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  2. Hill sphere - Wikipedia

    en.wikipedia.org/wiki/Hill_sphere

    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 ]

  3. Sphere of influence (astrodynamics) - Wikipedia

    en.wikipedia.org/wiki/Sphere_of_influence_(astro...

    A sphere of influence (SOI) in astrodynamics and astronomy is the oblate spheroid-shaped region where a particular celestial body exerts the main gravitational influence on an orbiting object. This is usually used to describe the areas in the Solar System where planets dominate the orbits of surrounding objects such as moons , despite the ...

  4. Earth - Wikipedia

    en.wikipedia.org/wiki/Earth

    The Hill sphere, or the sphere of gravitational influence, of Earth is about 1.5 million km (930,000 mi) in radius. [164] [n 11] This is the maximum distance at which Earth's gravitational influence is stronger than that of the more distant Sun and planets.

  5. Satellite system (astronomy) - Wikipedia

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

    Gravitational accelerations at L 4. The Hill sphere is the region in which an astronomical body dominates the attraction of satellites. Of the Solar System planets, Neptune and Uranus have the largest Hill spheres, due to the lessened gravitational influence of the Sun at their far orbits, however all of the giant planets have Hill spheres in the vicinity of 100 million kilometres in radius.

  6. File:Comparison of Hill sphere and Roche limit.svg - Wikipedia

    en.wikipedia.org/wiki/File:Comparison_of_Hill...

    comparison of Hill sphere and Roche limit: Image title: Comparison of the Hill spheres and Roche limits of the Sun-Earth-Moon system (not to scale) with shaded regions denoting stable orbits of satellites of each body by CMG Lee. Width: 100%: Height: 100%

  7. Lagrange point - Wikipedia

    en.wikipedia.org/wiki/Lagrange_point

    Again, if the mass of the smaller object (M 2) is much smaller than the mass of the larger object (M 1) then L 2 is at approximately the radius of the Hill sphere, given by: The same remarks about tidal influence and apparent size apply as for the L 1 point.

  8. Roche lobe - Wikipedia

    en.wikipedia.org/wiki/Roche_lobe

    It is the easiest way for the debris to commute between a Hill sphere (an inner circle of blue and light blue) and communal gravity regions (figure-eights of yellow and green in the inner side). Hill sphere and horseshoe orbit. L 2 and L 3 are gravitational perturbation equilibria points. Passing through these two equilibrium points, debris can ...

  9. Irregular moon - Wikipedia

    en.wikipedia.org/wiki/Irregular_moon

    On the other hand, Neptune's Triton, which is probably a captured object, is usually listed as irregular despite being within 0.05 of the radius of Neptune's Hill sphere, so that Triton's precession is primarily controlled by Neptune's oblateness instead of by the Sun. [5] Neptune's Nereid and Saturn's Iapetus have semi-major axes close to 0.05 ...