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  2. File:Neptune, Earth size comparison.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Neptune,_Earth_size...

    File:Neptune, Earth size comparison.jpg. Size of this preview: 800 × 587 pixels. Other resolutions: 320 × 235 pixels | 640 × 469 pixels | 1,024 × 751 pixels | 1,280 × 939 pixels | 2,560 × 1,877 pixels | 3,000 × 2,200 pixels. Original file ‎ (3,000 × 2,200 pixels, file size: 2.02 MB, MIME type: image/jpeg) This is a file from the ...

  3. List of Solar System objects by size - Wikipedia

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

    Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system. Relative masses of the solid bodies of the Solar System. Earth at 48% and Venus at 39% dominate. Bodies less massive than Pluto are not visible at this scale. Relative masses of the rounded moons of the Solar System.

  4. Exoplanet orbital and physical parameters - Wikipedia

    en.wikipedia.org/wiki/Exoplanet_orbital_and...

    However, the planets detected by Kepler are mostly between the size of Neptune and the size of Earth. [9] If a planet is detectable by both the radial-velocity and the transit methods, then both its true mass and its radius can be determined, as well as its density .

  5. Ceres (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Ceres_(dwarf_planet)

    Ceres follows an orbit between Mars and Jupiter, near the middle of the asteroid belt, with an orbital period (year) of 4.6 Earth years. Compared to other planets and dwarf planets, Ceres's orbit is moderately tilted relative to that of Earth; its inclination (i) is 10.6°, compared to 7° for Mercury and 17° for Pluto.

  6. 28978 Ixion - Wikipedia

    en.wikipedia.org/wiki/28978_Ixion

    Absolute magnitude (H) 3.774 ± 0.021 [17] [12] 3.6 (assumed) [2] [5] 28978 Ixion ( / ɪkˈsaɪ.ən /, provisional designation 2001 KX76) is a large trans-Neptunian object and a possible dwarf planet. It is located in the Kuiper belt, a region of icy objects orbiting beyond Neptune in the outer Solar System.

  7. Template:Planetary radius - Wikipedia

    en.wikipedia.org/wiki/Template:Planetary_radius

    Directory. This template is to show size comparison of Jupiter, Neptune and the Earth alongside extrasolar planets that have their radial size confirmed. {{Planetary radius | radius = <!--simplified number of the radius (Jupiter equals 100px)--> }} Some planets might have a radius that would be hard to compare to Jupiter.

  8. Hill sphere - Wikipedia

    en.wikipedia.org/wiki/Hill_sphere

    v. t. e. The Hill sphere is a common model for the calculation of a gravitational sphere of influence. It is the most commonly used model to calculate the spatial extent of gravitational influence of an astronomical body ( m) in which it dominates over the gravitational influence of other bodies, particularly a primary ( M ). [1]

  9. Outline of Neptune - Wikipedia

    en.wikipedia.org/wiki/Outline_of_Neptune

    The following outline is provided as an overview of and topical guide to Neptune: Neptune – eighth and farthest known planet from the Sun in the Solar System. In the Solar System, it is the fourth-largest planet by diameter, the third-most-massive planet, and the densest giant planet. Neptune is 17 times the mass of Earth and is slightly more ...