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  2. Jupiter's South Pole - Wikipedia

    en.wikipedia.org/wiki/Jupiter's_South_Pole

    For more than three years the structure of cyclones at both poles of the nearest to us gas giant remained stable, but on November 3, 2019, on the 22nd rotation, "Juno" found the birth of a new cyclone at the South Pole: it quickly "pushed" the previous (although still has a smaller size, about 800 km), and now the centers of peripheral cyclones ...

  3. Poles of astronomical bodies - Wikipedia

    en.wikipedia.org/wiki/Poles_of_astronomical_bodies

    The poles of astronomical bodies are determined based on their axis of rotation in relation to the celestial poles of the celestial sphere. Astronomical bodies include stars, planets, dwarf planets and small Solar System bodies such as comets and minor planets (e.g., asteroids), as well as natural satellites and minor-planet moons.

  4. Pole star - Wikipedia

    en.wikipedia.org/wiki/Pole_star

    The south pole star is Delta Doradus. Mars: The top two stars in the Northern Cross, Sadr and Deneb, point to the pole. [26] Markeb is a couple of degrees away. Jupiter: a little over two degrees away from Aldhibah: about two degrees north of Delta Doradus: Saturn: in the far northern region of Cepheus, about six degrees from Polaris: Delta ...

  5. 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.

  6. Jupiter actually does not orbit the sun - AOL

    www.aol.com/article/2016/07/27/jupiter-actually...

    In science class, we always learned that all the planets in our solar system orbit around the sun. Scientists have figured out this is not necessarily true.

  7. Axial tilt - Wikipedia

    en.wikipedia.org/wiki/Axial_tilt

    Since obliquity is the angle between the axis of rotation and the direction perpendicular to the orbital plane, it changes as the orbital plane changes due to the influence of other planets. But the axis of rotation can also move (axial precession), due to torque exerted by the Sun on a planet's equatorial bulge. Like Earth, all of the rocky ...

  8. AOL Mail

    mail.aol.com

    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  9. Great Red Spot - Wikipedia

    en.wikipedia.org/wiki/Great_Red_Spot

    Jupiter's Great Red Spot (GRS) is an elliptical shaped anticyclone, occurring at 22 degrees below the equator, in Jupiter's southern hemisphere. [39] The largest anticyclonic storm (~16,000 km) in our solar system, little is known about its internal depth and structure. [ 40 ]