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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |