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  2. Saturn - Wikipedia

    en.wikipedia.org/wiki/Saturn

    The Moon's orbit is inclined by several degrees relative to Saturn's, so occultations will only occur when Saturn is near one of the points in the sky where the two planes intersect (both the length of Saturn's year and the 18.6-Earth-year nodal precession period of the Moon's orbit influence the periodicity).

  3. Cassini–Huygens - Wikipedia

    en.wikipedia.org/wiki/Cassini–Huygens

    Cassini was captured by Saturn's gravity at around 8:54 pm Pacific Daylight Time on June 30, 2004. During the maneuver Cassini passed within 20,000 km (12,000 mi) of Saturn's cloud tops. When Cassini was in Saturnian orbit, departure from the Saturn system was evaluated in 2008 during end of mission planning. [86] [clarification needed]

  4. Kepler's laws of planetary motion - Wikipedia

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

    The square of a planet's orbital period is proportional to the cube of the length of the semi-major axis of its orbit. The elliptical orbits of planets were indicated by calculations of the orbit of Mars. From this, Kepler inferred that other bodies in the Solar System, including those farther away from the Sun, also have elliptical orbits. The ...

  5. Rings of Saturn - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Saturn

    The rings of Saturn are the most extensive and complex ring system of any planet in the Solar System. They consist of countless small particles, ranging in size from micrometers to meters, [ 1] that orbit around Saturn. The ring particles are made almost entirely of water ice, with a trace component of rocky material.

  6. List of orbits - Wikipedia

    en.wikipedia.org/wiki/List_of_orbits

    Saturn orbit (Cronocentric orbit, ... (ASO): A synchronous orbit around the planet Mars with an orbital period equal in length to Mars' sidereal day, 24.6229 hours.

  7. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    There is a near-resonance between the precession of Saturn's rotational axis and that of Neptune's orbital axis (both of which have periods of about 1.87 million years), which has been identified as the likely source of Saturn's large axial tilt (26.7°). [18] [19] [20] Initially, Saturn probably had a tilt closer to that of Jupiter (3.1 ...

  8. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    When the orbit is more ... (the length of a sidereal ... Saturn's moon Titan has a cycle of approximately 60,000 years that could change the location of ...

  9. Saturn IB - Wikipedia

    en.wikipedia.org/wiki/Saturn_IB

    The Saturn IB [a] (also known as the uprated Saturn I) was an American launch vehicle commissioned by the National Aeronautics and Space Administration (NASA) for the Apollo program. It uprated the Saturn I by replacing the S-IV second stage (90,000-pound-force (400,000 N), 43,380,000 lb-sec total impulse), with the S-IVB (200,000-pound-force ...