• Thumbnail for 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...
    26 KB (2,933 words) - 05:29, 5 April 2024
  • the sphere of activity which extends well beyond the sphere of influence. The most common base models to calculate the sphere of influence is the Hill sphere...
    13 KB (1,386 words) - 00:04, 17 April 2024
  • to the Hill sphere, but smaller, only about 60% of the radius Sphere of influence (black hole), a region around a supermassive black hole SPHERES (Synchronized...
    5 KB (607 words) - 01:15, 11 February 2024
  • Thumbnail for Earth's orbit
    surface covered by water in the southern hemisphere. The Hill sphere (gravitational sphere of influence) of the Earth is about 1,500,000 kilometers (0...
    17 KB (1,834 words) - 05:28, 17 March 2024
  • Thumbnail for Oort cloud
    cosmographic boundary of the Solar System. This area is defined by the Sun's Hill sphere, and hence lies at the interface between solar and galactic gravitational...
    56 KB (6,188 words) - 20:27, 16 April 2024
  • Thumbnail for Lagrange point
    equal distances r from the smaller object, equal to the radius of the Hill sphere, given by: r ≈ R μ 3 3 {\displaystyle r\approx R{\sqrt[{3}]{\frac {\mu...
    50 KB (5,705 words) - 15:45, 18 April 2024
  • Thumbnail for Solar System
    as Comet West, have aphelia around 70,000 AU from the Sun. The Sun's Hill sphere with respect to the galactic nucleus, the effective range of its gravitational...
    204 KB (20,507 words) - 20:22, 27 April 2024
  • Thumbnail for 469219 Kamoʻoalewa
    translates into 13 lunar distances. This distance is well outside of Earth's Hill sphere of 1.5 million km (3.9 LD). As it orbits the Sun, Kamoʻoalewa appears...
    21 KB (1,859 words) - 01:13, 25 April 2024
  • surface of a sphere of tungsten half a metre in radius would travel at slightly more than 1 mm/s, completing an orbit every hour. If the same sphere were made...
    17 KB (2,059 words) - 21:43, 10 April 2024
  • such a way that it appears to orbit Earth, but well outside Earth's Hill sphere, making it a quasi-satellite. The orbit of 2023 FW13 has a one-to-one...
    5 KB (214 words) - 19:04, 10 April 2024
  • where the negligible body is a satellite of the body of lesser mass, see Hill sphere; for binary systems, see Roche lobe. Specific solutions to the three-body...
    66 KB (8,605 words) - 09:20, 22 April 2024
  • Thumbnail for Outer space
    pontentials from other bodies, is the body's sphere of influence or gravity well, mostly described with the Hill sphere model. In the case of Earth this includes...
    132 KB (12,971 words) - 18:57, 28 April 2024
  • satellite, assumed to be the size of Ceres, orbiting near the planet's Hill sphere, and thus more subject to gravitational perturbations from Jupiter. As...
    22 KB (2,341 words) - 18:24, 23 April 2024
  • Thumbnail for Sphere eversion
    In differential topology, sphere eversion is the process of turning a sphere inside out in a three-dimensional space (the word eversion means "turning...
    12 KB (1,127 words) - 21:19, 9 March 2024
  • Thumbnail for Interplanetary Transport Network
    these low energy paths. Gravitational keyhole Gravity assist Halo orbit Hill sphere Horseshoe orbit Interplanetary spaceflight Lunar cycler Mars cycler Orbital...
    17 KB (1,862 words) - 01:45, 28 April 2024
  • Thumbnail for Aerospace engineering
    equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    24 KB (2,424 words) - 00:25, 24 March 2024
  • Thumbnail for Apsis
    Archived July 29, 2017, at the Wayback Machine is also common (e.g., McGraw Hill Dictionary of Scientific and Technical Terms, 5th edition, 1994, p. 114)...
    42 KB (3,898 words) - 23:55, 26 April 2024
  • Thumbnail for Interstellar probe
    of the region in which the Sun's gravitational field is dominant (the Hill sphere) is thought to be at around 230,000 astronomical units (3.6 light-years)...
    38 KB (4,192 words) - 22:27, 27 April 2024
  • Thumbnail for Light-year
    Szirtes (1997), Applied dimensional analysis and modeling, New York: McGraw-Hill, p. 60, ISBN 978-0-07-062811-3 Comins, Neil F. (2013), Discovering the Essential...
    24 KB (1,885 words) - 04:10, 21 April 2024
  • Thumbnail for Io (moon)
    plasma torus (discussed below) and by other processes into filling Io's Hill sphere, which is the region where Io's gravity is dominant over Jupiter's. Some...
    112 KB (12,388 words) - 03:07, 26 April 2024
  • Thumbnail for True anomaly
    equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    8 KB (1,107 words) - 22:41, 12 January 2024
  • Thumbnail for Parabolic trajectory
    equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    7 KB (1,090 words) - 14:52, 9 December 2023
  • Thumbnail for Kepler's laws of planetary motion
    in a laborious attempt to determine what he viewed as the "music of the spheres" according to precise laws, and express it in terms of musical notation...
    57 KB (8,338 words) - 19:35, 27 April 2024
  • Thumbnail for Halo orbit
    equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    11 KB (1,104 words) - 16:53, 22 April 2024
  • Thumbnail for Lunar orbit
    insufficient and three-body models are required. Although the Moon's Hill sphere extends to a radius of 60,000 km (37,000 mi), the gravity of Earth intervenes...
    16 KB (1,730 words) - 18:59, 18 April 2024
  • equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    13 KB (1,947 words) - 23:49, 23 April 2024
  • equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    11 KB (1,395 words) - 16:44, 13 January 2024
  • Thumbnail for Orbital inclination
    equation Celestial mechanics Gravitational influences Barycenter Hill sphere Perturbations Sphere of influence N-body orbits Lagrangian points (Halo orbits)...
    11 KB (1,465 words) - 15:40, 23 October 2023
  • Thumbnail for Escape velocity
    typically used to determine whether an object will remain in the gravitational sphere of influence of a given body. For example, in solar system exploration it...
    27 KB (3,642 words) - 22:08, 24 March 2024
  • Thumbnail for Quasi-satellite
    to true satellites, quasi-satellite orbits lie outside the planet's Hill sphere, and are unstable. Over time they tend to evolve to other types of resonant...
    14 KB (1,585 words) - 01:00, 18 April 2024