The photon sphere of a black hole is a region where light can orbit the black hole before being pulled in, while the event horizon is the point of no return where nothing, not even light, can escape the black hole's gravitational pull. The photon sphere is closer to the black hole than the event horizon.
The phrase commonly used to describe the event horizon in black holes is "point of no return."
The event horizon balance beam is significant in the study of black holes because it helps scientists understand the concept of an event horizon, which is the point of no return around a black hole where gravity is so strong that nothing, not even light, can escape. By studying how objects behave on the balance beam near the event horizon, researchers can gain insights into the extreme gravitational forces at play near black holes.
The event horizon of a black hole is a boundary beyond which the gravitational pull is so strong that not even light can escape. This means that anything beyond the event horizon is invisible to us, as no light or information can reach us from that region.
At the event horizon of a black hole, the gravitational pull is so strong that not even light can escape. This creates a boundary beyond which nothing can return, including matter and energy. In the interstellar environment, this means that anything that crosses the event horizon is essentially lost to the black hole, with no possibility of escape or communication.
The escape velocity at the event horizon of a black hole is the speed at which an object must travel to break free from the black hole's gravitational pull. It is equal to the speed of light, which is approximately 186,282 miles per second.
A black hole's photon sphere is the region around the black hole where photons can orbit in a stable circular path. The event horizon is the boundary beyond which nothing, not even light, can escape the gravitational pull of the black hole. In simpler terms, the photon sphere is where light can circle the black hole before falling in, while the event horizon marks the point of no return.
The escape velocity is affected by altitude for any celestial body; the further away from the mass, the lower the escape velocity from that point. At the event horizon, the escape velocity is the speed of light. Within the photon sphere but outside the event horizon, light paths not pointing outward will intersect the event horizon. At the photon sphere, a notionally tangential light beam would ideally remain in a perfectly circular "orbit" around the black hole (although, traveling in a geodesic, the light beam will be only traveling straight as far as it's concerned, space itself is bent).... outside the photon sphere, the escape velocity continues to fall with distance.
Photons do not become "entangled" with each other any more than waves on water do. They move along independently. If a photon crosses the event horizon of a black hole as that photon follows the curve of spacetime "down" into the black hole, it is probable that a photon moving "with" it will suffer the same fate.
The event horizon is the "point of no return" - nothing inside that can escape. In the simplest case (of a non-rotating black hole), this is a sphere, at a certain distance from the black hole's center. The size of the black hole is often taken to be the size of the event horizon.
That refers specifically to black holes (there are other types of "collapsed stars"). This sphere is called the "event horizon".
It seems you are referring not to any collapsed star, but a black hole. The "event horizon" is the area from which nothing can escape.
Black holes have both material and non-material components. For example, the photon sphere, ergosphere, and event horizon are all "notional" aspects of its anatomy, despite having significant practical consequences; strictly speaking you could not "touch" them. The singularity at the center, where the mass is concentrated, definitely contains matter - but is a form of matter not fully described by our physics, and sometimes referred to as exotic matter.
Simply divide the mass of the black hole by the volume contained within the event horizon. This is fairly simple for a typical black hole, since the event horizon will approximate a sphere whose radius is the collapsed object's Schwarzschild radius.
The apparent horizon is formed first in the evolution of a black hole. It represents the point from which no light can escape, defining the boundary of a black hole's event horizon.
No planet has an event horizon. A black hole has an event horizon; it is the radius within which light cannot escape.
The event horizon of a black hole is spherical.
The so-called "event horizon" of a black hole is the point-of-no-return. That means that anything that gets inside the event horizon can't get out any more, even if if it moves at the speed of light.