Event Horizon – Am Rande des Universums ist ein Science-Fiction- und Horrorfilm aus dem Jahr von Regisseur Paul W. S. Anderson. Hauptdarsteller sind. Event Horizon (Lim. Uncut Mediabook - Cover A) (DVD + BLURAY). Logo Bluray Logo DVD. Kurzübersicht. MediaBook - 2 Discs. Paul W.S. Andersons Weltraum-Horrorfilm Event Horizon wird diesen Herbst dank Scream Factory im neuen Gewand auf Blu-ray erstrahlen.
Event Horizon – Am Rande des UniversumsEvent Horizon (Lim. Uncut Mediabook - Cover A) (DVD + BLURAY). Logo Bluray Logo DVD. Kurzübersicht. MediaBook - 2 Discs. Paul W.S. Andersons Weltraum-Horrorfilm Event Horizon wird diesen Herbst dank Scream Factory im neuen Gewand auf Blu-ray erstrahlen. Im Jahr verschwindet das Raumschiff Event Horizon urplötzlich in einem schwarzen Loch, und aus dem Routineauftrag wird ein Horrortrip. Erst sieben.
Event Horizon Uncut 📩 Stay up-to-date VideoEvent Horizon deleted scene
It is never contacted, even by an accelerating observer. One of the best-known examples of an event horizon derives from general relativity's description of a black hole, a celestial object so dense that no nearby matter or radiation can escape its gravitational field.
Often, this is described as the boundary within which the black hole's escape velocity is greater than the speed of light. However, a more detailed description is that within this horizon, all lightlike paths paths that light could take and hence all paths in the forward light cones of particles within the horizon, are warped so as to fall farther into the hole.
Once a particle is inside the horizon, moving into the hole is as inevitable as moving forward in time - no matter what direction the particle is traveling, and can actually be thought of as equivalent to doing so, depending on the spacetime coordinate system used.
The surface at the Schwarzschild radius acts as an event horizon in a non-rotating body that fits inside this radius although a rotating black hole operates slightly differently.
The Schwarzschild radius of an object is proportional to its mass. Theoretically, any amount of matter will become a black hole if compressed into a space that fits within its corresponding Schwarzschild radius.
For the mass of the Sun this radius is approximately 3 kilometers and for the Earth it is about 9 millimeters. In practice, however, neither the Earth nor the Sun have the necessary mass and therefore the necessary gravitational force, to overcome electron and neutron degeneracy pressure.
The minimal mass required for a star to be able to collapse beyond these pressures is the Tolman—Oppenheimer—Volkoff limit , which is approximately three solar masses.
According to the fundamental gravitational collapse models,  an event horizon forms before the singularity of a black hole. If all the stars in the Milky Way would gradually aggregate towards the galactic center while keeping their proportionate distances from each other, they will all fall within their joint Schwarzschild radius long before they are forced to collide.
Black hole event horizons are widely misunderstood. Common, although erroneous, is the notion that black holes "vacuum up" material in their neighborhood, where in fact they are no more capable of seeking out material to consume than any other gravitational attractor.
As with any mass in the universe, matter must come within its gravitational scope for the possibility to exist of capture or consolidation with any other mass.
Equally common is the idea that matter can be observed falling into a black hole. This is not possible. Astronomers can detect only accretion disks around black holes, where material moves with such speed that friction creates high-energy radiation which can be detected similarly, some matter from these accretion disks is forced out along the axis of spin of the black hole, creating visible jets when these streams interact with matter such as interstellar gas or when they happen to be aimed directly at Earth.
Furthermore, a distant observer will never actually see something reach the horizon. Instead, while approaching the hole, the object will seem to go ever more slowly, while any light it emits will be further and further redshifted.
The black hole event horizon is teleological in nature, meaning that we need to know the entire future space-time of the universe to determine the current location of the horizon, which is essentially impossible.
Because of the purely theoretical nature of the event horizon boundary, the traveling object does not necessarily experience strange effects and does, in fact, pass through the calculatory boundary in a finite amount of proper time.
A misconception concerning event horizons, especially black hole event horizons, is that they represent an immutable surface that destroys objects that approach them.
In practice, all event horizons appear to be some distance away from any observer, and objects sent towards an event horizon never appear to cross it from the sending observer's point of view as the horizon-crossing event's light cone never intersects the observer's world line.
Attempting to make an object near the horizon remain stationary with respect to an observer requires applying a force whose magnitude increases unboundedly becoming infinite the closer it gets.
In the case of the horizon around a black hole, observers stationary with respect to a distant object will all agree on where the horizon is.
While this seems to allow an observer lowered towards the hole on a rope or rod to contact the horizon, in practice this cannot be done.
The proper distance to the horizon is finite,  so the length of rope needed would be finite as well, but if the rope were lowered slowly so that each point on the rope was approximately at rest in Schwarzschild coordinates , the proper acceleration G-force experienced by points on the rope closer and closer to the horizon would approach infinity, so the rope would be torn apart.
If the rope is lowered quickly perhaps even in freefall , then indeed the observer at the bottom of the rope can touch and even cross the event horizon.
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Weir briefly hallucinates Justin turning into his late wife, who stares at him despite her notable lack of eyes. Get the best of Den of Geek delivered right to your inbox!
The special edition DVD managed to find a couple of deleted moments, including a briefing scene establishing the re-emergence of the Event Horizon.5/19/ · Released in , Paul W.S. Anderson's hellish space horror flick Event Horizon is a favorite of ours here on Bloody Disgusting, and we know we're not alon Uncut. 7/22/ · The Hell Scenes From 'Event Horizon' Slowed Way Down 2 diggs Movies Video. Hey, do you have nightmares? Would you like more? Well then step right up and watch a slowed-down version of the cult-film "Event Horizon." The original version still haunts our dreams, almost two decades later. I tell my friends that Event Horizon is the first film set in the Warhammer 40k universe. This is what happens when ships spend too much time in the Warp. level 2. 15 points · 7 years ago. I tell my friends the same thing. The movie is infinitely better when cast in that light. It also doesn't help when the ship returns with an active portal.