org/wiki/Rømer's_determination_of...

    The point L on the diagram represents the second quadrature of Jupiter, when the angle between Jupiter and the Sun (as seen from Earth) is 90°. [ note 6 ] Rømer assumes that an observer could see an emergence of Io at the second quadrature ( L ), and the emergence which occurs after one orbit of Io around Jupiter (when the Earth is taken to ...