Event Horizon - Am Rande des Universums Trailer & Teaser, Interviews, Clips und mehr Videos auf Deutsch und im Original. Schaue dir alle 3 Videos jetzt an! Event Horizon – Am Rande des Universums: lauert eine scheinbar unbezwingbare Gefahr. Düsterer Sprachen: Deutsch, Englisch (OV). Mieten SD €. Event Horizon - Am Rande des Universums ein Film von Paul W.S. Anderson mit Jetzt auch auf Deutsch: Neuer Trailer zu "Halloween Kills" zeigt gleich 3.
Event Horizon Trailer Deutsch Inhaltsverzeichnis
Weir erläutert erst nach der Ankunft Captain Miller und dessen Mannschaft das Ziel des Unternehmens: Sie sollen die Event Horizon (deutsch: Ereignishorizont). Video 1 von 3 zur Serie: Event Horizon - Trailer (Deutsch) jetzt anschauen! Event Horizon - Am Rande des Universums Trailer & Teaser, Interviews, Clips und mehr Videos auf Deutsch und im Original. Schaue dir alle 3 Videos jetzt an! Event Horizon – Am Rande des Universums: lauert eine scheinbar unbezwingbare Gefahr. Düsterer Sprachen: Deutsch, Englisch (OV). Mieten SD €. Event Horizon - Am Rande des Universums ein Film von Paul W.S. Anderson mit Jetzt auch auf Deutsch: Neuer Trailer zu "Halloween Kills" zeigt gleich 3. Event Horizon - Trailer (Fantrailer) deutsch HD - YouTubeYour browser indicates if you've visited this linkhttps youtube com/watch?v=PMf2HW8Gr50Event. Event Horizon - Am Rande des Universums (Event Horizon): Science-Fiction-Film/Horrorfilm/Monsterfilm/Alien-Horrorfilm von Lawrence.
Event Horizon - Am Rande des Universums (Event Horizon): Science-Fiction-Film/Horrorfilm/Monsterfilm/Alien-Horrorfilm von Lawrence. Event Horizon - Trailer (Fantrailer) deutsch HD - YouTubeYour browser indicates if you've visited this linkhttps youtube com/watch?v=PMf2HW8Gr50Event. Weir erläutert erst nach der Ankunft Captain Miller und dessen Mannschaft das Ziel des Unternehmens: Sie sollen die Event Horizon (deutsch: Ereignishorizont). Folglich ist der Engländer also durchaus nicht untalentiert, wenn er allerdings mit einer — wie so oft — dürftigen Geschichte Schon mindestens Honeymooners mal habe ich mir diesen Film angesehen und ich hatte erneut Lust Frau Weiß mir zu Gemüte zu führen. Weir, wurden nur drei Monate nach Premiere des Films in einer Folge 4. Das könnte Heinz Emigholz auch interessieren. Seitenverhältnis 2.
Under these conditions, an apparent horizon is present in the particle's accelerating reference frame, representing a boundary beyond which events are unobservable.
For example, this occurs with a uniformly accelerated particle. A spacetime diagram of this situation is shown in the figure to the right.
As the particle accelerates, it approaches, but never reaches, the speed of light with respect to its original reference frame.
On the spacetime diagram, its path is a hyperbola , which asymptotically approaches a degree line the path of a light ray.
An event whose light cone's edge is this asymptote or is farther away than this asymptote can never be observed by the accelerating particle.
In the particle's reference frame, there is a boundary behind it from which no signals can escape an apparent horizon. While approximations of this type of situation can occur in the real world [ citation needed ] in particle accelerators , for example , a true event horizon is never present, as this requires the particle to be accelerated indefinitely requiring arbitrarily large amounts of energy and an arbitrarily large apparatus.
In the case of a horizon perceived by a uniformly accelerating observer in empty space, the horizon seems to remain a fixed distance from the observer no matter how its surroundings move.
Varying the observer's acceleration may cause the horizon to appear to move over time, or may prevent an event horizon from existing, depending on the acceleration function chosen.
The observer never touches the horizon and never passes a location where it appeared to be. In the case of a horizon perceived by an occupant of a de Sitter universe , the horizon always appears to be a fixed distance away for a non-accelerating observer.
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.
But once this happens it is impossible to pull the bottom of rope back out of the event horizon, since if the rope is pulled taut, the forces along the rope increase without bound as they approach the event horizon and at some point the rope must break.
Furthermore, the break must occur not at the event horizon, but at a point where the second observer can observe it. Assuming that the possible apparent horizon is far inside the event horizon, or there is none, observers crossing a black hole event horizon would not actually see or feel anything special happen at that moment.
In terms of visual appearance, observers who fall into the hole perceive the eventual apparent horizon as a black impermeable area enclosing the singularity.
Increasing tidal forces are also locally noticeable effects, as a function of the mass of the black hole. In realistic stellar black holes , spaghettification occurs early: tidal forces tear materials apart well before the event horizon.
However, in supermassive black holes , which are found in centers of galaxies, spaghettification occurs inside the event horizon.
A human astronaut would survive the fall through an event horizon only in a black hole with a mass of approximately 10, solar masses or greater.
A cosmic event horizon is commonly accepted as a real event horizon, whereas the description of a local black hole event horizon given by general relativity is found to be incomplete and controversial.
At present, it is expected by the Hawking radiation mechanism that the primary impact of quantum effects is for event horizons to possess a temperature and so emit radiation.
For black holes , this manifests as Hawking radiation , and the larger question of how the black hole possesses a temperature is part of the topic of black hole thermodynamics.
For accelerating particles, this manifests as the Unruh effect , which causes space around the particle to appear to be filled with matter and radiation.
According to the controversial black hole firewall hypothesis, matter falling into a black hole would be burned to a crisp by a high energy "firewall" at the event horizon.
An alternative is provided by the complementarity principle , according to which, in the chart of the far observer, infalling matter is thermalized at the horizon and reemitted as Hawking radiation, while in the chart of an infalling observer matter continues undisturbed through the inner region and is destroyed at the singularity.
This hypothesis does not violate the no-cloning theorem as there is a single copy of the information according to any given observer.
Black hole complementarity is actually suggested by the scaling laws of strings approaching the event horizon, suggesting that in the Schwarzschild chart they stretch to cover the horizon and thermalize into a Planck length -thick membrane.
A complete description of local event horizons generated by gravity is expected to, at minimum, require a theory of quantum gravity. One such candidate theory is M-theory.
Another such candidate theory is loop quantum gravity. From Wikipedia, the free encyclopedia. For other uses, see Event horizon disambiguation and Horizon general relativity.
A region in spacetime from which nothing can escape. Introduction History. Fundamental concepts. Principle of relativity Theory of relativity Frame of reference Inertial frame of reference Rest frame Center-of-momentum frame Light cone Equivalence principle Mass—energy equivalence Special relativity Doubly special relativity de Sitter invariant special relativity Scale relativity World line Proper time Riemannian geometry Energy condition.
Equations Formalisms. Main article: Cosmological horizon. See also: Hyperbolic motion relativity. Main article: Black hole. Physics portal. January General Relativity and Gravitation.
Bibcode : GReGr.. Weir shoots at him and is blown into space by the ensuing decompression. Miller, Starck, and Cooper survive and manage to seal off the ship's bridge.
With their own ship destroyed, Miller plans to split the Event Horizon in two and use the forward section of the ship as a lifeboat. He is attacked by manifestations of Corrick which turns out to be the resurrected Dr.
Miller fights them off and detonates the explosives, sacrificing himself. The gravity drive activates, pulling the ship's stern section into a black hole.
Starck and Cooper enter stasis beside a comatose Justin, and wait to be rescued. Seventy-two days later, the wreckage of the Event Horizon is boarded by a rescue party, who discover the remaining crew still in stasis.
Starck sees Weir posing as one of the rescuers and screams in terror; this is revealed to be a nightmare with Starck waking up moments later.
Cooper and the rescue team comfort the newly-awakened and terrified Starck as the bulkheads close. Anderson was inundated with screenplay offers, as well as the opportunity to direct the Mortal Kombat sequel Mortal Kombat: Annihilation ,  and the upcoming X-Men Anderson had in mind a "classic haunted house movie", incorporating significant influences to moderately successful horror films such as Robert Wise 's The Haunting and Kubrick 's The Shining because they enforce suspense from the unknown, meaning the ghost or creature was hidden from the viewer, and their endings induced ambiguities of perception in the audience.
Screenwriter Philip Eisner acknowledged Warhammer 40, as a major inspiration for the plot. Many fans of Warhammer 40, consider Event Horizon to be an unofficial prequel to the former, when humankind discovers the Warp and learns of its dangers the hard way.
As Anderson explains, directors usually have a standard week editing period to produce the first cut of a film, as guaranteed by the Directors Guild of America.
However, due to the short production schedule of the film, the rapidly approaching release date, and the fact that principal photography had not yet finished, Anderson agreed with the Paramount studio to an editing period of six weeks and promised to deliver the film by August , as Paramount wanted to have a hit film before Titanic's planned September release date.
When the main unit wrapped, Anderson was supposed to start editing the film, but he still had to shoot two weeks with the second unit , effectively shortening the time he could spend in post-production to just four weeks.
In that short amount of time, only a rough cut of the film could be assembled. Anderson notes that at two hours and 10 minutes, it was overly long, with weak directing and acting that could have used another editing pass, unfinished special effects, and a poor sound mix.
In test screenings , the cut was poorly received. There were complaints about the extreme amount of gore,  and Anderson and producer Jeremy Bolt claim members of the test audience fainted during the screening.
Anderson believes that while his first cut was justifiably considered too long, Paramount forced him to make a cut that was instead too short, and that the film would benefit by the restoration of around 10 minutes of footage, including some of the deleted gore.
After the initial DVD release became a surprise hit, the studio and Anderson became interested in assembling a director's cut , but they quickly discovered that the excised footage had not been carefully stored and much of it had gone missing.
The plan to assemble a director's cut was abandoned and instead a special-edition two-DVD set was released, featuring one deleted scene, two extended scenes, and a few shots of deleted material in the included making-of featurette.
The footage is of " video " quality. The "bloody orgy" video was also longer. As Anderson was sometimes too busy filming other scenes, second-unit director Vadim Jean filmed some parts of this scene.
The film's final ending was a combination of two unused alternate endings that were filmed. One did not have a jump scare at the end when the last two survivors are found by another rescue crew and Starck hallucinates that she sees Weir, although there was a similar version of the scene included in this ending where she hears screams of Event Horizon crew and screams in fear before Cooper wakes her up.
This was the original ending of the film included in the shooting script. He responded "never", explaining that much of it is gone forever. Anderson said that after finishing Resident Evil: Retribution , he planned to watch it for the first time since assembling the film.
Asked about the VHS tape, he said neither he, nor Levin, had watched it yet, as Levin moved to Spain; however, he was still excited about watching it at some point.
Michael Kamen was hired to compose the score for the film. Director Paul W. Anderson , a fan of hybrid genre music, invited the electronic dance music duo Orbital to collaborate with Kamen and to provide synthesizing sounds for the film's unsettling atmosphere.
A soundtrack album was released which edited various cues from the score into four tracks of approximately ten minutes.
Event Horizon was released on August 15, and was a box office failure. Roger Ebert gave the film two stars out of four, noting the opening portion as being particularly well-crafted, and commended its atmosphere.
However, Ebert went on to state that the film never managed to become the intense, thought-provoking experience it wanted to be.
The film had some early supporters, with Empire magazine awarding Event Horizon a 3 out of 5 stars rating, reporting: "That the film never fulfils its promise is down to its over reliance on horror vagaries in a precision-built sci-fi milieu, ultimately leaving too many unanswered queries.
A sharper script and a more credible solution could have turned this impressive hokum into a force to be reckoned with". There are certainly plenty of jumps on offer as a possessed ship torments and tortures any humans it can find.
Well worth a look. In August , it was reported that Paramount Television and Amazon Studios were developing a television series based on Event Horizon.
Horror filmmaker Adam Wingard is set to executive produce and possibly direct the series. Lawrence Gordon and Lloyd Levin, who produced the original film, are also involved.
From Wikipedia, the free encyclopedia. Redirected from Event Horizon movie. Theatrical release poster. Michael Kamen. Release date. Running time. This section needs expansion.
You can help by adding to it. June British Film Institute. Retrieved 11 February British Board of Film Classification. The Numbers. Retrieved 18 August Box Office Mojo.
Retrieved 16 July Anderson Director , Jeremy Bolt Producer Event Horizon Audio commentary. Paramount Home Entertainment.
Paul W. Den of Geek!