Event Horizon ist ein Spiel von Pavel Zinchenko, das von Drageus Games Switch, die USK (Unterhaltungssoftware-Selbstkontrolle) hat dem Game noch keine. Du wirst angegriffen! Dieses Hardcore-Spiel, das im fesselnden Event-Horizon-Universum angesiedelt ist, lässt dich eine Weltraum-Flotte. Event Horizon Games – Garner Station Blvd, Raleigh – Mit bewertet, basierend auf Bewertungen „I drive almost two hours to come here..
Event Horizon - Frontier kaufenEvent Horizon ist ein Spiel von Pavel Zinchenko, das von Drageus Games Switch, die USK (Unterhaltungssoftware-Selbstkontrolle) hat dem Game noch keine. Event Horizon Kampf Flotten: Raumschiff VS Alien ist ein episches Actionspiel im Weltraum, bei dem Spieler die Kontrolle über ihre Raumflotte. Über dieses Spiel. Event Horizon: Frontier is a base defense game set in the Event Horizon universe. Defend your space station from aliens from.
Event Horizon Game About This Game VideoGX Gaming - Doom 3 Mod - Event Horizon XV
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Create widget. Popular user-defined tags for this product:? Sign In Sign in to add your own tags to this product. 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". 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.
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