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  2. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    For example, if a TNO is incorrectly assumed to have a mass of 3.59 × 10 20 kg based on a radius of 350 km with a density of 2 g/cm 3 but is later discovered to have a radius of only 175 km with a density of 0.5 g/cm 3, its true mass would be only 1.12 × 10 19 kg.

  3. List of gravitationally rounded objects of the Solar System

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

    Vesta (radius 262.7 ± 0.1 km), the second-largest asteroid, appears to have a differentiated interior and therefore likely was once a dwarf planet, but it is no longer very round today. [74] Pallas (radius 255.5 ± 2 km ), the third-largest asteroid, appears never to have completed differentiation and likewise has an irregular shape.

  4. Uranus - Wikipedia

    en.wikipedia.org/wiki/Uranus

    [17] [84] The core is relatively small, with a mass of only 0.55 Earth masses and a radius less than 20% of the planet; the mantle comprises its bulk, with around 13.4 Earth masses, and the upper atmosphere is relatively insubstantial, weighing about 0.5 Earth masses and extending for the last 20% of Uranus's radius. [17] [84] Uranus's core ...

  5. Mean radius (astronomy) - Wikipedia

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

    The mean radius in astronomy is a measure for the size of planets and small Solar System bodies. Alternatively, the closely related mean diameter ( D {\displaystyle D} ), which is twice the mean radius, is also used.

  6. Schwarzschild radius - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild_radius

    The Schwarzschild radius or the gravitational radius is a physical ... is a coordinate singularity, meaning that it is an artifact of the ... Uranus: 8. 681 × 10 25 ...

  7. Miranda (moon) - Wikipedia

    en.wikipedia.org/wiki/Miranda_(moon)

    This sub-nebula either existed around Uranus for some period of time after its formation, or was created following a cosmic impact which would have given its great obliquity to the axis of rotation of Uranus. [56] However, this relatively small moon has areas that are surprisingly young compared to the geological time scale. [57]

  8. Rings of Uranus - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Uranus

    The mean size of the ring particles is 0.2–20.0 m, [18] and the mean separation is around 4.5 times their radius. [24] The ring is almost devoid of dust, possibly due to the aerodynamic drag from Uranus' extended atmospheric corona. [3] Due to its razor-thin nature the ε ring is invisible when viewed edge-on.

  9. Surface gravity - Wikipedia

    en.wikipedia.org/wiki/Surface_gravity

    These proportionalities may be expressed by the formula: where g is the surface gravity of an object, expressed as a multiple of the Earth's, m is its mass, expressed as a multiple of the Earth's mass (5.976 × 10 24 kg) and r its radius, expressed as a multiple of the Earth's (mean) radius (6,371 km). [9]