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  2. Atmosphere of Jupiter - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Jupiter

    Jupiter does not have a solid surface, and the lowest atmospheric layer, the troposphere, smoothly transitions into the planet's fluid interior. [2] This is a result of having temperatures and the pressures well above those of the critical points for hydrogen and helium, meaning that there is no sharp boundary between gas and liquid phases.

  3. Atmospheric super-rotation - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_super-rotation

    Atmospheric super-rotation is a phenomenon where a planet's atmosphere rotates faster than the planet itself. This behavior is observed in the atmospheres of Venus , Titan , Jupiter , and Saturn. Venus exhibits the most extreme super-rotation, with its atmosphere circling the planet in four Earth days, much faster than the planet's own rotation ...

  4. Vortex - Wikipedia

    en.wikipedia.org/wiki/Vortex

    For an example, if a water bucket is rotated or spun constantly, it will rotate around an invisible line called the axis line. The rotation moves around in circles. In this example the rotation of the bucket creates extra force. The reason that the vortices can change shape is the fact that they have open particle paths.

  5. Jupiter actually does not orbit the sun - AOL

    www.aol.com/2016-07-27-jupiter-actually-does-not...

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  6. The Big Picture: three Galilean moons make their way across ...

    www.aol.com/news/2015-02-07-big-picture-jupiter...

    It's easy for Hubble to take pictures of Jupiter or its moons, but it only gets the chance to capture the planet on cam with three visible Galilean satellites once or twice a decade. That's what ...

  7. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    Saturn would later have begun to migrate inwards at a faster rate than Jupiter until the two planets became captured in a 3:2 mean motion resonance at approximately 1.5 AU (220 million km; 140 million mi) from the Sun. [32] This changed the direction of migration, causing them to migrate away from the Sun and out of the inner system to their ...

  8. Tidal heating of Io - Wikipedia

    en.wikipedia.org/wiki/Tidal_heating_of_Io

    Io's shape changes as it completes its orbit. (C) Earth's moon's orbit is actually more eccentric than Io's, but Earth's gravity is much weaker than Jupiter's, so Earth's moon does not experience as much deformation. [1] Tidal heating of Io (also known as tidal working) occurs through the tidal friction processes between Jupiter and its moon ...

  9. Potential for water on Jupiter’s moon Europa - study - AOL

    www.aol.com/potential-shallow-liquid-water...

    Europa is a prime candidate for life in the Solar System, researchers suggest.