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  2. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    Alan Stern calls these satellite planets, although the term major moon is more common. The smallest natural satellite that is gravitationally rounded is Saturn I Mimas (radius 198.2 ± 0.4 km). This is smaller than the largest natural satellite that is known not to be gravitationally rounded, Neptune VIII Proteus (radius 210 ± 7 km).

  3. Rings of Saturn - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Saturn

    This structure is thought to arise, in several different ways, from the gravitational pull of Saturn's many moons. Some gaps are cleared out by the passage of tiny moonlets such as Pan , [ 48 ] many more of which may yet be discovered, and some ringlets seem to be maintained by the gravitational effects of small shepherd satellites (similar to ...

  4. Saturn - Wikipedia

    en.wikipedia.org/wiki/Saturn

    The examination of Saturn's gravitational moment, in combination with physical models of the interior, has allowed constraints to be placed on the mass of Saturn's core. In 2004, scientists estimated that the core must be 9–22 times the mass of Earth, [ 44 ] [ 45 ] which corresponds to a diameter of about 25,000 km (16,000 mi). [ 46 ]

  5. Tidal force - Wikipedia

    en.wikipedia.org/wiki/Tidal_force

    Figure 4: Saturn's rings are inside the orbits of its principal moons. Tidal forces oppose gravitational coalescence of the material in the rings to form moons. [12] In the case of an infinitesimally small elastic sphere, the effect of a tidal force is to distort the shape of the body without any change in volume.

  6. Mimas - Wikipedia

    en.wikipedia.org/wiki/Mimas

    Mimas, also designated Saturn I, is the seventh-largest natural satellite of Saturn. With a mean diameter of 396.4 kilometres or 246.3 miles, Mimas is the smallest astronomical body known to be roughly rounded in shape due to its own gravity.

  7. Escape velocity - Wikipedia

    en.wikipedia.org/wiki/Escape_velocity

    G is the universal gravitational constant (G ≈ 6.67 × 10 −11 m 3 ⋅kg −1 ⋅s −2 ‍ [4]) g = GM/d 2 is the local gravitational acceleration (or the surface gravity, when d = r). The value GM is called the standard gravitational parameter, or μ, and is often known more accurately than either G or M separately.

  8. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    Several prominent examples of secular resonance involve Saturn. 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°).

  9. Moons of Saturn - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Saturn

    In 2019, twenty new irregular satellites of Saturn were reported, resulting in Saturn overtaking Jupiter as the planet with the most known moons for the first time since 2000. [ 13 ] [ 3 ] In 2019, researchers Edward Ashton, Brett Gladman, and Matthew Beaudoin conducted a survey of Saturn's Hill sphere using the 3.6-meter Canada–France ...