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

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

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Donate

  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. Jupiter's north pole comes to life in this 3D infrared video

    www.aol.com/news/2018-04-12-jupiter-juno-nasa...

    Now, NASA has released a 3D infrared movie of Jupiter's north polar region, depicting the intense storms in the area, as well as the dynamo that powers the planet's massive magnetic field.

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

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

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  6. Astrometry - Wikipedia

    en.wikipedia.org/wiki/Astrometry

    Once a movement per unit time is observed, astronomers compensate for the parallax caused by Earth's motion during this time and the heliocentric distance to this object is calculated. Using this distance and other photographs, more information about the object, including its orbital elements , can be obtained. [ 18 ]

  7. Jet Propulsion Laboratory Development Ephemeris - Wikipedia

    en.wikipedia.org/wiki/Jet_Propulsion_Laboratory...

    Files vary in the time periods they cover, ranging from a few hundred years to several thousand, and bodies they include. Data may be based on each planet's geometric center or a planetary-system barycenter. The use of Chebyshev polynomials enables highly precise, efficient calculations for any given point in time.

  8. Differential rotation - Wikipedia

    en.wikipedia.org/wiki/Differential_rotation

    Stars and planets rotate in the first place because conservation of angular momentum turns random drifting of parts of the molecular cloud that they form from into rotating motion as they coalesce. Given this average rotation of the whole body, internal differential rotation is caused by convection in stars which is a movement of mass, due to ...

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