The sphere of influence is a region around a supermassive black hole in which the gravitational potential of the black hole dominates the gravitational...
4 KB (501 words) - 05:03, 5 April 2024
gravitational influence Sphere of influence (black hole), a region around a black hole in which the gravitation of the black hole dominates that of the host...
1 KB (183 words) - 06:54, 1 July 2024
orbiting objects Sphere of influence (black hole), a region around a black hole in which the gravity of the black hole dominates that of the host galaxy's bulge...
3 KB (438 words) - 11:48, 20 August 2023
a sphere of influence, and that needs to be accounted for to escape or stay in the sphere of influence. Hill sphere Sphere of influence (black hole) Clearing...
13 KB (1,385 words) - 10:15, 13 October 2024
(VLT) Sphere of influence (astrodynamics), similar to the Hill sphere, but smaller, only about 60% of the radius Sphere of influence (black hole), a region...
5 KB (626 words) - 09:14, 17 September 2024
An intermediate-mass black hole (IMBH) is a class of black hole with mass in the range of tens to tens thousand (102–105) solar masses: significantly higher...
26 KB (3,035 words) - 02:21, 10 October 2024
Roche limit (category Equations of astronomy)
Spaghettification (the extreme case of tidal distortion) Hill sphere Sphere of influence (black hole) Black hole Triton (moon) (Neptune's satellite) Comet...
13 KB (1,514 words) - 15:20, 1 October 2024
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 (2,917 words) - 08:03, 17 October 2024
Sagittarius A* (redirect from Black Hole at the center of the galaxy)
SADGE-AY-star), is the supermassive black hole at the Galactic Center of the Milky Way. Viewed from Earth, it is located near the border of the constellations Sagittarius...
73 KB (7,650 words) - 11:28, 30 September 2024
Messier 4 (section Central black hole)
center of this cluster, which appears to not be extended. This could thus be considered as kinematic evidence for an intermediate-mass black hole (even...
12 KB (1,213 words) - 02:22, 10 October 2024