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  2. Rotation period (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Rotation_period_(astronomy)

    For gaseous or fluid bodies, such as stars and giant planets, the period of rotation varies from the object's equator to its pole due to a phenomenon called differential rotation. Typically, the stated rotation period for a giant planet (such as Jupiter, Saturn, Uranus, Neptune) is its internal rotation period, as determined from the rotation ...

  3. (455502) 2003 UZ413 - Wikipedia

    en.wikipedia.org/wiki/(455502)_2003_UZ413

    (455502) 2003 UZ 413 (provisional designation 2003 UZ 413) is a trans-Neptunian object (TNO) with an absolute magnitude of 4.38. [5] It is in a 2:3 orbital resonance with Neptune, thus it is classified as a plutino. [3] There are indications it may be dense enough to be a dwarf planet. It was given the minor planet number 455502 on 22 February ...

  4. Neptune - Wikipedia

    en.wikipedia.org/wiki/Neptune

    The 3:4, 3:5, 4:7 and 2:5 resonances are less populated. [150] Neptune has a number of known trojan objects occupying both the Sun–Neptune L 4 and L 5 Lagrangian points—gravitationally stable regions leading and trailing Neptune in its orbit, respectively. [151] Neptune trojans can be viewed as being in a 1:1 resonance with Neptune.

  5. Scientists recreate Neptune's diamond rain using ... - AOL

    www.aol.com/news/2017-08-21-neptune-diamond-rain...

    They recreated Neptune's conditions at Stanford's SLAC Laboratory and successfully observed the formation of diamond rain, thanks to the help of some very powerful lasers. Scientists recreate ...

  6. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    According to Copernicus: [3] [4] The planetary orbit is a circle with epicycles. The Sun is approximately at the center of the orbit. The speed of the planet in the main orbit is constant. Despite being correct in saying that the planets revolved around the Sun, Copernicus was incorrect in defining their orbits.

  7. On Neptune and Uranus, Diamonds Rain Down from the Sky - AOL

    www.aol.com/lifestyle/neptune-uranus-diamonds...

    Scientists have finally discovered how sheets of diamond rain form on the ice giants, Neptune and Uranus. The answer could explain why Neptune’s core is hot.

  8. Poles of astronomical bodies - Wikipedia

    en.wikipedia.org/wiki/Poles_of_astronomical_bodies

    Venus rotates clockwise, and Uranus has been knocked on its side and rotates almost perpendicular to the rest of the Solar System. The ecliptic remains within 3° of the invariable plane over five million years, [2] but is now inclined about 23.44° to Earth's celestial equator used for the coordinates of poles. This large inclination means ...

  9. Outline of Neptune - Wikipedia

    en.wikipedia.org/wiki/Outline_of_Neptune

    Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times the mass of Earth and slightly larger than Neptune. [a] Neptune orbits the Sun once every 164.8 years at an average distance of 30.1 astronomical units (4.50 × 10 9 km).