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  2. Rotation period (astronomy) - Wikipedia

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

    Rotation period with respect to distant stars, the sidereal rotation period (compared to Earth's mean Solar days) Synodic rotation period (mean Solar day) Apparent rotational period viewed from Earth Sun [i] 25.379995 days (Carrington rotation) 35 days (high latitude) 25 d 9 h 7 m 11.6 s 35 d ~28 days (equatorial) [2] Mercury: 58.6462 days [3 ...

  3. Uranus - Wikipedia

    en.wikipedia.org/wiki/Uranus

    It has a marked axial tilt of 82.23° with a retrograde rotation period of 17 hours and 14 minutes. This means that in an 84-Earth-year orbital period around the Sun, its poles get around 42 years of continuous sunlight, followed by 42 years of continuous darkness.

  4. Synodic day - Wikipedia

    en.wikipedia.org/wiki/Synodic_day

    A synodic day (or synodic rotation period or solar day) is the period for a celestial object to rotate once in relation to the star it is orbiting, and is the basis of solar time. The synodic day is distinguished from the sidereal day , which is one complete rotation in relation to distant stars [ 1 ] and is the basis of sidereal time.

  5. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    Earth's rotation period relative to the International Celestial Reference Frame, called its stellar day by the International Earth Rotation and Reference Systems Service (IERS), is 86 164.098 903 691 seconds of mean solar time (UT1) (23 h 56 m 4.098 903 691 s, 0.997 269 663 237 16 mean solar days). [35] [n 3] Earth's rotation period relative to ...

  6. NASA’s only visit to Uranus happened during a rare cosmic ...

    www.aol.com/nasa-only-visit-uranus-happened...

    What’s known about Uranus could be off the mark. An unusual cosmic occurrence during the Voyager 2 spacecraft’s 1986 flyby might have skewed how scientists characterized the ice giant, new ...

  7. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    In the case of Mercury, half of the greater axis is about 5.79 × 10 10 m, the eccentricity of its orbit is 0.206 and the period of revolution 87.97 days or 7.6 × 10 6 s. From these and the speed of light (which is ~ 3 × 10 8 m/s ), it can be calculated that the apsidal precession during one period of revolution is ε = 5.028 × 10 −7 ...

  8. Orbital period - Wikipedia

    en.wikipedia.org/wiki/Orbital_period

    For example, the synodic period of the Moon's orbit as seen from Earth, relative to the Sun, is 29.5 mean solar days, since the Moon's phase and position relative to the Sun and Earth repeats after this period. This is longer than the sidereal period of its orbit around Earth, which is 27.3 mean solar days, owing to the motion of Earth around ...

  9. Disruptive Uranus Retrograde Ends! Blessings for Each ... - AOL

    www.aol.com/lifestyle/disruptive-uranus...

    On January 30, 2025, the planet of disruption gives us a break.Uranus stations direct, ending its retrograde. While Uranus is retrograde in Taurus, we're asked to move slowly and steadily toward ...